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Error code: DatasetGenerationError
Exception: TypeError
Message: Couldn't cast array of type
struct<temporalExtentStart: string, daac: string, temporalFrequency: string, cmrId: string, temporalExtentEnd: string, globalId: string, abstract: string, shortName: string, longName: string, doi: string, year: string, title: string, authors: string, Type: string, url: string>
to
{'temporalExtentStart': Value('string'), 'daac': Value('string'), 'temporalFrequency': Value('string'), 'cmrId': Value('string'), 'temporalExtentEnd': Value('string'), 'globalId': Value('string'), 'abstract': Value('string'), 'shortName': Value('string'), 'doi': Value('string'), 'longName': Value('string')}
Traceback: Traceback (most recent call last):
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/builder.py", line 1831, in _prepare_split_single
writer.write_table(table)
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/arrow_writer.py", line 714, in write_table
pa_table = table_cast(pa_table, self._schema)
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/table.py", line 2272, in table_cast
return cast_table_to_schema(table, schema)
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/table.py", line 2224, in cast_table_to_schema
cast_array_to_feature(
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/table.py", line 1795, in wrapper
return pa.chunked_array([func(chunk, *args, **kwargs) for chunk in array.chunks])
^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/table.py", line 2092, in cast_array_to_feature
raise TypeError(f"Couldn't cast array of type\n{_short_str(array.type)}\nto\n{_short_str(feature)}")
TypeError: Couldn't cast array of type
struct<temporalExtentStart: string, daac: string, temporalFrequency: string, cmrId: string, temporalExtentEnd: string, globalId: string, abstract: string, shortName: string, longName: string, doi: string, year: string, title: string, authors: string, Type: string, url: string>
to
{'temporalExtentStart': Value('string'), 'daac': Value('string'), 'temporalFrequency': Value('string'), 'cmrId': Value('string'), 'temporalExtentEnd': Value('string'), 'globalId': Value('string'), 'abstract': Value('string'), 'shortName': Value('string'), 'doi': Value('string'), 'longName': Value('string')}
The above exception was the direct cause of the following exception:
Traceback (most recent call last):
File "/src/services/worker/src/worker/job_runners/config/parquet_and_info.py", line 1455, in compute_config_parquet_and_info_response
parquet_operations = convert_to_parquet(builder)
^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/src/worker/job_runners/config/parquet_and_info.py", line 1054, in convert_to_parquet
builder.download_and_prepare(
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/builder.py", line 894, in download_and_prepare
self._download_and_prepare(
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/builder.py", line 970, in _download_and_prepare
self._prepare_split(split_generator, **prepare_split_kwargs)
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/builder.py", line 1702, in _prepare_split
for job_id, done, content in self._prepare_split_single(
^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/.venv/lib/python3.12/site-packages/datasets/builder.py", line 1858, in _prepare_split_single
raise DatasetGenerationError("An error occurred while generating the dataset") from e
datasets.exceptions.DatasetGenerationError: An error occurred while generating the datasetNeed help to make the dataset viewer work? Make sure to review how to configure the dataset viewer, and open a discussion for direct support.
type
string | id
string | labels
list | properties
dict |
|---|---|---|---|
node
|
0
|
[
"Dataset"
] |
{
"temporalExtentStart": "1992-01-01T00:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2617226208-POCLOUD",
"temporalExtentEnd": "1996-05-17T23:59:59.000Z",
"globalId": "dcf602c1-0e51-55f1-97fb-dbfb8a704c0f",
"abstract": "This European Remote Sensing (ERS) Sigma-0 dataset is generated by the Scatterometer Climate Record Pathfinder (SCP) project at Brigham Young University (BYU) and is generated using a Scatterometer Image Reconstruction (SIR) technique developed by Dr. David Long at BYU. The dataset provides SIR processed Sigma-0 data from the ERS-1 C-band scatterometer, which is also known as the Active Microwave Instrument (AMI). AMI is a multimode radar operating at a frequency of 5.3 GHz (C-band), using vertically polarized antennas for both transmission and reception. The SIR technique results in an enhanced resolution image reconstruction and gridded on an equal-area grid (for non-polar regions) at 8.9 km pixel resolution stored in SIR files; polar regions are gridded at the same resolution using a polar-stereographic technique. A non-enhanced version is provided at 44.5 km pixel resolution in a format known as GRD (i.e., gridded) files. All files are produced in IEEE formatted binary. All data files are separated and organized by region, parameter, and sampling technique (i.e., SIR vs. GRD). The regions of China and Japan are combined into a single region. In addition to Sigma-0, various statistical parameters are provided for added guidance, including but not limited to: standard deviation, measurement counts, pixel time, Sigma-0 error, and average incidence angle. This dataset was once distributed on tape, but has been made available on FTP thanks to the BYU SCP.",
"shortName": "ERS-1_BYU_L3_OW_SIGMA0_ENHANCED",
"longName": "ERS-1 Gridded Level 3 Enhanced Resolution Sigma-0 from BYU",
"doi": "10.5067/ERS1B-SNEN0"
}
|
node
|
1
|
[
"Dataset"
] |
{
"temporalExtentStart": "1996-09-15T00:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2617226510-POCLOUD",
"temporalExtentEnd": "1997-06-29T23:59:59.999Z",
"globalId": "592102e7-47ed-52f0-bde4-7a9bfa18ed5b",
"abstract": "This NASA Scatterometer (NSCAT) satellite Sigma-0 dataset is generated by the Scatterometer Climate Record Pathfinder (SCP) project at Brigham Young University (BYU) and is generated using a Scatterometer Image Reconstruction (SIR) technique developed by Dr. David Long. The SIR technique results in an enhanced resolution image reconstruction and gridded on an equal-area grid (for non-polar regions) at 4.45 km pixel resolution stored in SIR files; polar regions are gridded using a polar-stereographic technique. A non-enhanced version is provided at 22.25 km pixel resolution in a format known as GRD files. All files are produced in IEEE formatted binary. All data files are separated and organized by region, polarization, parameter, and sampling technique (i.e., SIR vs. GRD). The regions of China and Japan are combined into a single region. In additional to Sigma-0, various statistical parameters are provided for added guidance, including but not limited to: standard deviation, measurement counts, pixel time, Sigma-0 error, and average incidence angle. For more information, please visti: http://www.scp.byu.edu/docs/NSCAT_user_notes.html",
"shortName": "NSCAT_BYU_L3_OW_SIGMA0_ENHANCED",
"longName": "NSCAT Gridded Level 3 Enhanced Resolution Sigma-0 from BYU",
"doi": "10.5067/NSBYU-SNEN0"
}
|
node
|
2
|
[
"Dataset"
] |
{
"temporalExtentStart": "1996-06-03T00:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2617226211-POCLOUD",
"temporalExtentEnd": "2001-12-30T23:59:59.000Z",
"globalId": "9fa7db56-a9a2-5313-949e-4b30a3a2fbbf",
"abstract": "This European Remote Sensing (ERS) Sigma-0 dataset is generated by the Scatterometer Climate Record Pathfinder (SCP) project at Brigham Young University (BYU) and is generated using a Scatterometer Image Reconstruction (SIR) technique developed by Dr. David Long at BYU. The dataset provides SIR processed Sigma-0 data from the ERS-2 C-band scatterometer, which is also known as the Active Microwave Instrument (AMI). AMI is a multimode radar operating at a frequency of 5.3 GHz (C-band), using vertically polarized antennas for both transmission and reception. The SIR technique results in an enhanced resolution image reconstruction and gridded on an equal-area grid (for non-polar regions) at 8.9 km pixel resolution stored in SIR files; polar regions are gridded at the same resolution using a polar-stereographic technique. A non-enhanced version is provided at 44.5 km pixel resolution in a format known as GRD (i.e., gridded) files. All files are produced in IEEE formatted binary. All data files are separated and organized by region, parameter, and sampling technique (i.e., SIR vs. GRD). The regions of China and Japan are combined into a single region. In addition to Sigma-0, various statistical parameters are provided for added guidance, including but not limited to: standard deviation, measurement counts, pixel time, Sigma-0 error, and average incidence angle. This dataset was once distributed on tape, but has been made available on FTP thanks to the BYU SCP. For more information, please visit: http://www.scp.byu.edu/docs/ERS_user_notes.html",
"shortName": "ERS-2_BYU_L3_OW_SIGMA0_ENHANCED",
"longName": "ERS-2 Gridded Level 3 Enhanced Resolution Sigma-0 from BYU",
"doi": "10.5067/ERS2B-SNEN0"
}
|
node
|
3
|
[
"Dataset"
] |
{
"temporalExtentStart": "2013-08-01T13:09:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "hourly",
"cmrId": "C2499940523-POCLOUD",
"temporalExtentEnd": "2018-01-08T15:29:19.000Z",
"globalId": "99f70249-9d33-5647-8c57-e933c124e2e1",
"abstract": "The Geostationary Operational Environmental Satellites (GOES) operated by the United States National Oceanic and Atmospheric Administration (NOAA) support weather forecasting, severe storm tracking, meteorology and oceanography research. Generally there are several GOES satellites in geosynchronous orbit at any one time viewing different earth locations including the GOES-13 launched 24 May 2006. The radiometer aboard the satellite, The GOES N-P Imager, is a five channel (one visible, four infrared) imaging radiometer designed to sense radiant and solar reflected energy from sampled areas of the earth. The multi-element spectral channels simultaneously sweep east-west and west-east along a north-to-south path by means of a two-axis mirror scan system retuning telemetry in 10-bit precision. For this Group for High Resolution Sea Surface Temperature (GHRSST) dataset, skin sea surface temperature (SST) measurements are calculated from the far IR channels of GOES-13 at full resolution on a half hourly basis. In native satellite projection, vertically adjacent pixels are averaged and read out at every pixel. L2P datasets including Single Sensor Error Statistics (SSES) are then derived following the GHRSST Data Processing Specification (GDS) version 2.0. The full disk image is subsetted into granules representing distinct northern and southern regions.",
"shortName": "GOES13-OSPO-L2P-v1.0",
"longName": "GHRSST Level 2P Western Atlantic Regional Skin Sea Surface Temperature from the Geostationary Operational Environmental Satellites (GOES) Imager on the GOES-13 satellite (GDS version 2)",
"doi": "10.5067/GHG13-2PO02"
}
|
node
|
4
|
[
"Dataset"
] |
{
"temporalExtentStart": "2013-08-01T09:32:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "hourly",
"cmrId": "C2499940520-POCLOUD",
"temporalExtentEnd": "2015-12-04T11:15:00.000Z",
"globalId": "52ee160f-d9ad-5481-8196-b475c3da166a",
"abstract": "Multi-functional Transport Satellites (MTSAT) are a series of geostationary weather satellites operated by the Japan Meteorological Agency (JMA). MTSAT carries an aeronautical mission to assist air navigation, plus a meteorological mission to provide imagery over the Asia-Pacific region for the hemisphere centered on 140 East. The meteorological mission includes an imager giving nominal hourly full Earth disk images in five spectral bands (one visible, four infrared). MTSAT are spin stabilized satellites. With this system images are built up by scanning with a mirror that is tilted in small successive steps from the north pole to south pole at a rate such that on each rotation of the satellite an adjacent strip of the Earth is scanned. It takes about 25 minutes to scan the full Earth's disk. This builds a picture 10,000 pixels for the visible images (1.25 km resolution) and 2,500 pixels (4 km resolution) for the infrared images. The MTSAT-2 (also known as Himawari 7) and its radiometer (MTSAT-2 Imager) was successfully launched on 18 February 2006. For this Group for High Resolution Sea Surface Temperature (GHRSST) dataset, skin sea surface temperature (SST) measurements are calculated from the IR channels of the MTSAT-2 Imager full resolution data in satellite projection on a hourly basis by using Bayesian Cloud Mask algorithm at the Office of Satellite and Product Operations (OSPO). L2P datasets including Single Sensor Error Statistics (SSES) are then derived following the GHRSST Data Processing Specification (GDS) version 2.0.",
"shortName": "MTSAT2-OSPO-L2P-v1.0",
"longName": "GHRSST Level 2P Western Pacific Regional Skin Sea Surface Temperature from the Multifunctional Transport Satellite 2 (MTSAT-2) (GDS version 2)",
"doi": "10.5067/GHMT2-2PO02"
}
|
node
|
5
|
[
"Dataset"
] |
{
"temporalExtentStart": "2010-01-01T14:30:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2499940522-POCLOUD",
"temporalExtentEnd": "2017-12-14T15:30:01.000Z",
"globalId": "2af067fb-a040-5e22-9d3e-f25267c07af0",
"abstract": "A regional Group for High Resolution Sea Surface Temperature (GHRSST) Level 3 Collated (L3C) dataset for the America Region (AMERICAS) based on retrievals from the GOES-13 Imager on board GOES-13 satellite. The European Organization for the Exploitation of Meteorological Satellites (EUMETSAT),Ocean and Sea Ice Satellite Application Facility (OSI SAF) is producing SST products in near realtime from GOES 13 in East position. GOES 13 imager level 1 data are acquired at Meteo-France/Centre de Meteorologie Spatiale (CMS) through the EUMETSAT/EUMETCAST system.SST is retrieved from the GOES 13 infrared channels (3.9 and 10.8 micrometer) using a multispectralalgorithm. Due to the lack of 12 micrometer channel in the GOES 13 imager, SST retrieval is not possiblein daytime conditions. Atmospheric profiles of water vapor and temperature from a numericalweather prediction model, together with a radiatiave transfer model, are used to correct themultispectral algorithm for regional and seasonal biases due to changing atmospheric conditions.Every 30 minutes slot is processed at full satellite resolution. The operational products are thenproduced by remapping over a 0.05 degree regular grid (60S-60N and 135W-15W) SST fieldsobtained by aggregating 30 minute SST data available in one hour time, and the priority beinggiven to the value the closest in time to the product nominal hour. The product format is compliantwith the GHRSST Data Specification (GDS) version 2.",
"shortName": "GOES13-OSISAF-L3C-v1.0",
"longName": "GHRSST Level 3C sub-skin Sea Surface Temperature from the Geostationary Operational Environmental Satellites (GOES 13) Imager in East position (GDS V2) produced by OSI SAF",
"doi": "10.5067/GHG13-3CO01"
}
|
node
|
6
|
[
"Dataset"
] |
{
"temporalExtentStart": "2013-06-04T10:25:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2491735309-POCLOUD",
"temporalExtentEnd": "2016-11-23T11:52:04.000Z",
"globalId": "e5807c1a-4ed8-5e4b-a749-372104676cac",
"abstract": "A global 1 km Group for High Resolution Sea Surface Temperature (GHRSST) Level 2P dataset based on multi-channel sea surface temperature (SST) retrievals generated in real-time from the Advanced Very High Resolution Radiometer (AVHRR) on the European Meteorological Operational-A (MetOp-A)satellite (launched 19 Oct 2006). The European Organization for the Exploitation of Meteorological Satellites (EUMETSAT),Ocean and Sea Ice Satellite Application Facility (OSI SAF) is producing SST products in near realtime from Metop/AVHRR. Global AVHRR level 1b data are acquired at Meteo-France/Centre deMeteorologie Spatiale (CMS) through the EUMETSAT/EUMETCAST system. SST is retrievedfrom the AVHRR infrared channels (3.7, 10.8 and 12.0 micrometer) using a multispectral algorithm.Atmospheric profiles of water vapor and temperature from a numerical weather prediction model,together with a radiatiave transfer model, are used to correct the multispectral algorithm forregional and seasonal biases due to changing atmospheric conditions. This product is delivered atfull resolution in satellite projection as metagranule corresponding to 3 minutes of acquisition. Theproduct format is compliant with the GHRSST Data Specification (GDS) version 2.",
"shortName": "AVHRR_SST_METOP_A-OSISAF-L2P-v1.0",
"longName": "GHRSST Level 2P sub-skin Sea Surface Temperature from the Advanced Very High Resolution Radiometer (AVHRR) on Metop satellites (currently Metop-A) (GDS V2) produced by OSI SAF",
"doi": "10.5067/GHAMA-2PO02"
}
|
node
|
7
|
[
"Dataset"
] |
{
"temporalExtentStart": "2019-05-14T18:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2491772160-POCLOUD",
"temporalExtentEnd": "2019-10-11T18:30:01.000Z",
"globalId": "ec4120b7-6e96-5d2f-a370-b8c3c906517e",
"abstract": "The Saildrone Arctic 2019 dataset presents a unique collection of high-quality, near real-time, multivariate surface ocean, and atmospheric observations obtained through the deployment of Saildrone, an innovative wind and solar-powered uncrewed surface vehicle (USV). Saildrone is capable of extended missions lasting up to 12 months, covering vast distances at typical speeds of 3-5 knots and operates autonomously, relying solely on wind propulsion, while its navigation can be remotely guided from land. The 2019 Saildrone Arctic campaign featured six Saildrone USVs (jointly funded by NOAA and NASA) deployed during a 150-day cruise in the Bering and Chukchi Seas, spanning from 14 May 2019 to 11 October 2019. The primary mission objective for 2019 was to gather comprehensive atmospheric and oceanographic data in Alaskan arctic waters, which could lead to significant improvements in modeling of diurnal warming and understanding of the marginal ice zones. Additionally, these new data will provide additional Arctic SST observations to benefit SST algorithm development and validation, and for studies of air- sea-ice interactions. Please see the cruise report: https://archive.podaac.earthdata.nasa.gov/podaac-ops-cumulus-docs/insitu/open/L2/saildrone/docs/Saildrone_2019_Arctic_Cruise_Report.pdf <p>\rDuring the Arctic campaign, NASA-funded Saildrones SD-1036 and SD-1037 undertook transects in the Chukchi Sea, approaching the sea ice edge to measure air-sea heat and momentum fluxes in the ocean near sea ice and to validate satellite sea-surface temperature measurements in the Arctic. Each Saildrone was equipped with a suite of instruments to measure various parameters, including air temperature, relative humidity, barometric pressure, surface skin temperature, wind speed and direction, wave height and period, seawater temperature and salinity, chlorophyll fluorescence, and dissolved oxygen. Additionally, both vehicles utilized 300 kHz acoustic Doppler current profilers (ADCP) to measure near-surface currents. Seven temperature data loggers positioned vertically along the hull enhanced understanding of thermal variability near the ocean surface.<p>\rThe Saildrone Arctic 2019 dataset, part of the Multi-sensor Improved Sea-Surface Temperature (MISST) project, encompasses three netCDF format files for each deployed Saildrone. The first file integrates saildrone platform telemetry and surface observational data at 1-minute temporal resolution including key parameters such as air temperature, sea surface skin, and bulk temperatures, salinity, oxygen and chlorophyll-a concentrations, barometric pressure, and wind speed and direction. The second file focuses on ADCP current vector data, providing depth-resolved information to 100m at 2m intervals and binned temporally at 5-minute resolution. The third file includes temperature logger measurements at various depths at 1-minute resolution. This project, funded by NASA through the National Ocean Partnership Program (NOPP), demonstrates a commitment to advancing scientific understanding of the Arctic environment through innovative and autonomous observational technologies. \r",
"shortName": "SAILDRONE_ARCTIC",
"longName": "Saildrone Arctic field campaign surface and ADCP measurements for NOPP-MISST project",
"doi": "10.5067/SDRON-NOPP0"
}
|
node
|
8
|
[
"Dataset"
] |
{
"temporalExtentStart": "2020-01-17T00:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2491772162-POCLOUD",
"temporalExtentEnd": "2020-03-02T23:59:59.000Z",
"globalId": "4a26c4bc-222a-5c74-b989-9cf4edb6b4d6",
"abstract": "Saildrone is a wind and solar powered unmanned surface vehicle (USV) capable of long distance deployments lasting up to 12 months and providing high quality, near real-time, multivariate surface ocean and atmospheric observations while transiting at typical speeds of 3-5 knots. The drone is autonomous in that it may be guided remotely from land while being completely wind driven. The saildrone ATOMIC (Atlantic Tradewind Ocean-Atmosphere Mesoscale Interaction Campaign) campaign involved the deployment of a fleet of saildrones, jointly funded by NASA and NOAA, in the Atlantic waters offshore of Barbados over a 45 day period from 17 January to 2 March 2020. The goal was to understand the Ocean-Atmosphere interaction particularly over the mesoscale ocean eddies in that region. The saildrones were equipped with a suite of instruments that included a CTD, IR pyrometer, fluorometer, dissolved oxygen sensor, anemometer, barometer, and Acoustic Doppler Current Profiler (ADCP). Additionally, four temperature data loggers were positioned vertically along hull to provide further information on thermal variability near the ocean surface. This Saildrone ATOMIC dataset is comprised of two data files for each of the three NASA-funded saildrones deployed, one for the surface observations and one for the ADCP measuements. The surface data files contain saildrone platform telemetry and near-surface observational data (air temperature, sea surface skin and bulk temperatures, salinity, oxygen and chlorophyll-a concentrations, barometric pressure, wind speed and direction) spanning the entire cruise at 1 minute temporal resolution. The ADCP files for each saildrone are at 5 minute resolution for the duration of the deployments. All data files are in netCDF format and CF/ACDD compliant consistent with the NOAA/NCEI specification.",
"shortName": "SAILDRONE_ATOMIC",
"longName": "Saildrone field campaign surface and ADCP measurements for the Atlantic Tradewind Ocean-Atmosphere Mesoscale Interaction Campaign (ATOMIC) project",
"doi": "10.5067/SDRON-ATOM0"
}
|
node
|
9
|
[
"Dataset"
] |
{
"temporalExtentStart": "2018-04-11T18:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2491772165-POCLOUD",
"temporalExtentEnd": "2018-06-11T20:17:26.000Z",
"globalId": "ca6e9b81-316e-5625-b26c-25655e067780",
"abstract": "Saildrone is a wind and solar powered unmanned surface vehicle (USV) capable of long distance deployments lasting up to 12 months and providing high quality, near real-time, multivariate surface ocean and atmospheric observations while transiting at typical speeds of 3-5 knots. The drone is autonomous in that it may be guided remotely from land while being completely wind driven. \rThe saildrone Baja campaign was a 60-day cruise from San Francisco Bay, down along the US/Mexico coast to Guadalupe Island and back again over the period 11 April 2018 to 11 June 2018. Repeat surveys were taken around NDBC moored buoys, and during the final week of the cruise a targeted front was sampled. Scientific objectives included studies of upwelling and frontal region dynamics, air-sea interactions, and diurnal warming effects, while its validation objectives included establishing the utility of data from the saildrone platform for assessment of satellite data accuracy and model assimilation. During the Baja campaign, the single deployed saildrone was equipped with a suite of instruments that included a CTD, IR pyrometer, fluorometer, dissolved oxygen sensor, anemometer, barometer, and Acoustic Doppler Current Profiler (ADCP). Additionally, four temperature data loggers were positioned vertically along hull to provide further information on thermal variability near the ocean surface.\rThis Saildrone Baja dataset is comprised of one data file with the saildrone platform telemetry and near-surface observational data (air temperature, sea surface skin and bulk temperatures, salinity, oxygen and chlorophyll-a concentrations, barometric pressure, wind speed and direction) for the entire cruise at 1 minute temporal resolution. A second file contains the ADCP current vector data that is depth-resolved to 100m at 2m intervals and binned temporally at 5 minute resolution. All data files are in netCDF format and CF/ACDD compliant consistent with the NOAA/NCEI specification.",
"shortName": "SAILDRONE_BAJA_SURFACE",
"longName": "Saildrone Baja field campaign surface and ADCP measurements",
"doi": "10.5067/SDRON-SURF0"
}
|
node
|
10
|
[
"Dataset"
] |
{
"temporalExtentStart": "1991-09-01T00:00:00.000Z",
"daac": "NASA/JPL/PODAAC",
"temporalFrequency": "daily",
"cmrId": "C2499940521-POCLOUD",
"temporalExtentEnd": "2017-03-18T00:00:00.000Z",
"globalId": "102c01e1-bcd7-58b0-837d-102f90effbf0",
"abstract": "A Group for High Resolution Sea Surface Temperature (GHRSST) Level 4 sea surface temperature (SST) analysis produced daily on an operational basis at the Canadian Meteorological Center. This dataset merges infrared satellite SST at varying points in the time series from the (A)TSR series of radiometers from ERS-1, ERS-2 and Envisat, AVHRR from NOAA-16,17,18,19 and METOP-A, and microwave data from TMI, AMSR-E and Windsat in conjunction with in situ observations of SST from drifting buoys and ships from the ICOADS program. It uses the previous days analysis as the background field for the statistical interpolation used to assimilate the satellite and in situ observations. This dataset adheres to the GHRSST Data Processing Specification (GDS) version 2 format specifications.",
"shortName": "CMC0.2deg-CMC-L4-GLOB-v2.0",
"longName": "GHRSST Level 4 CMC0.2deg Global Foundation Sea Surface Temperature Analysis (GDS version 2)",
"doi": "10.5067/GHCMC-4FM02"
}
|
node
|
11
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763289482-LPCLOUD",
"temporalExtentEnd": "2023-02-17T23:59:59.999Z",
"globalId": "e8b0bfee-b836-5367-a068-44f54be9e13f",
"abstract": "The MCD43C4 Version 6 data product was decommissioned on July 31, 2023. Users are encouraged to use the [MCD43C4 Version 6.1](https://doi.org/10.5067/MODIS/MCD43C4.061) data product.The Moderate Resolution Imaging Spectroradiometer (MODIS) MCD43C4 Version 6 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Nadir BRDF-Adjusted Reflectance (NBAR) dataset is produced daily using 16 days of Terra and Aqua MODIS data in a 0.05 degree (5,600 meters at the equator) Climate Modeling Grid (CMG). Data are temporally weighted to the ninth day of the retrieval period which is reflected in the Julian date in the file name. This CMG product covers the entire globe for use in climate simulation models. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the User Guide.MCD43C4 removes view angle effects from directional reflectances to model the values as if they were collected from a nadir view at local solar noon. These NBAR values are calculated from [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.006). The product includes separate NBAR layers for MODIS spectral bands 1 through 7 as well as ancillary layers for quality, local solar noon, percent finer resolution inputs, snow cover, and uncertainty.Known Issues* The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* [Corrections](https://landweb.modaps.eosdis.nasa.gov/data/userguide/LSRHighAerosolFlagFinal.pdf) were implemented in Collection 6.1 reprocessing.* For complete information about the MCD43C4 known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* When there are insufficient high quality reflectances, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid for MCD43C as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43C4",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Nadir BRDF-Adjusted Ref Daily L3 Global 0.05Deg CMG V006",
"doi": "10.5067/MODIS/MCD43C4.006"
}
|
node
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12
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[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2540275683-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "ac139cfa-2b7a-5e1d-a995-1d2beefa5449",
"abstract": "The MCD43D62 Version 6.1 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Nadir BRDF-Adjusted Reflectance (NBAR) dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter (m)) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. MCD43D62 through MCD43D68 are the NBAR products of the MCD43D BRDF/Albedo product suite for MODIS bands 1 through 7. The NBAR algorithm removes view angle effects from directional reflectances to model the values as if they were collected from a nadir view at local solar noon.Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).MCD43D62 is the NBAR for MODIS band 1. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43D62",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Nadir BRDF-Adjusted Ref Band1 Daily L3 Global 30ArcSec CMG V061",
"doi": "10.5067/MODIS/MCD43D62.061"
}
|
node
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13
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[
"Dataset"
] |
{
"temporalExtentStart": "2000-03-03T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C1623882456-LPDAAC_ECS",
"temporalExtentEnd": "2017-12-31T23:59:59.999Z",
"globalId": "750cff52-9834-585b-9773-bf5b680e77d6",
"abstract": "The Daily Moderate Resolution Imaging Spectroradiometer (MODIS) Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) 30 arc second, Global Gap-Filled, Snow-Free, (MCD43GF) Version 6 is derived from the 30 arc second Climate Modeling Grid (CMG) MCD43D Version 6 product suite, with additional processing to provide a gap-filled, snow-free product. The highest quality full inversion values were used for the temporal fitting effort and supplemented with lower quality pixels, spatial fitting, and spatial smoothing as needed. The status of each pixel can be found in the quality layer for each band. To generate a snow-free product, pixels with ephemeral snow were removed using the [MCD43D41](https://doi.org/10.5067/MODIS/MCD43D41.006) snow flags. The underlying MCD43D utilizes a BRDF model derived from all available high quality cloud clear reflectance data over a 16 day moving window centered on and emphasizing the daily day of interest (the ninth day of each retrieval period as reflected in the Julian date in the filename). This 30 arc second BRDF model is then used to produce the Albedo and NBAR products (MCD43D). These BRDF model parameters are computed for MODIS spectral bands 1 through 7 (0.47 um, 0.55 um, 0.67 um, 0.86 um, 1.24 um, 1.64 um, 2.1 um), as well as the shortwave infrared band (0.3-5.0 um), visible band (0.3-0.7 um), and near-infrared (0.7-5.0 um) broad bands. The MCD43GF product includes 67 layers containing black-sky albedo (BSA) at local solar noon, isotropic model parameter (ISO), volumetric model parameter (VOL), geometric model parameter (GEO), quality (QA), Nadir BRDF-Adjusted Reflectance (NBAR) at local solar noon, and white-sky albedo (WSA). Due to the large file size, each data layer is distributed as a separate HDF file. Users are encouraged to download the quality layers for each of the 10 bands to check quality assessment information before using the BRDF/Albedo data.The MCD43 product is not recommended for solar zenith angles beyond 70 degrees.Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the User Guide.Known Issues* There is an error in the DataFieldName value in the metadata. This affects bands 2-7 for the years 2000-2004 and 2013. * The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* For complete information about the MCD43GF known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* In cases where insufficient high-quality reflectances are obtained, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43GF",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Gap-Filled Snow-Free Daily L3 Global 30ArcSec CMG V006",
"doi": "10.5067/MODIS/MCD43GF.006"
}
|
node
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14
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[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-24T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2565807733-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "63ae7d47-5577-5d4f-9a63-9f631d8901d3",
"abstract": "The MCD19A2CMG Version 6.1 data product is a Moderate Resolution Imaging Spectroradiometer (MODIS) Terra and Aqua combined Multi-Angle Implementation of Atmospheric Correction (MAIAC) Land Aerosol Optical Depth (AOD) and Water Vapor Level 3 product produced daily in a 0.05 degree (5,600 meters at the equator) Climate Modeling Grid (CMG). The MCD19A2CMG product provides the atmospheric properties and view geometry used to calculate the MAIAC Surface Reflectance data products ([MCD19A1CMGL](https://doi.org/10.5067/MODIS/MCD19A1CMGL.061) and [MCD19A1CMGO](https://doi.org/10.5067/MODIS/MCD19A1CMGO.061)). The MCD19A2CMG AOD data product contains the following Science Dataset (SDS) layers: blue band AOD at 0.47 µm, green band AOD at 0.55 µm, AOD uncertainty, column water vapor for Terra, column water vapor for Aqua, average cloud fraction, available AOD, satellite overpass times, line and sample number, offset, and number of AOD records. A low-resolution browse image is also included showing AOD of the blue band at 0.47 µm created using a composite of all available orbits. Known Issues* Known issues are described in Section 6 of the User Guide.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).",
"shortName": "MCD19A2CMG",
"longName": "MODIS/Terra+Aqua AOD and Water Vapor from MAIAC, Daily L3 Global 0.05Deg CMG V061",
"doi": "10.5067/MODIS/MCD19A2CMG.061"
}
|
node
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15
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[
"Dataset"
] |
{
"temporalExtentStart": "2018-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2545310883-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "21778272-ec52-54b3-91ff-defa25d9040b",
"abstract": "The NOAA-20 Visible Infrared Imaging Radiometer Suite (VIIRS) Land Surface Temperature and Emissivity (LST&E) Version 2 swath product (VJ121) is produced daily in 6-minute temporal increments of satellite acquisition. The VJ121 product uses a physics-based algorithm to dynamically retrieve both the LST and emissivity simultaneously for VIIRS thermal infrared bands M14 (8.55 µm), M15 (10.76 µm), and M16 (12 µm) at a spatial resolution of 750 meters.The VJ121 product is developed developed synergistically with the Moderate Resolution Imaging Spectroradiometer (MODIS) LST&E Version 6.1 product ([MOD21](https://doi.org/10.5067/MODIS/MOD21.061)) using the same input atmospheric products and algorithmic approach based on the ASTER Temperature Emissivity Separation (TES) technique. The TES algorithm is combined with an improved Water Vapor Scaling (WVS) atmospheric correction scheme to stabilize the retrieval during very warm and humid conditions. The overall objective for NASA VIIRS products is to ensure the algorithms and products are compatible with the MODIS Terra and Aqua algorithms to promote the continuity of the Earth Observation System (EOS) mission. VIIRS LST&E products are available two months after acquisition due to latency of data inputs. Additional details regarding the method used to create this Level 2 (L2) product are available in the Algorithm Theoretical Basis Document (ATBD).Provided in the VJ121 product are layers for LST, quality control, emissivity for bands M14, M15, and M16, LST&E errors, view angle, ASTER Global Emissivity Dataset (GED), Precipitable Water Vapor (PWV), ocean-land mask, latitude, and longitude. A low-resolution browse image for LST is also available for each VJ121 granule.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS) and the User Guide.Improvements/Changes from Previous Version* Improved calibration algorithm and coefficients for entire NOAA-20 mission.* Improved geolocation accuracy and applied updates to fix outliers around maneuver periods.* Corrected the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid- to high-latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 Bidirectional Reflectance Distribution Function (BRDF)/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data. * Replaced the land/water mask input product with the eight-class land/water mask from the VNP03 geolocation product that better aligns with MODIS.* Replaced MERRA2 inputs with GEOS5.* Included inland water body pixels to allow for LST retrieval over these areas.* Introduced daily, 8-day, and monthly LST CMG products.* More details can be found in this [VIIRS Land V2 Changes document](https://landweb.modaps.eosdis.nasa.gov/data/userguide/VIIRS_Land_C2_Changes_09152022.pdf).",
"shortName": "VJ121",
"longName": "VIIRS/JPSS1 Land Surface Temperature and Emissivity 6-Min L2 Swath 750m V002",
"doi": "10.5067/VIIRS/VJ121.002"
}
|
node
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16
|
[
"Dataset"
] |
{
"temporalExtentStart": "1984-03-12T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763261610-LPCLOUD",
"temporalExtentEnd": "2011-12-25T23:59:59.999Z",
"globalId": "bf3e0ad8-3e3d-526e-8480-98e3d92ac4be",
"abstract": "The Land Processes Distributed Active Archive Center (LP DAAC) archives and distributes Global Forest Cover Change (GFCC) data products through the NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Program. The GFCC Surface Reflectance Estimates Multi-Year Global dataset is derived from the enhanced Global Land Survey (GLS) datasets for epochs centered on the years 1990, 2000, 2005, and 2010. The GLS datasets are composed of Landsat 5 Thematic Mapper (TM) and Landsat 7 Enhanced Thematic Mapper Plus (ETM+) images at 30 meter resolution. Data available for this product represent the best available \"leaf-on\" date during the peak growing season. The original GLS datasets were enhanced with supplemental Landsat images when data were incomplete for the epoch or inadequate for analysis due to acquisition during \"leaf-off\" seasons. The enhanced GLS data were acquired June 1984 through August 2011. Atmospheric corrections were applied to seven visible bands to estimate surface reflectance by compensating for the scattering and absorption of radiance by atmospheric conditions. GFCC30SR is a multi-file data product. The surface reflectance data products are used as source data for other datasets in the GFCC collection.For each available date, data files are delivered in a zip folder that consists of six surface reflectance bands, a Top of Atmosphere temperature band, an Atmospheric Opacity layer, and the Landsat Surface Reflectance Quality layer. Data follow the Worldwide Reference System-2 tiling scheme. Additional details regarding the methodology used to create the data are available in the Algorithm Theoretical Basis Document (ATBD). ",
"shortName": "GFCC30SR",
"longName": "Global Forest Cover Change Surface Reflectance Estimates Multi-Year Global 30m V001",
"doi": "10.5067/MEASURES/GFCC/GFCC30SR.001"
}
|
node
|
17
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2540268566-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "ba90c3ad-6ad8-582b-bdde-ee853e3ac6bf",
"abstract": "The MCD43D25 Version 6.1 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Model Parameter dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands included in [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.061) are stored in a separate file as MCD43D01 through MCD43D30. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).MCD43D25 is the BRDF isotropic parameter for the MODIS NIR broadband. The isotropic parameter, in conjunction with the volumetric and geometric parameters, is used to derive the BRDF/Albedo values for the MODIS NIR broadband. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43D25",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Parameter1 NIR Daily L3 Global 30ArcSec CMG V061",
"doi": "10.5067/MODIS/MCD43D25.061"
}
|
node
|
18
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380538-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "311380ae-3001-5be3-9edc-6e096386e625",
"abstract": "The VNP43D65 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D65](https://doi.org/10.5067/VIIRS/VNP43D65.002) and [VJ143D65](https://doi.org/10.5067/VIIRS/VJ143D65.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Black-Sky Albedo for ShortWave (VNP43D65) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D65 is the BSA for the VIIRS shortwave broadband (1.61 μm).Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D65",
"longName": "VIIRS/NPP BRDF/Albedo BSA at Solar Noon ShortWave Daily L3 Global 30ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D65.001"
}
|
node
|
19
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763295129-LPCLOUD",
"temporalExtentEnd": "2023-02-17T23:59:59.999Z",
"globalId": "7b62046e-5942-53b4-9e5e-aa5549539457",
"abstract": "The MCD43D33 Version 6 data product was decommissioned on July 31, 2023. Users are encouraged to use the [MCD43D33 Version 6.1](https://doi.org/10.5067/MODIS/MCD43D33.061) data product.The MCD43D33 Version 6 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) QA ValidObs Band 1 dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter (m)) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. MCD43D33 provides MODIS band 1 valid observation quality information for the MCD43D products. MCD43D33 contains the valid observation quality layer representing each of the 16 days of the retrieval period for MODIS band 1. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).Known Issues* The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* [Corrections](https://landweb.modaps.eosdis.nasa.gov/data/userguide/LSRHighAerosolFlagFinal.pdf) were implemented in Collection 6.1 reprocessing.* For complete information about MCD43D33 known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* When there are insufficient high quality reflectances, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid for MCD43D as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43D33",
"longName": "MODIS/Terra+Aqua BRDF/Albedo QA ValidobsBand1 Daily L3 Global 30ArcSec CMG V006",
"doi": "10.5067/MODIS/MCD43D33.006"
}
|
node
|
20
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2847921472-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "8054251f-8e14-5523-a3e1-bddb73e64069",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 1 Band M3 product (VNP43D07) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D07 is the BRDF isotropic parameter for VIIRS band M3 (0.488 μm). The isotropic parameter, in conjunction with the volumetric and geometric parameters, is used to derive the BRDF/Albedo values for VIIRS band M3.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous Version* Improved calibration algorithm and better coefficients for entire Suomi NPP mission.* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events.* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data.* Replaced the land/water mask input product with MODIS heritage seven class land/water mask.",
"shortName": "VNP43D07",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 1 Band M3 Daily L3 Global 30 ArcSec CMG V002",
"doi": "10.5067/VIIRS/VNP43D07.002"
}
|
node
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21
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[
"Dataset"
] |
{
"temporalExtentStart": "2002-07-04T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2343109950-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "8ef7367e-8223-569b-b9c0-703f0591bd98",
"abstract": "The MYD09GQ Version 6.1 product provides an estimate of the surface spectral reflectance of Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) 250 meter (m) bands 1 and 2, corrected for atmospheric conditions such as gasses, aerosols, and Rayleigh scattering. Along with the 250 m bands are the Quality Assurance (QA) layer and five observation layers. This product is intended to be used in conjunction with the quality and viewing geometry information of the 500 m product (MYD09GA). Known Issues* Prior to the Aqua MODIS launch, Band 6 exhibited several anomalous detectors. Band 6 performance degraded seriously after launch and presently a majority of the Band 6 detectors are non-functional. Science users should read and use the non-functional detector flags and decide for themselves the optimum manner to handle non-functional detector \"gaps\" for their products. For complete information please refer to the [MODIS Characterization Support Team (MCST) website](https://mcst.gsfc.nasa.gov/time-dependent-list-non-functional-or-noisy-detector).* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Aqua&as=61).Improvments/Changes from Previous Version* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MYD09GQ",
"longName": "MODIS/Aqua Surface Reflectance Daily L2G Global 250m SIN Grid V061",
"doi": "10.5067/MODIS/MYD09GQ.061"
}
|
node
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22
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763377746-LPCLOUD",
"temporalExtentEnd": "2024-05-01T23:59:59.999Z",
"globalId": "af5e9dd9-c71d-5ed0-8a47-94d071c5dcb7",
"abstract": "The VNP21A1D VIIRS Version 1 data product was decommissioned on April 8th, 2025. Users are encouraged to use Version 2 data products, which provide [better calibration and consistency](https://landweb.modaps.eosdis.nasa.gov/data/userguide/VIIRS_Land_C2_Changes_09152022.pdf) for the end user. VIIRS Version 2 data products are available from both the SNPP ([VNP21A1D](https://doi.org/10.5067/VIIRS/VNP21A1D.002)) and NOAA-20 ([VJ121A1D]( https://doi.org/10.5067/VIIRS/VJ121A1D.002)) satellites.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Land Surface Temperature and Emissivity (LST&E) Day Version 1 product (VNP21A1D) is compiled daily from daytime Level 2 Gridded (L2G) intermediate products. The L2G process maps the daily [VNP21](https://doi.org/10.5067/VIIRS/VNP21.001) swath granules onto a sinusoidal MODIS grid and stores all observations overlapping a gridded cell for a given day. The VNP21A1 algorithm sorts through all these observations for each cell and estimates the final LST value as an average from all cloud-free observations that have good LST accuracies. The daytime average is weighted by the observation coverage for that cell. Only observations having observation coverage more than a certain threshold (15%) are considered for this averaging. The 1 kilometer dataset is derived through resampling the native 750 meter VIIRS resolution in the input product.The VNP21A1D product is developed synergistically with the Moderate Resolution Imaging Spectroradiometer (MODIS) LST&E Version 6 product (MOD21A1D) using the same input atmospheric products and algorithmic approach. The overall objective for NASA VIIRS products is to ensure the algorithms and products are compatible with the MODIS Terra and Aqua algorithms to promote the continuity of the Earth Observation System (EOS) mission. Additional details regarding the method used to create this Level 3 (L3) product are available in the Algorithm Theoretical Basis Document (ATBD). VIIRS LST&E products are available 2 months after acquisition due to latency of data inputs.The VNP21A1D product contains seven Science Datasets (SDS): LST, quality control, emissivity for bands M14, M15, and M16, view zenith angle, and time of observation. A low-resolution browse image for LST is also available for each VNP21A1D granule.Known Issues* Users of VIIRS and MODIS LST products may notice an increase in occurrences of [extreme high temperature outliers](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=707) in the unfiltered VNP21 and MxD21 products compared to the heritage MxD11 LST products. This can occur especially over desert regions like the Sahara where undetected cloud and dust can negatively impact MxD11, MxD21, and VNP21 retrieval algorithms. * In the MxD11 LST products, these contaminated pixels are flagged in the algorithm and set to fill values in the output products based on differences in the band 32 and band 31 radiances used in the generalized split window algorithm. In the VNP21 and MxD21 LST products, values for the contaminated pixels are retained in the output products (and may result in overestimated temperatures), and users need to apply Quality Control (QC) filtering and other error analyses for filtering out bad values. High temperature outlier thresholds are not employed in VNP21 and MxD21 since it would potentially remove naturally occurring hot surface targets such as fires and lava flows.* High atmospheric aerosol optical depth (AOD) caused by vast dust outbreaks in the Sahara and other deserts highlighted in the example documentation are the primary reason for high outlier surface temperature values (and corresponding low emissivity values) in the VNP21 and MxD21 LST products. Future versions of the VNP21 and MxD21 products will include a dust flag from the MODIS aerosol product and/or brightness temperature look up tables to filter out contaminated dust pixels. It should be noted that in the MxD11B day/night algorithm products, more advanced cloud filtering is employed in the multi-day products based on a temporal analysis of historical LST over cloudy areas. This may result in more stringent filtering of dust contaminated pixels in these products. * To mitigate the impact of dust in the VNP21 and MxD21 products, the science team recommends using a combination of the existing QC bits, emissivity values, and estimated product errors, to confidently remove bad pixels from analysis. For more details, refer to this dust and cloud contamination [example documentation](https://landweb.modaps.eosdis.nasa.gov/QA_WWW/forPage/MOD21_dust_QC_examples.pdf).* VNP21 v001 products utilize the Modern-Era Retrospective analysis for Research and Applications, Version 2 (MERRA-2) as an input. This may result in product latency of a month or more. * For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP21A1D",
"longName": "VIIRS/NPP Land Surface Temperature/Emissivity Daily L3 Global 1km SIN Grid Day V001",
"doi": "10.5067/VIIRS/VNP21A1D.001"
}
|
node
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23
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763379968-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "1e0a193d-c5b0-5307-ad50-59476aab41f7",
"abstract": "The VNP43D22 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D22](https://doi.org/10.5067/VIIRS/VNP43D22.002) and [VJ143D22](https://doi.org/10.5067/VIIRS/VJ143D22.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 1 Band M10 product (VNP43D22) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D22 is the BRDF isotropic parameter for VIIRS band M10 (1.61 μm). The isotropic parameter, in conjunction with the volumetric and geometric parameters, is used to derive the BRDF/Albedo values for VIIRS band M10.Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D22",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 1 Band M10 Daily L3 Global 30 ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D22.001"
}
|
node
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24
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2849397809-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "3c224c9b-3e6a-57fe-891f-d9360083916d",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Black-Sky Albedo for Band M8 (VNP43D60) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.002) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.002) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D60 is the BSA for VIIRS band M8 (1.240 μm).Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous Version* Improved calibration algorithm and better coefficients for entire Suomi NPP mission.* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events.* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data.* Replaced the land/water mask input product with MODIS heritage seven class land/water mask.",
"shortName": "VNP43D60",
"longName": "VIIRS/NPP BRDF/Albedo BSA at Solar Noon Band M8 Daily L3 Global 30ArcSec CMG V002",
"doi": "10.5067/VIIRS/VNP43D60.002"
}
|
node
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25
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2540268595-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "5274396c-c028-581a-a873-dabb6808074a",
"abstract": "The MCD43D30 Version 6.1 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Model Parameter dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Sprectroradiometer (MODIS) data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands included in [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.061) are stored in a separate file as MCD43D01 through MCD43D30. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).MCD43D30 is the BRDF geometric parameter for the MODIS shortwave broadband. The geometric parameter, in conjunction with the isotropic and volumetric parameters, is used to derive the BRDF/Albedo values for the MODIS shortwave broadband.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43D30",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Parameter3 Shortwave Daily L3 Global 30ArcSec CMG V061",
"doi": "10.5067/MODIS/MCD43D30.061"
}
|
node
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26
|
[
"Dataset"
] |
{
"temporalExtentStart": "2013-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763261708-LPCLOUD",
"temporalExtentEnd": "2016-12-31T23:59:59.999Z",
"globalId": "0b07a9ca-a72d-5199-b0b7-321bb5fff297",
"abstract": "The NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Global Food Security-support Analysis Data (GFSAD) data product provides cropland extent data over South America for nominal year 2015 at 30 meter resolution (GFSAD30SACE). The monitoring of global cropland extent is critical for policymaking and provides important baseline data that are used in many agricultural cropland studies pertaining to water sustainability and food security. The GFSAD30SACE data product uses the pixel-based supervised classifier, Random Forest (RF), to retrieve cropland extent from a combination of Landsat 5 Thematic Mapper (TM), Landsat 7 Enhanced Thematic Mapper Plus (ETM+), Landsat 8 Operational Land Imager (OLI) data, and elevation derived from the Shuttle Radar Topography Mission (SRTM) Version 3 data products. Each GFSAD30SACE GeoTIFF file contains a cropland extent layer that defines areas of cropland, non-cropland, and water bodies over a 10° by 10° area.Known Issues* Known issues, including constraints and limitations, are provided on page 18 of the ATBD.",
"shortName": "GFSAD30SACE",
"longName": "Global Food Security-support Analysis Data (GFSAD) Cropland Extent 2015 South America product 30 m V001",
"doi": "10.5067/MEaSUREs/GFSAD/GFSAD30SACE.001"
}
|
node
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27
|
[
"Dataset"
] |
{
"temporalExtentStart": "2002-07-04T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2565794850-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "9a63b101-635c-5f3d-b011-e4f2c5c368f1",
"abstract": "The MYD17A3HGF Version 6.1 product provides information about annual Gross and Net Primary Production (GPP and NPP) at 500 meter (m) pixel resolution. Annual Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) GPP and NPP is derived from the sum of all 8-day GPP and Net Photosynthesis (PSN) products ([MYD17A2H](https://doi.org/10.5067/MODIS/MYD17A2H.061)) from the given year. The PSN value is the difference of the GPP and the Maintenance Respiration (MR).The MYD17A3HGF will be generated at the end of each year when the entire yearly 8-day [MYD15A2H](https://doi.org/10.5067/modis/myd15a2h.061) is available. Hence, the gap-filled MYD17A3HGF is the improved MYD17, which has cleaned the poor-quality inputs from 8-day Leaf Area Index and Fraction of Photosynthetically Active Radiation (FPAR/LAI) based on the Quality Control (QC) label for every pixel. If any LAI/FPAR pixel did not meet the quality screening criteria, its value is determined through linear interpolation. However, users cannot get MYD17A3HGF in near-real time because it will be generated only at the end of a given year.Known Issues* Operational and uncertainty issues are provided under Section 2 in the User Guide.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Aqua&as=61).Improvments/Changes from Previous Version* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).* The product uses Climatology LAI/FPAR as back up to the operational LAI/FPAR.",
"shortName": "MYD17A3HGF",
"longName": "MODIS/Aqua Net Primary Production Gap-Filled Yearly L4 Global 500m SIN Grid V061",
"doi": "10.5067/MODIS/MYD17A3HGF.061"
}
|
node
|
28
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2218719731-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "21b38d33-e1f1-5520-8f88-beca75d6b8df",
"abstract": "The Moderate Resolution Imaging Spectroradiometer (MODIS) MCD43A4 Version 6.1 Nadir Bidirectional Reflectance Distribution Function (BRDF)-Adjusted Reflectance (NBAR) dataset is produced daily using 16 days of Terra and Aqua MODIS data at 500 meter (m) resolution. The view angle effects are removed from the directional reflectances, resulting in a stable and consistent NBAR product. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name.Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43a4-nbar-product/).The MCD43A4 provides NBAR and simplified mandatory quality layers for MODIS bands 1 through 7. Essential quality information provided in the corresponding [MCD43A2](https://doi.org/10.5067/MODIS/MCD43A2.061) data file should be consulted when using this product.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43A4",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Nadir BRDF-Adjusted Ref Daily L3 Global - 500m V061",
"doi": "10.5067/MODIS/MCD43A4.061"
}
|
node
|
29
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2847920280-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "f2804f4b-5b5d-52e7-a9c1-8e28311cf795",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 1 Band M2 product (VNP43D04) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product page and in the Algorithm Theoretical Basis Document (ATBD). VNP43D04 is the BRDF isotropic parameter for VIIRS band M2 (0.445 μm). The isotropic parameter, in conjunction with the volumetric and geometric parameters, is used to derive the BRDF/Albedo values for VIIRS band M2.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous Version* Improved calibration algorithm and better coefficients for entire Suomi NPP mission.* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events.* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data.* Replaced the land/water mask input product with MODIS heritage seven class land/water mask.",
"shortName": "VNP43D04",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 1 Band M2 Daily L3 Global 30 ArcSec CMG V002",
"doi": "10.5067/VIIRS/VNP43D04.002"
}
|
node
|
30
|
[
"Dataset"
] |
{
"temporalExtentStart": "2018-01-05T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2841241866-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "9f1c350d-abdd-57a5-847a-cf8c57aebfd7",
"abstract": "The NOAA-20 Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 2 Band M11 product (VJ143D26) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VJ143D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VJ143D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VJ143MA1](https://doi.org/10.5067/VIIRS/VJ143MA1.002) product is stored in a separate file as VJ143D01 through VJ143D36. In addition to the bands included in VJ143MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VJ143D37 through VJ143D39. Details regarding methodology are available on the VJ143MA1 product page and in the Algorithm Theoretical Basis Document [ATBD).VJ143D26 is the BRDF volumetric parameter for VIIRS band M11 (2.25 μm). The volumetric parameter, in conjunction with the isotropic and geometric parameters, is used to derive the BRDF/Albedo values for VIIRS band M11.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website]( https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous VersionsThe NOAA-20 VIIRS algorithms include the same improvements as the S-NPP VIIRS V002* Improved calibration algorithm and better coefficients for entire NOAA-20 mission* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VJ113 Vegetation Indices and VJ143 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data* Replaced the land/water mask input product with MODIS heritage seven class land/water mask",
"shortName": "VJ143D26",
"longName": "VIIRS/JPSS1 BRDF/Albedo Parameter 2 Band M11 Daily L3 Global 30 ArcSec CMG V002",
"doi": "10.5067/VIIRS/VJ143D26.002"
}
|
node
|
31
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-24T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2343115666-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "b328d420-0866-547a-a3e4-05a110c434fc",
"abstract": "The MOD09GQ Version 6.1 product provides an estimate of the surface spectral reflectance of Terra Moderate Resolution Imaging Spectroradiometer (MODIS) 250 meter (m) bands 1 and 2, corrected for atmospheric conditions such as gasses, aerosols, and Rayleigh scattering. Along with the 250 m surface reflectance bands are the Quality Assurance (QA) layer and five observation layers. This product is intended to be used in conjunction with the quality and viewing geometry information of the 500 m product (MOD09GA). Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Terra&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MOD09GQ",
"longName": "MODIS/Terra Surface Reflectance Daily L2G Global 250m SIN Grid V061",
"doi": "10.5067/MODIS/MOD09GQ.061"
}
|
node
|
32
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380535-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "18a93a6f-482d-56cd-a054-1bded4bd0a34",
"abstract": "The VNP43D64 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D64](https://doi.org/10.5067/VIIRS/VNP43D64.002) and [VJ143D64](https://doi.org/10.5067/VIIRS/VJ143D64.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Black-Sky Albedo for NIR (VNP43D64) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D64 is the BSA for the VIIRS NIR broadband (0.865 μm).Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D64",
"longName": "VIIRS/NPP BRDF/Albedo BSA at Solar Noon NIR Daily L3 Global 30ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D64.001"
}
|
node
|
33
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763295217-LPCLOUD",
"temporalExtentEnd": "2023-02-17T23:59:59.999Z",
"globalId": "979c1a13-2742-55e1-b0a2-9aa191d82354",
"abstract": "The MCD43D45 Version 6 data product was decommissioned on July 31, 2023. Users are encouraged to use the [MCD43D45 Version 6.1](https://doi.org/10.5067/MODIS/MCD43D45.061) data product.The MCD43D45 Version 6 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Black-Sky Albedo dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter (m)) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. MCD43D42 through MCD43D61 are the albedo products of the MCD43D BRDF/Albedo product suite. There are 10 black-sky albedo and 10 white-sky albedo layers representing MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands. The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. MCD43D45 is the black-sky albedo for MODIS band 4. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).Known Issues* The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* [Corrections](https://landweb.modaps.eosdis.nasa.gov/data/userguide/LSRHighAerosolFlagFinal.pdf) were implemented in Collection 6.1 reprocessing.* For complete information about MCD43D45 known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* When there are insufficient high quality reflectances, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid for MCD43D as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43D45",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Black Sky Albedo Band4 Daily L3 Global 30ArcSec CMG V006",
"doi": "10.5067/MODIS/MCD43D45.006"
}
|
node
|
34
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2532007810-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "39a7b3a8-3250-55a5-bd07-2d3d055dbd57",
"abstract": "The MCD43D06 Version 6.1 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Model Parameter dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands included in [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.061) are stored in a separate file as MCD43D01 through MCD43D30. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).MCD43D06 is the BRDF geometric parameter for MODIS band 2. The geometric parameter, in conjunction with the isotropic and volumetric parameters, is used to derive the BRDF/Albedo values for MODIS band 2. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43D06",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Parameter 3 Band 2 Daily L3 Global 30 ArcSec CMG V061",
"doi": "10.5067/MODIS/MCD43D06.061"
}
|
node
|
35
|
[
"Dataset"
] |
{
"temporalExtentStart": "2022-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2517904291-LPCLOUD",
"temporalExtentEnd": "2024-02-26T23:59:59.999Z",
"globalId": "2dad0227-f474-55ad-9d7d-e54cfccbb2ea",
"abstract": "The OPERA_L3_DIST-ALERT-HLS Version 0 data product was decommissioned on April 25, 2025. Users are encouraged to use the [OPERA_L3_DIST-ALERT-HLS V1](https://doi.org/10.5067/SNWG/OPERA_L3_DIST-ALERT-HLS_V1.001) data product which was released on March 14, 2024, and has achieved stage 1 validation.The Observational Products for End-Users from Remote Sensing Analysis (OPERA) Land Surface Disturbance Alert from Harmonized Landsat Sentinel-2 (HLS) provisional data product Version 0 maps vegetation disturbance alerts from data collected by Landsat 8 and Landsat 9 Operational Land Imager (OLI) and Sentinel-2A, Sentinel-2B, and Sentinel-2C Multi-Spectral Instrument (MSI). Vegetation disturbance alert is detected at 30 meter (m) spatial resolution when there is an indicated decrease in vegetation cover within an HLS pixel. The product also provides auxiliary generic disturbance information as determined from the variations of the reflectance through the HLS scenes to provide information about more general disturbance trends. HLS data represent the highest temporal frequency data available at medium spatial resolution. The combined observations will provide greater sensitivity to land changes, whether of large magnitude/short duration, or small magnitude/long duration. The OPERA_L3_DIST-ALERT-HLS (or DIST-ALERT) data product is provided in Cloud Optimized GeoTIFF (COG) format, and each layer is distributed as a separate file. There are 19 layers contained within in the DIST-ALERT product: vegetation disturbance status, current vegetation cover indicator, current vegetation anomaly value, historical vegetation cover indicator, max vegetation anomaly value, vegetation disturbance confidence layer, date of initial vegetation disturbance, number of detected vegetation loss anomalies, and vegetation disturbance duration. See the Product Specification for a more detailed description of the individual layers provided in the DIST-ALERT product. Known Issues* Additional usage constraints are provided under Section 5 of the Algorithm Theoretical Basis Document (ATBD).",
"shortName": "OPERA_L3_DIST-ALERT-HLS_PROVISIONAL_V0",
"longName": "OPERA Land Surface Disturbance Alert from Harmonized Landsat Sentinel-2 provisional product (Version 0)",
"doi": "10.5067/SNWG/OPERA_L3_DIST-ALERT-HLS_PROVISIONAL_V0.000"
}
|
node
|
36
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-03-06T00:30:05.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C3306877498-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "42b92e53-0278-5484-9e14-8df03de48ad8",
"abstract": "The Terra Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) Surface Reflectance VNIR and SWIR (AST_07) data product contains measures of the fraction of incoming solar radiation reflected from the Earth’s surface to the ASTER instrument corrected for atmospheric effects and viewing geometry for both the Visible and Near Infrared (VNIR) and Shortwave Infrared (SWIR) sensors. The AST_07 product has a spatial resolution of 15 meters (m) for the VNIR bands and 30 m for the SWIR bands.Known Issues* Level 2 products that are on the international date line/anti-meridian have incorrect bounding coordinates for the Universal Transverse Mercator (UTM) zone defined in the file metadata.* SWIR data acquired after April 2008 may exhibit anomalous saturation and striping. Users should consult the ASTER SWIR User Advisory for additional details.Improvements/Changes from Previous Versions* Enhanced Atmospheric Correction: Version 4 uses Modern-Era Retrospective analysis for Research and Applications Version 2 (MERRA-2) data as the primary source for atmospheric parameters (ozone, water vapor, pressure, and temperature), improving the precision of emissivity calculations. Fallback Mechanisms: When MERRA-2 data are unavailable, the product employs Global Data Assimilation System (GDAS) data as a backup, with climatology data serving as a final fallback to ensure continuous processing. Radiometric Calibration Update: Version 4 applies Radiometric Calibration Coefficient Version 5 (RCC V5) to improve the radiometric accuracy of the raw DNs, based on research by [Tsuchida and others (2020)](https://doi.org/10.3390/rs12030427), published in Remote Sensing.",
"shortName": "AST_07",
"longName": "ASTER L2 Surface Reflectance VNIR and SWIR V004",
"doi": "10.5067/ASTER/AST_07.004"
}
|
node
|
37
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763293490-LPCLOUD",
"temporalExtentEnd": "2023-02-17T23:59:59.999Z",
"globalId": "4cc53cdb-eeac-5a8d-9ae6-4d49d5052079",
"abstract": "The MCD43D29 Version 6 data product was decommissioned on July 31, 2023. Users are encouraged to use the [MCD43D29 Version 6.1](https://doi.org/10.5067/MODIS/MCD43D29.061) data product.The MCD43D29 Version 6 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Model Parameter dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands included in [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.006) are stored in a separate file as MCD43D01 through MCD43D30. MCD43D29 is the BRDF volumetric parameter for the MODIS shortwave broadband. The volumetric parameter, in conjunction with the isotropic and geometric parameters, is used to derive the BRDF/Albedo values for the MODIS shortwave broadband. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).Known Issues* The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* [Corrections](https://landweb.modaps.eosdis.nasa.gov/data/userguide/LSRHighAerosolFlagFinal.pdf) were implemented in Collection 6.1 reprocessing.* For complete information about MCD43D29 known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* When there are insufficient high quality reflectances, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid for MCD43D as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43D29",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Parameter2 Shortwave Daily L3 Global 30ArcSec CMG V006",
"doi": "10.5067/MODIS/MCD43D29.006"
}
|
node
|
38
|
[
"Dataset"
] |
{
"temporalExtentStart": "2018-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2545310918-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "a530e2cb-b0d5-52e9-82e3-8aa685b9363d",
"abstract": "The NOAA-20 Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Quality (VJ143IA2) Version 2 product provides BRDF and Albedo quality at 500 meter (m) resolution. The VJ143IA2 product is produced daily using 16 days of VIIRS data and is weighted temporally to the ninth day, which is reflected in the file name. The VJ143IA2 product provides information regarding band quality and days of valid observation within a 16-day period for the VIIRS imagery bands. The VJ143 data products are designed to promote the continuity of NASA’s Moderate Resolution Imaging Spectroradiometer (MODIS) BRDF/Albedo data product suite. The VJ143 algorithm uses the RossThick/Li-Sparse-Reciprocal (RTLSR) semi-empirical kernel-driven BRDF model, with the three kernel weights from [VJ143IA1](https://doi.org/10.5067/VIIRS/VJ143IA1.002) to reconstruct surface anisotropic effects, correcting the directional reflectance to a common view geometry ([VJ143IA4](https://doi.org/10.5067/VIIRS/VJ143IA4.002)), while also computing integrated black-sky albedo (BSA) at local solar noon and white-sky albedo (WSA) ([VJ143IA3](https://doi.org/10.5067/VIIRS/VJ143IA3.002)). Researchers can use the BRDF model parameters with a simple polynomial, to obtain black-sky albedo at any solar illumination angle. Likewise, both the BSA and WSA Science Dataset (SDS) layers can be used with a simple polynomial, to manually estimate instantaneous actual albedo (blue-sky albedo). Additional details regarding the methodology are available in the Algorithm Theoretical Basis Document (ATBD). The VJ143IA2 data product provides a total of 11 SDS layers including: BRDF/Albedo band quality (inversion information) and days of valid observation within a 16-day period for VIIRS imagery bands I1, I2, and I3, as well as land water type class flag, snow BRDF albedo class flag, local solar noon, albedo uncertainty and the platform name.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).Improvements/Changes from Previous Version* Improved calibration algorithm and coefficients for entire NOAA-20 mission.* Improved geolocation accuracy and applied updates to fix outliers around maneuver periods.* Corrected the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid- to high-latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 Bidirectional Reflectance Distribution Function (BRDF)/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data. * Replaced the land/water mask input product with the eight-class land/water mask from the VNP03 geolocation product that better aligns with MODIS.* More details can be found in this [VIIRS Land V2 Changes document](https://landweb.modaps.eosdis.nasa.gov/data/userguide/VIIRS_Land_C2_Changes_09152022.pdf).",
"shortName": "VJ143IA2",
"longName": "VIIRS/JPSS1 BRDF/Albedo Quality Daily L3 Global 500m SIN Grid V002",
"doi": "10.5067/VIIRS/VJ143IA2.002"
}
|
node
|
39
|
[
"Dataset"
] |
{
"temporalExtentStart": "2002-07-04T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2565805789-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "a00df9d0-fe40-5391-84f9-89f0332db352",
"abstract": "A suite of Moderate Resolution Imaging Spectroradiometer (MODIS) Land Surface Temperature and Emissivity (LST&E) products are available in Collection 6.1. The MYD21 Land Surface Temperature (LST) algorithm differs from the algorithm of the [MYD11](https://doi.org/10.5067/modis/myd11_l2.061) LST products, in that the MYD21 algorithm is based on the ASTER Temperature/Emissivity Separation (TES) technique, whereas the MYD11 uses the split-window technique. The MYD21 TES algorithm uses a physics-based algorithm to dynamically retrieve both the LST and spectral emissivity simultaneously from the MODIS thermal infrared bands 29, 31, and 32. The TES algorithm is combined with an improved Water Vapor Scaling (WVS) atmospheric correction scheme to stabilize the retrieval during very warm and humid conditions. The MYD21A1N dataset is produced daily from nighttime Level 2 Gridded (L2G) intermediate LST products. The L2G process maps the daily [MYD21](http://doi.org/10.5067/MODIS/MYD21.061) swath granules onto a sinusoidal MODIS grid and stores all observations falling over a gridded cell for a given day. The MOD21A1 algorithm sorts through all these observations for each cell and estimates the final LST value as an average from all observations that are cloud free and have good LST&E accuracies. The nighttime average is weighted by the observation coverage for that cell. Only observations having an observation coverage greater than a 15% threshold are considered. The MYD21A1N product contains seven Science Datasets (SDS), which include the calculated LST as well as quality control, the three emissivity bands, view zenith angle, and time of observation. Additional details regarding the methodology used to create this Level 3 (L3) product are available in the Algorithm Theoretical Basis Document (ATBD).Known Issues* Users of MODIS LST products may notice an increase in occurrences of [extreme high temperature outliers](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=117) in the unfiltered MxD21 Version 6 and 6.1 products compared to the heritage MxD11 LST products. This can occur especially over desert regions like the Sahara where undetected cloud and dust can negatively impact both the MxD21 and MxD11 retrieval algorithms. * In the MxD11 LST products, these contaminated pixels are flagged in the algorithm and set to fill values in the output products based on differences in the band 32 and band 31 radiances used in the generalized split window algorithm. In the MxD21 LST products, values for the contaminated pixels are retained in the output products (and may result in overestimated temperatures), and users need to apply Quality Control (QC) filtering and other error analyses for filtering out bad values. High temperature outlier thresholds are not employed in MxD21 since it would potentially remove naturally occurring hot surface targets such as fires and lava flows.* High atmospheric aerosol optical depth (AOD) caused by vast dust outbreaks in the Sahara and other deserts highlighted in the example documentation are the primary reason for high outlier surface temperature values (and corresponding low emissivity values) in the MxD21 LST products. Future versions of the MxD21 product will include a dust flag from the MODIS aerosol product and/or brightness temperature look up tables to filter out contaminated dust pixels. It should be noted that in the MxD11B day/night algorithm products, more advanced cloud filtering is employed in the multi-day products based on a temporal analysis of historical LST over cloudy areas. This may result in more stringent filtering of dust contaminated pixels in these products. * In order to mitigate the impact of dust in the MxD21 V6 and 6.1 products, the science team recommends using a combination of the existing QC bits, emissivity values, and estimated product errors, to confidently remove bad pixels from analysis. For more details, refer to this dust and cloud contamination [example documentation](https://landweb.modaps.eosdis.nasa.gov/data/userguide/MOD21_dust_QC_examples.pdf).* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Aqua&as=61).Improvments/Changes from Previous Version* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).* The product utilizes GEOS data replacing MERRA2.* Three new CMG products are available in the MxD21 suite (MxD21C1/C2/C3).",
"shortName": "MYD21A1N",
"longName": "MODIS/Aqua Land Surface Temperature/3-Band Emissivity Daily L3 Global 1km SIN Grid Night V061",
"doi": "10.5067/MODIS/MYD21A1N.061"
}
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40
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2847921079-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "3aed5697-3ba1-5835-ab26-03ff1d5b91c6",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 3 Band M2 product (VNP43D06) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.002) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D06 is the BRDF geometric parameter for VIIRS band M2 (0.445 μm). The geometric parameter, in conjunction with the isotropic and volumetric parameters, is used to derive the BRDF/Albedo values for VIIRS band M2.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous Version* Improved calibration algorithm and better coefficients for entire Suomi NPP mission.* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events.* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data.* Replaced the land/water mask input product with MODIS heritage seven class land/water mask.",
"shortName": "VNP43D06",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 3 Band M2 Daily L3 Global 30 ArcSec CMG V002",
"doi": "10.5067/VIIRS/VNP43D06.002"
}
|
node
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41
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[
"Dataset"
] |
{
"temporalExtentStart": "2016-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763264758-LPCLOUD",
"temporalExtentEnd": "2018-12-31T23:59:59.000Z",
"globalId": "7cb1b6c2-45cd-590d-a6e1-5116f46cbda6",
"abstract": "MSLSP V1 data was decommissioned on December 14, 2021. Users are encouraged to use the improved [MSLSP V1.1](https://doi.org/10.5067/Community/MuSLI/MSLSP30NA.011) data product.NASA’s Multi-Source Land Imaging (MuSLI) Land Surface Phenology (LSP) Yearly North America 30 meter (m) Version 1 product (MSLSP) provides a Land Surface Phenology product for North America derived from Harmonized Landsat Sentinel-2 (HLS) data. Data from the combined Landsat 8 Operational Land Imager (OLI) and Sentinel 2A and 2B Multispectral Instrument (MSI) provide the user community with dates of phenophase transitions, including the timing of greenup, maturity, senescence, and dormancy. MSLSP30NA is aligned with the Military Grid Reference System ([MGRS](https://hls.gsfc.nasa.gov/products-description/tiling-system)) at 30 m spatial resolution. These datasets are useful for a wide range of applications, including ecosystem and agro-ecosystem modeling, monitoring the response of terrestrial ecosystems to climate variability and extreme events, crop-type discrimination, land cover, land use, and land cover change mapping.Provided in the MSLSP product are variables for percent greenness, onset greenness dates, Enhanced Vegetative Index (EVI2) amplitude, maximum EVI2, and data quality information for up to two phenological cycles per year. For areas where the data values are missing due to cloud cover or other reasons, the data gaps are filled with good quality values from the year directly preceding or following the product year. A low-resolution browse image representing maximum EVI is also available for each MSLSP30NA granule.Known Issues* Data are sparse in 2016 and early 2017, as Sentinel-2B was not yet launched, and Sentinel-2A was not fully operational, leading to poorer quality retrievals of phenology in 2016 and 2017. However, poor quality pixels can be masked with Quality Assurance (QA) flags.* Disturbance has not been explicitly accounted for or mapped, which can lead to premature detections of senescence and dormancy when sharp spectral changes occur.* Pixels with more than two growth cycles per year (e.g., alfalfa fields) may not be accurately characterized, especially if they occur in rapid succession.",
"shortName": "MSLSP30NA",
"longName": "MuSLI Multi-Source Land Surface Phenology Yearly North America 30 m V001",
"doi": "10.5067/Community/MuSLI/MSLSP30NA.001"
}
|
node
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42
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[
"Dataset"
] |
{
"temporalExtentStart": "1999-06-29T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763261619-LPCLOUD",
"temporalExtentEnd": "2003-01-14T23:59:59.999Z",
"globalId": "beb83473-9a5c-5810-bcd5-1bf2ca7ee3ad",
"abstract": "The Land Processes Distributed Active Archive Center (LP DAAC) archives and distributes Global Forest Cover Change (GFCC) data products through the NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Program. The GFCC Water Cover 2000 Global dataset provides surface-water information at 30 meter spatial resolution. This dataset was derived from waterbodies in the GFCC Tree Cover ([GFCC30TC](https://doi.org/10.5067/MEaSUREs/GFCC/GFCC30TC.003)) and Forest Cover Change ([GFCC30FCC](https://doi.org/10.5067/MEaSUREs/GFCC/GFCC30FCC.001)) products based on a classification-tree model. Data are available for selected dates between June 1999 and January 2003. GFCC30WC follows the Worldwide Reference System-2 tiling scheme. Additional details regarding the methodology used to create the data are available in the Algorithm Theoretical Basis Document (ATBD). ",
"shortName": "GFCC30WC",
"longName": "Global Forest Cover Change Water Cover 2000 Global 30m V001",
"doi": "10.5067/MEASURES/GFCC/GFCC30WC.001"
}
|
node
|
43
|
[
"Dataset"
] |
{
"temporalExtentStart": "2018-01-05T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2842065088-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "ef52fd0f-f0f5-5db0-bb3f-b8f768026180",
"abstract": "The NOAA-20 Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Nadir BRDF-Adjusted Reflectance (NBAR) for Band M5 (VJ143D84) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VJ143D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VJ143D product contains just one data layer. VJ143D80 through VJ143D89 are the NBAR products of the VJ143D BRDF/Albedo product suite. NBAR values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) included in the [VJ143MA4](https://doi.org/10.5067/VIIRS/VJ143MA4.002) product. In addition to the bands included in VNP43MA4, this product suite includes NBAR values for the VIIRS Day/Night Band (DNB). The NBAR algorithm removes view angle effects from directional reflectances to model the values as if they were collected from a nadir view at local solar noon. Details regarding methodology are available on the VJ143MA4 product page and in the Algorithm Theoretical Basis Document (ATBD).VJ143D84 is the NBAR for VIIRS band M5 (0.672 μm). Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website]( https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous VersionsThe NOAA-20 VIIRS algorithms include the same improvements as the S-NPP VIIRS V002* Improved calibration algorithm and better coefficients for entire NOAA-20 mission* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VJ113 Vegetation Indices and VJ143 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data* Replaced the land/water mask input product with MODIS heritage seven class land/water mask",
"shortName": "VJ143D84",
"longName": "VIIRS/JPSS1 BRDF/Albedo NBAR at Solar Noon Band M5 Daily L3 Global 30ArcSec CMG V002",
"doi": "10.5067/VIIRS/VJ143D84.002"
}
|
node
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44
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[
"Dataset"
] |
{
"temporalExtentStart": "2018-07-15T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2076105456-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "cbc9c93f-d916-53e9-bf52-3a70a23a057f",
"abstract": "The ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) mission measures the temperature of plants to better understand how much water plants need and how they respond to stress. ECOSTRESS is attached to the International Space Station (ISS) and collects data globally between 52° N and 52° S latitudes.The ECOSTRESS Tiled Evapotranspiration disALEXI 24-hour L3 CONUS 70 m Version 2 data product provides estimates of daily evapotranspiration (ET). It utilizes the ECOSTRESS Level 2 (L2) land surface temperature and emissivity (LST&E) product ([ECO_L2T_LSTE.002](https://doi.org/10.5067/ECOSTRESS/ECO_L2T_LSTE.002)), regional-scale fluxes from the Atmospheric Land Exchange Interface (ALEXI) model, and Normalized Difference Vegetation Index (NDVI) and albedo from the Spatial Timeseries for Automated high-Resolution multi-Sensor (STARS) data-fusion product ([ECO_L2T_STARS.002](https://doi.org/10.5067/ECOSTRESS/ECO_L2T_STARS.002)), with meteorology sourced from the Climate Forecast System Reanalysis (CFSR).The ECO_L3T_ET_ALEXI data product is derived using a physics-based Two-Source Energy Balance (TSEB) model, implemented in the Atmosphere Land Exchange Inverse (ALEXI) disaggregation algorithm (DisALEXI). Described in the Algorithm Theoretical Basis Document (ATBD), DisALEXI spatially disaggregates the regional ET produced by the ALEXI TSEB model. While there are many approaches for spatially mapping ET, models based on the surface energy balance are favored for remote sensing retrievals based on land-surface temperature. Applications include estimating crop water use, phenology monitoring, and drought early warning or detecting vegetation water stress.The ECO_L3T_ET_ALEXI Version 2 data product is available in Cloud Optimized GeoTIFF (COG) format for Conterminous United States (CONUS) using a modified version of the Military Grid Reference System (MGRS), which divides Universal Transverse Mercator (UTM) zones into square tiles that are 109.8 km by 109.8 km with a 70 m spatial resolution. Each granule contains a separate COG file for each variable: Evapotranspiration Daily and Evapotranspiration Daily Uncertainty. A low-resolution browse is also available showing daily ET as a stretched image with a color ramp in JPEG format.Known Issues* Data acquisition gap: ECOSTRESS was launched on June 29, 2018, and moved to autonomous science operations on August 20, 2018, following a successful in-orbit checkout period. On September 29, 2018, ECOSTRESS experienced an anomaly with its primary mass storage unit (MSU). ECOSTRESS has a primary and secondary MSU (A and B). On December 5, 2018, the instrument was switched to the secondary MSU and science operations resumed. On March 14, 2019, the secondary MSU experienced a similar anomaly, temporarily halting science acquisitions. On May 15, 2019, a new data acquisition approach was implemented, and science acquisitions resumed. To optimize the new acquisition approach TIR bands 2, 4, and 5 are being downloaded. The data products are as previously, except the bands not downloaded contain fill values (L1 radiance and L2 emissivity). This approach was implemented from May 15, 2019, through April 28, 2023.* Data acquisition gap: From February 8 to February 16, 2020, an ECOSTRESS instrument issue resulted in a data anomaly that created striping in band 4 (10.5 micron). These data products have been reprocessed and are available for download. No ECOSTRESS data were acquired on February 17, 2020, due to the instrument being in SAFEHOLD. Data acquired following the anomaly have not been affected.* Solar Array Obstruction: Some ECOSTRESS scenes may be affected by solar array obstructions from the International Space Station (ISS), potentially impacting data quality of obstructed pixels. The 'FieldOfViewObstruction' metadata field is included in all Version 2 products to indicate possible obstructions: * Before October 24, 2024 (orbits prior to 35724): The field is present but was not populated and does not reliably identify affected scenes. * On or after October 24, 2024 (starting with orbit 35724): The field is populated and generally accurate, except for late December 2024, when a temporary processing error may have caused false positives. * A [list of scenes](https://lpdaac.usgs.gov/documents/2249/obst_all_sort.txt) confirmed to be affected by obstructions is available and is recommended for verifying historical data (before October 24, 2024) and scenes from late December 2024.* The ISS native pointing information is coarse relative to ECOSTRESS pixels, so ECOSTRESS geolocation is improved through image matching with a basemap. Metadata in the L1B_GEO file shows the success of this geolocation improvement, using categorizations \"best\", \"good\", \"suspect\", and \"poor\". We recommend that users use only \"best\" and \"good\" scenes for evaluations where geolocation is important (e.g., comparison to field sites). For some scenes, this metadata is not reflected in the higher-level products (e.g., land surface temperature, evapotranspiration, etc.). While this metadata is always available in the geolocation product, to save users additional download, we have produced a [summary text file](https://lpdaac.usgs.gov/documents/2253/qa_20250423-present.txt) that includes the geolocation quality flags for all scenes from launch to present. At a later date, all higher-level products will reflect the geolocation quality flag correctly (the field name is GeolocationAccuracyQA).* During the time period of May 15th, 2025, through July 1st, 2025, ECOSTRESS data was noisier than expected. Cycling the payload resolved the issue, but researchers should use all levels of ECOSTRESS data acquired during this time period with caution.* During the time period of January 1st, 2023, through September 30th, 2023, ECOSTRESS STARS and the resulting ET products are considered lower quality due to the priors used in the STARS model. The bug was corrected, and the lower quality data will be reprocessed.Improvements/Changes from Previous Versions* ECO_L3T_ET_ALEXI Version 2 was improved by ingesting coincident, gap-filled NDVI and albedo estimates at 70 m ECOSTRESS standard resolution for each daytime ECOSTRESS overpass through data fusion. This method fuses temporally sparse but fine spatial resolution images from the Harmonized Landsat Sentinel (HLS) Version 2 product with daily, moderate spatial resolution images from the NASA/NOAA Suomi National Polar-orbiting Partnership (NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) VNP09GA Version 2 product. The data fusion is performed using a variant of the Spatial Timeseries for Automated high-Resolution multi-Sensor data fusion (STARS) methodology. STARS is a state-space time series methodology that provides streaming data fusion and uncertainty quantification through efficient Kalman filtering.* Quality Flag variables are not used for ECO_L3T_ET_ALEXI Version 2 as only the best quality ECOSTRESS LST&E data are used as inputs.",
"shortName": "ECO_L3T_ET_ALEXI",
"longName": "ECOSTRESS Tiled Evapotranspiration disALEXI 24-Hour L3 CONUS 70 m V002",
"doi": "10.5067/ECOSTRESS/ECO_L3T_ET_ALEXI.002"
}
|
node
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45
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2872613065-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "264b4aa3-de07-5c09-a64c-441c01d2b1cd",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Gross and Net Primary Production (NPP) Gap-Filled (VNP17A3GF) Version 2 product is a cumulative composite of Gross Primary Productivity (GPP) values based on the radiation use efficiency concept that is potentially used as inputs to data models to calculate terrestrial energy, carbon, water cycle processes, and biogeochemistry of vegetation. VNP17A3GF is a yearly composite at 500 meter (m) spatial resolution delivered as a gridded Level 4 (L4) product in Sinusoidal projection. The VNP17A3GF will be generated at the end of each year when the entire yearly 8-day VNP15A2H is available. Hence, the gap-filled VNP17A3GF is the improved VNP17A2, which has cleaned the poor-quality inputs from 8-day Leaf Area Index and Fraction of Photosynthetically Active Radiation (LAI/FPAR) based on the Quality Control (QC) label for every pixel. If any LAI/FPAR pixel did not meet the quality screening criteria, its value is determined through linear interpolation. However, users cannot get VNP17A3GF in near-real time because it will be generated only at the end of a given year.Provided in the VNP17A3GF product are layers for GPP, NPP, along with a quality control layer. A low resolution browse image for GPP is also available for each VNP17A3GF granule.Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP17A3GF",
"longName": "VIIRS/NPP Gross and Net Primary Production Gap-Filled Yearly L4 Global 500m SIN Grid V002",
"doi": "10.5067/VIIRS/VNP17A3GF.002"
}
|
node
|
46
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380527-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "322e7a15-70bb-5a93-a3ad-7ee61e23ef0f",
"abstract": "The VNP43D63 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D63](https://doi.org/10.5067/VIIRS/VNP43D63.002) and [VJ143D63](https://doi.org/10.5067/VIIRS/VJ143D63.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Black-Sky Albedo for Band VIS (VNP43D63) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible (VIS), near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D63 is the BSA for the VIIRS visible broadband (0.64 μm).Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D63",
"longName": "VIIRS/NPP BRDF/Albedo BSA at Solar Noon Band VIS Daily L3 Global 30ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D63.001"
}
|
node
|
47
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-11T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763266322-LPCLOUD",
"temporalExtentEnd": "2000-02-21T23:59:59.000Z",
"globalId": "e8633c4e-23b0-5b9b-aac3-5664bf268dff",
"abstract": "The Land Processes Distributed Active Archive Center (LP DAAC) is responsible for the archive and distribution of NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Digital Elevation Model (DEM) version 1 (NASADEM_SHHP) dataset, which provides Shuttle Radar Topography Mission (SRTM) global elevation height data at 1 arc second spacing.NASADEM data products were derived from original telemetry data from SRTM, a collaboration between NASA and the National Geospatial-Intelligence Agency (NGA), as well as participation from the German and Italian space agencies. SRTM's primary focus was to generate a near-global DEM of the Earth using radar interferometry. It was a primary component of the payload on space shuttle _Endeavour_ during its STS-99 mission, which was launched on February 11, 2000, and flew for 11 days. In addition to Terra Advanced Spaceborne Thermal and Reflection Radiometer (ASTER) Global Digital Elevation Model (GDEM) Version 2 data, NASADEM also relied on Ice, Cloud, and Land Elevation Satellite (ICESat) Geoscience Laser Altimeter System (GLAS) ground control points of its lidar shots to improve surface elevation measurements that led to improved geolocation accuracy. Other reprocessing improvements include the conversion to geoid reference and the use of GDEMs and Advanced Land Observing Satellite Panchromatic Remote-sensing Instrument for Stereo Mapping (PRISM) AW3D30 DEM, and interpolation for void filling.NASADEM are distributed in 1 degree latitude by 1 degree longitude tiles and consist of all land between 60° N and 56° S latitude. This accounts for about 80% of Earth's total landmass. NASADEM_SHHP data product layers include SRTM-only floating-point DEM and height error. A low-resolution browse image showing the SRTM-only elevation is also available for each NASADEM_SHHP granule.",
"shortName": "NASADEM_SHHP",
"longName": "NASADEM SRTM-only Height and Height Precision Mosaic Global 1 arc second V001",
"doi": "10.5067/MEASURES/NASADEM/NASADEM_SHHP.001"
}
|
node
|
48
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-11T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763268444-LPCLOUD",
"temporalExtentEnd": "2000-02-21T23:59:59.000Z",
"globalId": "901cb123-5ca1-5ac2-a2af-3ab4d0602a64",
"abstract": "The Land Processes Distributed Active Archive Center (LP DAAC) is responsible for the archive and distribution of NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) SRTM, which includes the global 1 arc second (~30 meter) swath (raw) image data product. (See User Guide Section 2.2.1)The SRTM swath image data set consists of radar image files containing brightness values, as well as quality assurance (incidence angle) files for each of four overlapping sub-swaths that passes through a 1 degree by 1 degree tile. Data from each sub-swath is included as a separate file. Some files may contain only partial data; however, every image pixel acquired by SRTM is included in this data set.The NASA SRTM data sets result from a collaborative effort by the National Aeronautics and Space Administration (NASA) and the National Geospatial-Intelligence Agency (NGA - previously known as the National Imagery and Mapping Agency, or NIMA), as well as the participation of the German and Italian space agencies. This collaboration aims to generate a near-global digital elevation model (DEM) of Earth using radar interferometry. SRTM was the primary (and virtually only) payload on the STS-99 mission of the Space Shuttle Endeavour, which launched February 11, 2000 and flew for 11 days.The SRTM swaths extended from ~30 degrees off-nadir to ~58 degrees off-nadir from an altitude of 233 kilometers (km), creating swaths ~225 km wide, and consisted of all land between 60° N and 56° S latitude to account for 80% of Earth's total landmass. Known Issues* Known issues in the NASA SRTM are described in the following publication: * Rodriguez, E., C. S. Morris, and J. E. Belz (2006), A global assessment of the SRTM performance, Photogramm. Eng. Remote Sens., 72, 249–260. https://doi.org/10.14358/PERS.72.3.249Improvements/Changes from Previous Version* Version 3.0 products are filled with ASTER Global Digital Elevation Model (GDEM) Version 2.0, the Global Multi-resolution Terrain Elevation Data 2010 (GMTED2010), and the National Elevation Dataset (NED).",
"shortName": "SRTMIMGR",
"longName": "NASA Shuttle Radar Topography Mission Swath Image Data V003",
"doi": "10.5067/MEASURES/SRTM/SRTMIMGR.003"
}
|
node
|
49
|
[
"Dataset"
] |
{
"temporalExtentStart": "2018-07-10T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2076109886-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "55beff87-9492-50f9-8c10-5733e83cf4bc",
"abstract": "The ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) mission measures the temperature of plants to better understand how much water plants need and how they respond to stress. ECOSTRESS is attached to the International Space Station (ISS) and collects data globally between 52° N and 52° S latitudes. A map of the acquisition coverage can be found on the [ECOSTRESS website](https://ecostress.jpl.nasa.gov/science).The ECOSTRESS Gridded Water Use Efficiency Instantaneous L4 Global 70 m (ECO_L4G_WUE) Version 2 data product provides Water Use Efficiency (WUE) data generated by dividing the Breathing Earth System Simulator (BESS) Gross Primary Production (GPP) by the Priestley-Taylor Jet Propulsion Laboratory Soil Moisture (PT-JPL-SM) transpiration to estimate WUE, the ratio of grams of carbon that plants absorb to kilograms of water that plants release. The product provides a BESS GPP estimate that represents the amount of carbon surrounding the plants. The ECO_L4G_WUE Version 2 data product is available globally and projected to a globally snapped 0.0006° grid with a 70 meter spatial resolution and is distributed in HDF5. Each granule contains layers of Water Use Efficiency (WUE), Water Gross Primary Production (GPP), cloud mask, and water mask. A low-resolution browse is also available showing daily WUE as a stretched image with a color ramp in JPEG format.Known Issues* Data acquisition gap: ECOSTRESS was launched on June 29, 2018, and moved to autonomous science operations on August 20, 2018, following a successful in-orbit checkout period. On September 29, 2018, ECOSTRESS experienced an anomaly with its primary mass storage unit (MSU). ECOSTRESS has a primary and secondary MSU (A and B). On December 5, 2018, the instrument was switched to the secondary MSU, and science operations resumed. On March 14, 2019, the secondary MSU experienced a similar anomaly, temporarily halting science acquisitions. On May 15, 2019, a new data acquisition approach was implemented, and science acquisitions resumed. To optimize the new acquisition approach, only Thermal Infrared (TIR) bands 2, 4, and 5 are being downloaded. The data products are the same as before, but the bands not downloaded contain fill values (L1 radiance and L2 emissivity). This approach was implemented from May 15, 2019, through April 28, 2023.* Data acquisition gap: From February 8 to February 16, 2020, an ECOSTRESS instrument issue resulted in a data anomaly that created striping in band 4 (10.5 micron). These data products have been reprocessed and are available for download. No ECOSTRESS data were acquired on February 17, 2020, due to the instrument being in SAFEHOLD. Data acquired following the anomaly have not been affected.* Data acquisition: ECOSTRESS has now successfully returned to 5-band mode after being in 3-band mode since 2019. This feature was successfully enabled following a Data Processing Unit firmware update (version 4.1) to the payload on April 28, 2023. To better balance contiguous science data scene variables, 3-band collection is currently being interleaved with 5-band acquisitions over the orbital day/night periods.* Solar Array Obstruction: Some ECOSTRESS scenes may be affected by solar array obstructions from the International Space Station (ISS), potentially impacting data quality of obstructed pixels. The 'FieldOfViewObstruction' metadata field is included in all Version 2 products to indicate possible obstructions: * Before October 24, 2024 (orbits prior to 35724): The field is present but was not populated and does not reliably identify affected scenes. * On or after October 24, 2024 (starting with orbit 35724): The field is populated and generally accurate, except for late December 2024, when a temporary processing error may have caused false positives. * A [list of scenes](https://lpdaac.usgs.gov/documents/2249/obst_all_sort.txt) confirmed to be affected by obstructions is available and is recommended for verifying historical data (before October 24, 2024) and scenes from late December 2024.* The ISS native pointing information is coarse relative to ECOSTRESS pixels, so ECOSTRESS geolocation is improved through image matching with a basemap. Metadata in the L1B_GEO file shows the success of this geolocation improvement, using categorizations \"best\", \"good\", \"suspect\", and \"poor\". We recommend that users use only \"best\" and \"good\" scenes for evaluations where geolocation is important (e.g., comparison to field sites). For some scenes, this metadata is not reflected in the higher-level products (e.g., land surface temperature, evapotranspiration, etc.). While this metadata is always available in the geolocation product, to save users additional download, we have produced a [summary text file](https://lpdaac.usgs.gov/documents/2253/qa_20250423-present.txt) that includes the geolocation quality flags for all scenes from launch to present. At a later date, all higher-level products will reflect the geolocation quality flag correctly (the field name is GeolocationAccuracyQA).*During the time period of May 15th, 2025, through July 1st, 2025, ECOSTRESS data was noisier than expected. Cycling the payload resolved the issue, but researchers should use all levels of ECOSTRESS data acquired during this time period with caution.* During the time period of January 1st, 2023, through September 30th, 2023, ECOSTRESS STARS and the resulting ET products are considered lower quality due to the priors used in the STARS model. The bug was corrected, and the lower quality data will be reprocessed.",
"shortName": "ECO_L4G_WUE",
"longName": "ECOSTRESS Gridded Water Use Efficiency Instantaneous L4 Global 70 m V002",
"doi": "10.5067/ECOSTRESS/ECO_L4G_WUE.002"
}
|
node
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50
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[
"Dataset"
] |
{
"temporalExtentStart": "2018-07-10T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2074852168-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "b966e9c9-5905-5832-a92c-14d23206bffb",
"abstract": "The ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) mission measures the temperature of plants to better understand how much water plants need and how they respond to stress. ECOSTRESS is attached to the International Space Station (ISS) and collects data globally between 52° N and 52° S latitudes. A map of the acquisition coverage can be found in Figure 2 on the [ECOSTRESS website](https://ecostress.jpl.nasa.gov/science).The ECOSTRESS Tiled Surface Energy Balance Instantaneous L3 Global 70 m (ECO_L3T_SEB) Version 2 data product provides estimated incoming surface radiation (Rg) and net radiation (Rn) aligned with each daytime ECOSTRESS overpass. The Rg was generated using the Forest Light Environmental Simulator (FLiES) radiative transfer model implemented in an artificial neural network using Cloud Optical Thickness (COT) and Aerosol Optical Thickness (AOT) from Goddard Earth Observing System Version 5 (GEOS-5) Forward Processing (FP) along with albedo from ECOSTRESS Tiled Ancillary NDVI and Albedo Level 2 Global 70 m ([ECO_L2T_STARS](https://doi.org/10.5067/ECOSTRESS/ECO_L2T_STARS.002)) Version 2 as variables. The Rg output from the FLiES model was bias corrected to Rg from GEOS-FP. The Rn is an output from the Breathing Earth System Simulator (BESS) algorithm. This data product is tiled using a modified version of the Military Grid Reference System ([MGRS](https://hls.gsfc.nasa.gov/products-description/tiling-system/)), which divides Universal Transverse Mercator (UTM) zones into square tiles that are 109.8 km by 109.8 km with a 70 meter (m) spatial resolution.The ECO_L3T_SEB Version 2 data product is provided in Cloud Optimized GeoTIFF (COG) format with each data layer distributed as a separate COG. This product contains four layers including Rg, Rn, cloud mask, and water mask.Known Issues* Data acquisition gap: ECOSTRESS was launched on June 29, 2018, and moved to autonomous science operations on August 20, 2018, following a successful in-orbit checkout period. On September 29, 2018, ECOSTRESS experienced an anomaly with its primary mass storage unit (MSU). ECOSTRESS has a primary and secondary MSU (A and B). On December 5, 2018, the instrument was switched to the secondary MSU and science operations resumed. On March 14, 2019, the secondary MSU experienced a similar anomaly, temporarily halting science acquisitions. On May 15, 2019, a new data acquisition approach was implemented, and science acquisitions resumed. To optimize the new acquisition approach TIR bands 2, 4, and 5 are being downloaded. The data products are as previously, except the bands not downloaded contain fill values (L1 radiance and L2 emissivity). This approach was implemented from May 15, 2019, through April 28, 2023.* Data acquisition gap: From February 8 to February 16, 2020, an ECOSTRESS instrument issue resulted in a data anomaly that created striping in band 4 (10.5 micron). These data products have been reprocessed and are available for download. No ECOSTRESS data were acquired on February 17, 2020, due to the instrument being in SAFEHOLD. Data acquired following the anomaly have not been affected.* Data acquisition: ECOSTRESS has now successfully returned to 5-band mode after being in 3-band mode since 2019. This feature was successfully enabled following a Data Processing Unit firmware update (version 4.1) to the payload on April 28, 2023. To better balance contiguous science data scene variables, 3-band collection is currently being interleaved with 5-band acquisitions over the orbital day/night periods.* Missing Cloud Layer Alert: All users of ECOSTRESS Tiled and Gridded L3 Soil Moisture and Surface Energy Balance v002 products (ECO_L3T_SM, ECO_L3G_SM, ECO_L3T_SEB and ECO_L3G_SEB) should be aware that the ‘cloud mask’ layer may be unavailable for a select number of granules for the year 2023. Users are encouraged to get that information from the corresponding Level 2 Standard Cloud Mask products (ECO_L2_CLOUD and ECO_L2G_CLOUD) to assess if a pixel is clear or cloudy (see section 3 of the User Guide).* Solar Array Obstruction: Some ECOSTRESS scenes may be affected by solar array obstructions from the International Space Station (ISS), potentially impacting data quality of obstructed pixels. The 'FieldOfViewObstruction' metadata field is included in all Version 2 products to indicate possible obstructions: * Before October 24, 2024 (orbits prior to 35724): The field is present but was not populated and does not reliably identify affected scenes. * On or after October 24, 2024 (starting with orbit 35724): The field is populated and generally accurate, except for late December 2024, when a temporary processing error may have caused false positives. * A [list of scenes](https://lpdaac.usgs.gov/documents/2249/obst_all_sort.txt) confirmed to be affected by obstructions is available and is recommended for verifying historical data (before October 24, 2024) and scenes from late December 2024.* The ISS native pointing information is coarse relative to ECOSTRESS pixels, so ECOSTRESS geolocation is improved through image matching with a basemap. Metadata in the L1B_GEO file shows the success of this geolocation improvement, using categorizations \"best\", \"good\", \"suspect\", and \"poor\". We recommend that users use only \"best\" and \"good\" scenes for evaluations where geolocation is important (e.g., comparison to field sites). For some scenes, this metadata is not reflected in the higher-level products (e.g., land surface temperature, evapotranspiration, etc.). While this metadata is always available in the geolocation product, to save users additional download, we have produced a [summary text file](https://lpdaac.usgs.gov/documents/2253/qa_20250423-present.txt) that includes the geolocation quality flags for all scenes from launch to present. At a later date, all higher-level products will reflect the geolocation quality flag correctly (the field name is GeolocationAccuracyQA).*During the time period of May 15th, 2025, through July 1st, 2025, ECOSTRESS data was noisier than expected. Cycling the payload resolved the issue, but researchers should use all levels of ECOSTRESS data acquired during this time period with caution.",
"shortName": "ECO_L3T_SEB",
"longName": "ECOSTRESS Tiled Surface Energy Balance Instantaneous L3 Global 70 m V002",
"doi": "10.5067/ECOSTRESS/ECO_L3T_SEB.002"
}
|
node
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51
|
[
"Dataset"
] |
{
"temporalExtentStart": "2013-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763261715-LPCLOUD",
"temporalExtentEnd": "2016-12-31T23:59:59.999Z",
"globalId": "7a1103ae-2987-5d09-bed1-5eee725f2d88",
"abstract": "The NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Global Food Security-support Analysis Data (GFSAD) data product provides cropland extent data over Southeast and Northeast Asia for nominal year 2015 at 30 meter resolution (GFSAD30SEACE). The monitoring of global cropland extent is critical for policymaking and provides important baseline data that are used in many agricultural cropland studies pertaining to water sustainability and food security. The GFSAD30SEACE data product uses the pixel-based supervised classifiers, Random Forest (RF), to retrieve cropland extent from a combination of Landsat 8 Operational Land Imager (OLI), Landsat 7 Enhanced Thematic Mapper Plus (ETM+), and elevation derived from the Shuttle Radar Topography Mission (SRTM) Version 3 data products. Each GFSAD30SEACE GeoTIFF file contains a cropland extent layer that defines areas of cropland, non-cropland, and water bodies over a 10° by 10° area.Known Issues* Certain small islands in the Pacific are not classified and therefore data for these areas are not provided.* Additional known issues, including constraints and limitations, are provided on page 19 of the ATBD.",
"shortName": "GFSAD30SEACE",
"longName": "Global Food Security-support Analysis Data (GFSAD) Cropland Extent 2015 Southeast and Northeast Asia product 30 m V001",
"doi": "10.5067/MEaSUREs/GFSAD/GFSAD30SEACE.001"
}
|
node
|
52
|
[
"Dataset"
] |
{
"temporalExtentStart": "2023-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2519119034-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "3e9e8dff-b011-5cff-b79b-c69868fda626",
"abstract": "The Observational Products for End-Users from Remote Sensing Analysis ([OPERA](https://www.jpl.nasa.gov/go/opera)) Land Surface Disturbance Annual from Harmonized Landsat Sentinel-2 (HLS) product Version 1 summarizes the [DIST-ALERT](https://doi.org/10.5067/SNWG/OPERA_L3_DIST-ALERT-HLS_V1.001) data product into an annual vegetation disturbance data product. Vegetation disturbance is mapped when there is an indicated decrease in vegetation cover within an HLS Version 2 pixel. The product also provides auxiliary generic disturbance information as determined from the variations of the reflectance through the DIST-ALERT scenes to provide information about more general disturbance trends. The DIST-ANN product tracks changes at the annual scale, aggregating changes identified in the DIST-ALERT product. Only confirmed disturbances from the associated year are reported together with the date of initial disturbance. As confirmed disturbances are determined using subsequent cloud-free observations to determine if the loss detections persist, the required number of HLS scenes depends on visibility of the target. Due to this dependency, summarizing the DIST-ALERT in the DIST-ANN product will have some latency contingent on the algorithmic calibration and is detailed in the Algorithm Theoretical Basis Document (ATBD).The OPERA_L3_DIST-ANN-HLS (or DIST-ANN) data product is provided in Cloud Optimized GeoTIFF (COG) format, and each layer is distributed as a separate COG. There are 21 layers contained within the DIST-ANN product: vegetation disturbance status, historical vegetation cover indicator, maximum vegetation cover indicator, maximum vegetation anomaly value, vegetation disturbance confidence layer, date of initial vegetation disturbance, number of detected vegetation loss anomalies, vegetation disturbance duration, date of last observation assessed for vegetation disturbance, and several generic disturbance layers. Each product layer is gridded to the same resolution and tiling system as HLS V2: 30 meter (m) and Military Grid Reference System ([MGRS](https://hls.gsfc.nasa.gov/products-description/tiling-system/)). See the Product Specification Document (PSD) for a more detailed description of the individual layers provided in the DIST-ANN product. The OPERA_L3_DIST-ANN-HLS product contains modified Copernicus Sentinel data (2020-2025).Known Issues* Additional usage constraints are provided under Section 5 of the Algorithm Theoretical Basis Document (ATBD).",
"shortName": "OPERA_L3_DIST-ANN-HLS_V1",
"longName": "OPERA Land Surface Disturbance Annual from Harmonized Landsat Sentinel-2 product (Version 1)",
"doi": "10.5067/SNWG/OPERA_L3_DIST-ANN-HLS_V1.001"
}
|
node
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53
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[
"Dataset"
] |
{
"temporalExtentStart": "2002-07-04T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2565794042-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "21b6906c-8a31-57c6-bf10-d60d5d2c957c",
"abstract": "The Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) Land Surface Temperature/Emissivity 8-Day (MYD11C2) Version 6.1 product provides Land Surface Temperature and Emissivity (LST&E) values in a 0.05 degree (5,600 meters at the equator) latitude/longitude Climate Modeling Grid (CMG). A CMG granule follows a geographic grid with 7,200 columns and 3,600 rows, representing the entire globe. The LST&E values in the MYD11C2 product are derived by compositing and averaging the values from the corresponding eight [MYD11C1](https://doi.org/10.5067/MODIS/MYD11C1.061) daily files. The MYD11C2 granule consists of 17 layers. Each MYD11C2 product consists of the following layers for daytime and nighttime observations: LSTs, quality control assessments, observation times, view zenith angles, and number of clear-sky observations along with percentage of land in the grid and emissivities from bands 20, 22, 23, 29, 31, and 32. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Aqua&as=61).Improvments/Changes from Previous Version* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MYD11C2",
"longName": "MODIS/Aqua Land Surface Temperature/Emissivity 8-Day L3 Global 0.05Deg CMG V061",
"doi": "10.5067/MODIS/MYD11C2.061"
}
|
node
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54
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380517-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "f82d51f3-98ef-5321-bdeb-1d3a097ec773",
"abstract": "The VNP43D61 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D61](https://doi.org/10.5067/VIIRS/VNP43D61.002) and [VJ143D61](https://doi.org/10.5067/VIIRS/VJ143D61.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Black-Sky Albedo for Band M10 (VNP43D61) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D61 is the BSA for VIIRS band M10 (1.61 μm). Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D61",
"longName": "VIIRS/NPP BRDF/Albedo BSA at Solar Noon Band M10 Daily L3 Global 30ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D61.001"
}
|
node
|
55
|
[
"Dataset"
] |
{
"temporalExtentStart": "2011-06-30T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2763264748-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "c5c94c76-4648-58c0-a8a1-6a5e6b691d9a",
"abstract": "Goddard’s LiDAR, Hyperspectral, and Thermal Imagery ([G-LiHT](https://gliht.gsfc.nasa.gov/)) mission is a portable, airborne imaging system that aims to simultaneously map the composition, structure, and function of terrestrial ecosystems. G-LiHT primarily focuses on a broad diversity of forest communities and ecoregions in North America, mapping aerial swaths over Conterminous United States (CONUS), Alaska, Puerto Rico, and Mexico.The purpose of G-LiHT’s Trajectory data product (GLTRAJECTORY) is to provide aircraft location and orientation to support and supplement other G-LiHT data products.GLTRAJECTORY data are processed as a Google Earth overlay Keyhole Markup Language (KML) file over the extent of an entire flight path. A low resolution browse is also provided to show the flight path. ",
"shortName": "GLTRAJECTORY",
"longName": "G-LiHT Trajectory Data V001",
"doi": "10.5067/Community/GLIHT/GLTRAJECTORY.001"
}
|
node
|
56
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763379206-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "8389d243-a731-5d00-8692-a222cf57c0f3",
"abstract": "The VNP43D12 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D12](https://doi.org/10.5067/VIIRS/VNP43D12.002) and [VJ143D12](https://doi.org/10.5067/VIIRS/VJ143D12.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 3 Band M4 product (VNP43D12) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D12 is the BRDF geometric parameter for VIIRS band M4 (0.555 μm). The geometric parameter, in conjunction with the isotropic and volumetric parameters, is used to derive the BRDF/Albedo values for VIIRS band M4.Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D12",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 3 Band M4 Daily L3 Global 30 ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D12.001"
}
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node
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57
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[
"Dataset"
] |
{
"temporalExtentStart": "2008-12-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "monthly",
"cmrId": "C2763266354-LPCLOUD",
"temporalExtentEnd": "2011-11-30T23:59:59.999Z",
"globalId": "854a37a3-b0e9-595e-a36a-0e71f75f0839",
"abstract": "The NASA Making Earth System Data Records for Use in Research Environments ([MEaSUREs](https://earthdata.nasa.gov/about/competitive-programs/measures)) Global Web-Enabled Landsat Data Monthly (GWELDMO) Version 3 data product provides Landsat data at 30 meter (m) resolution for terrestrial non-Antarctica locations over monthly reporting periods for the 2010 epoch. GWELD data products are generated from all available Landsat 4 and 5 Thematic Mapper (TM) and Landsat 7 Enhanced Thematic Mapper Plus (ETM+) data in the U.S. Geological Survey (USGS) Landsat archive. The GWELD suite of products provide consistent data to derive land cover as well as geophysical and biophysical information for regional assessment of land surface dynamics.The GWELD products include Nadir Bidirectional Reflectance Distribution Function (BRDF)-Adjusted Reflectance (NBAR) for the reflective wavelength bands and top of atmosphere (TOA) brightness temperature for the thermal bands. The products are defined in the Sinusoidal coordinate system to promote continuity of NASA's Moderate Resolution Imaging Spectroradiometer (MODIS) land tile grid.Provided in the GWELDMO product are layers for surface reflectance bands 1 through 5 and 7, TOA brightness temperature for thermal bands, Normalized Difference Vegetation Index (NDVI), day of year, ancillary angle, and data quality information. A low-resolution red, green, blue (RGB) browse image of bands 5, 4, 3 is also available for each granule.Known Issues* GWELDMO known issues can be found in Section 4 of the Algorithm Theoretical Basis Document (ATBD). Please note that the version 3.0 GWELD products for 2009, 2010 and 2011 are defined in HDF4 which cannot be read correctly by GDAL/ArcGIS. This is not an issue for the version 3.1 GWELD products",
"shortName": "GWELDMO",
"longName": "NASA Global Web-Enabled Landsat Data Monthly Global 30 m V003",
"doi": "10.5067/MEaSUREs/GWELD/GWELDMO.003"
}
|
node
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58
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[
"Dataset"
] |
{
"temporalExtentStart": "2002-12-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "monthly",
"cmrId": "C3545740790-LPCLOUD",
"temporalExtentEnd": "2012-11-30T23:59:59.999Z",
"globalId": "acd147f0-4bbf-56f9-b764-60645536ea46",
"abstract": "WELDUSLL.015 was decommissioned on December 2, 2019. Users are encouraged to use the improved monthly Global Web-Enabled Landsat Data (GWELD) [Version 3](https://doi.org/10.5067/MEaSUREs/GWELD/GWELDMO.003), [3.1](https://doi.org/10.5067/MEaSUREs/GWELD/GWELDMO.031), and [3.2](https://doi.org/10.5067/MEaSUREs/GWELD/GWELDMO.032) datasets. NASA’s Web-Enabled Landsat Data (WELD) are generated from composited 30 meter (m) Landsat Enhanced Thematic Mapper Plus (ETM+) mosaics of the United States and Alaska from 2002 to 2012. These mosaics provide consistent data to derive land cover as well as geophysical and biophysical products for regional assessments of surface dynamics for effective study of Earth system function. The Conterminous (CONUS) United States Latitude/Longitude (WELDUSLL) products provide the geographic latitude and longitude for the center of each 30 meter (m) pixel within a tile of WELD data. WELDUSLL is distributed in Hierarchical Data Format 4 (HDF4).The WELD project is funded by the National Aeronautics and Space Administration (NASA) and is a collaboration between the United States Geological Survey (USGS) Earth Resources Observation and Science (EROS) Center and the South Dakota State University (SDSU) Geospatial Sciences Center of Excellence (GSCE). Known Issues* WELD Version 1.5 known issues can be found in the WELD Version 1.5 User Guide.Improvements/Changes from Previous Version* Version 1.5 is the original version.",
"shortName": "WELDUSLL",
"longName": "NASA Web-Enabled Landsat Data CONUS 30m Composite Pixel Center Lat/Longs V001",
"doi": "10.5067/MEASURES/WELD/WELDUSLL.001"
}
|
node
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59
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380059-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "81587273-aff7-523e-a32d-4ebdb7b8a965",
"abstract": "The VNP43D39 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D39](https://doi.org/10.5067/VIIRS/VNP43D39.002) and [VJ143D39](https://doi.org/10.5067/VIIRS/VJ143D39.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 3 Day-Night Band (DNB) product (VNP43D39) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D39 is the BRDF geometric parameter for the VIIRS DNB (0.7 μm). The geometric parameter, in conjunction with the isotropic and volumetric parameters, is used to derive the BRDF/Albedo values for the VIIRS DNB.Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D39",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 3 DNB Daily L3 Global 30 ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D39.001"
}
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node
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60
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2849434111-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "600120de-57a8-561e-9af6-ab0944b91e60",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo white-sky albedo for Day/Night Band (DNB) product (VNP43D79) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. VNP43D54 through VNP43D79 are the albedo products of the VNP43D BRDF/Albedo product suite. Black-sky albedo (BSA) and white-sky albedo (WSA) values are provided for the nine VIIRS moderate resolution bands (M1 through M5, M7, M8, M10, and M11) along with the visible, near-infrared (NIR), and shortwave bands included in the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.002) product. In addition to the bands included in VNP43MA3, this product suite includes albedo values for the VIIRS Day/Night Band (DNB). The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Details regarding methodology are available on the [VNP43MA3](https://doi.org/10.5067/VIIRS/VNP43MA3.002) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D79 is the WSA for the VIIRS DNB (0.7 μm).Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue).Improvements/Changes from Previous Version* Improved calibration algorithm and better coefficients for entire Suomi NPP mission.* Improved geolocation accuracy and updates to fix outliers around maneuver periods and other events.* Corrections to the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid to high latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 BRDF/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data.* Replaced the land/water mask input product with MODIS heritage seven class land/water mask.",
"shortName": "VNP43D79",
"longName": "VIIRS/NPP BRDF/Albedo WSA at Solar Noon DNB Daily L3 Global 30ArcSec CMG V002",
"doi": "10.5067/VIIRS/VNP43D79.002"
}
|
node
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61
|
[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2540273183-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "bf07e850-0d94-58dc-bee2-01cc4af96a19",
"abstract": "The MCD43D59 Version 6.1 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) White-Sky Albedo dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter (m)) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. MCD43D42 through MCD43D61 are the albedo products of the MCD43D BRDF/Albedo product suite. There are 10 black-sky albedo and 10 white-sky albedo layers representing MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands. The black-sky albedo (directional hemispherical reflectance) is defined as albedo in the absence of a diffuse component and is a function of solar zenith angle. White-sky albedo (bihemispherical reflectance) is defined as albedo in the absence of a direct component when the diffuse component is isotropic. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).MCD43D59 is the white-sky albedo for the MODIS visible broadband. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=TerraAqua&as=61).Improvements/Changes from Previous Versions* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).",
"shortName": "MCD43D59",
"longName": "MODIS/Terra+Aqua BRDF/Albedo White Sky Albedo VIS Daily L3 Global 30ArcSec CMG V061",
"doi": "10.5067/MODIS/MCD43D59.061"
}
|
node
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62
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[
"Dataset"
] |
{
"temporalExtentStart": "2018-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2631841524-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "70100cc4-fc96-54de-b4fe-ff3d02f439d6",
"abstract": "The Visible Infrared Imaging Radiometer Suite (VIIRS) daily surface reflectance (VJ109GA) Version 2 product provides an estimate of land surface reflectance from the NOAA-20 VIIRS sensor. Data are provided for three imagery bands (I1-I3) at nominal 500 meter resolution (~463 meter) and nine moderate resolution bands (M1-M5, M7, M8, M10, M11) at nominal 1 kilometer (~926 meter) resolution. The 500 meter and 1 kilometer datasets are derived through resampling the native 375 meter and 750 meter VIIRS resolutions, respectively, in the Level 2 input product. These bands are corrected for atmospheric conditions such as the effects of molecular gases, including ozone and water vapor, and for the effects of atmospheric aerosols. The inputs to the surface reflectance algorithm are top-of-atmosphere reflectance for the VIIRS visible bands, the VIIRS cloud mask and aerosol product, aerosol optical thickness and atmospheric data obtained from the NOAA National Centers for Environmental Prediction (NCEP) reanalysis system. Along with the twelve reflectance bands are reflectance band quality, sensor azimuth angle, solar azimuth angle, sensor zenith angle, solar zenith angle, and observations layers. The reflectance layers from the VJ109GA data product are used as input data for many of the VIIRS land products. Known Issues* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS) and in Section 4.0 of the User Guide.Improvements/Changes from Previous Version* Improved calibration algorithm and coefficients for entire NOAA-20 mission.* Improved geolocation accuracy and applied updates to fix outliers around maneuver periods.* Corrected the aerosol quantity flag (low, average, high) mainly over brighter surfaces in the mid- to high-latitudes such as desert and tropical vegetation areas. This has an impact on the retrieval of other downstream data products such as VNP13 Vegetation Indices and VNP43 Bidirectional Reflectance Distribution Function (BRDF)/Albedo.* Improved cloud mask input product for corrections along coastlines and artifacts from use of coarse resolution climatology data. * Replaced the land/water mask input product with the eight-class land/water mask from the VNP03 geolocation product that better aligns with MODIS.* Added secondary day-night flag to improve retrieval of Climate Modeling Grid (CMG) values over daytime pixels.* More details can be found in this [VIIRS Land V2 Changes document](https://landweb.modaps.eosdis.nasa.gov/data/userguide/VIIRS_Land_C2_Changes_09152022.pdf).",
"shortName": "VJ109GA",
"longName": "VIIRS/JPSS1 Surface Reflectance Daily L2G Global 1km and 500m SIN Grid V002",
"doi": "10.5067/VIIRS/VJ109GA.002"
}
|
node
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63
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[
"Dataset"
] |
{
"temporalExtentStart": "2000-02-16T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763293211-LPCLOUD",
"temporalExtentEnd": "2023-02-17T23:59:59.999Z",
"globalId": "ab944316-5212-5f52-b7f0-c6e5c7549441",
"abstract": "The MCD43D10 Version 6 data product was decommissioned on July 31, 2023. Users are encouraged to use the [MCD43D10 Version 6.1](https://doi.org/10.5067/MODIS/MCD43D10.061) data product.The MCD43D10 Version 6 Bidirectional Reflectance Distribution Function and Albedo (BRDF/Albedo) Model Parameter dataset is produced daily using 16 days of Terra and Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day which is reflected in the Julian date in the file name. This Climate Modeling Grid (CMG) product covers the entire globe for use in climate simulation models. Due to the large file size, each MCD43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the MODIS bands 1 through 7 and the visible, near-infrared (NIR), and shortwave bands included in [MCD43C1](https://doi.org/10.5067/MODIS/MCD43C1.006) are stored in a separate file as MCD43D01 through MCD43D30. MCD43D10 is the BRDF isotropic parameter for MODIS band 4. The isotropic parameter, in conjunction with the volumetric and geometric parameters, is used to derive the BRDF/Albedo values for MODIS band 4. Users are urged to use the band specific quality flags to isolate the highest quality full inversion results for their own science applications as described in the [User Guide](https://www.umb.edu/spectralmass/modis-user-guide-v006-and-v0061/mcd43d-cmg-30-arc-second-products/).Known Issues* The incorrect representation of the aerosol quantities (low average high) [in the C6 MYD09 and MOD09 surface reflectance products](https://landweb.modaps.eosdis.nasa.gov/displayissue?id=86) may have impacted downstream products particularly over arid bright surfaces. This (and a few other issues) have been corrected for C6.1. Therefore users should avoid substantive use of the C6 MCD43 products and wait for the C6.1 products. In any event, users are always strongly encouraged to download and use the extensive QA data provided in MCD43A2, in addition to the briefer mandatory QAs provided as part of the MCD43A1, 3, and 4 products.* [Corrections](https://landweb.modaps.eosdis.nasa.gov/data/userguide/LSRHighAerosolFlagFinal.pdf) were implemented in Collection 6.1 reprocessing.* For complete information about MCD43D10 known issues refer to the [MODIS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&as=6).Improvements/Changes from Previous Version* Observations are weighted to estimate the BRDF/Albedo on the ninth day of the 16-day period.* MCD43 products use the snow status weighted to the ninth day instead of the majority snow/no-snow observations from the 16-day period.* Better quality at high latitudes from use of all available observations for the acquisition period. Collection 5 used only four observations per day.* The MCD43 products use L2G-lite surface reflectance as input.* When there are insufficient high quality reflectances, a database with archetypal BRDF parameters is used to supplement the observational data and perform a lower quality magnitude inversion. This database is continually updated with the latest full inversion retrieval for each pixel.* CMG Albedo is estimated using all the clear-sky observations within the 1,000 m grid for MCD43D as opposed to aggregating from the 500 m albedo.",
"shortName": "MCD43D10",
"longName": "MODIS/Terra+Aqua BRDF/Albedo Parameter1 Band4 Daily L3 Global 30ArcSec CMG V006",
"doi": "10.5067/MODIS/MCD43D10.006"
}
|
node
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64
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[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2872596186-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "ece2e2ab-48d7-5f19-b6db-895d1dc0e28d",
"abstract": "The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Actual and Potential Evapotranspiration product is a gap-filled 8-day composite dataset produced at 500 meter (m) pixel resolution. The VIIRS ET and PET algorithm is based on the Penman-Monteith equation, which includes inputs of daily meteorological reanalysis data along with VIIRS remotely sensed data products such as 8-day vegetation property dynamics and daily surface albedo.The VNP16A2GF will be generated at the end of each year when the entire yearly 8-day VNP15A2H is available. Hence, the gap-filled VNP16A2GF is the improved VNP16A2, which has cleaned the poor-quality inputs from 8-day Leaf Area Index and Fraction of Photosynthetically Active Radiation (LAI/FPAR) based on the Quality Control (QC) label for every pixel. If any LAI/FPAR pixel did not meet the quality screening criteria, its value is determined through linear interpolation. However, users cannot get VNP16A2GF in near-real time because it will be generated only at the end of a given year.Provided in the VNP16A2GF product are layers for composited Evapotranspiration (ET), Latent Heat Flux (LE), Potential ET (PET) and Potential LE (PLE) along with a quality control layer. Two low resolution browse images, ET and LE, are also available for each VNP16A2GF granule.The pixel values for the two Evapotranspiration layers (ET and PET) are the summation of 8-day total water loss within the composite period and the pixel values for the two Latent Heat layers (LE and PLE) are the average total energy over a unit area for a day during the composite period. Note that the last acquisition period of each year is a 5 or 6-day composite period, depending on the year. Known Issues* Please refer to the [VIIRS Land Products website](https://viirsland.gsfc.nasa.gov/Products/NASA/ET_ESDR.html) and [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS) for information about VNP16A2GF known issues.",
"shortName": "VNP16A2GF",
"longName": "VIIRS/NPP Actual and Potential Evapotranspiration Gap-Filled 8-Day L4 Global 500m SIN Grid V002",
"doi": "10.5067/VIIRS/VNP16A2GF.002"
}
|
node
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65
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[
"Dataset"
] |
{
"temporalExtentStart": "2002-01-01T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "Unknown",
"cmrId": "C2565794824-LPCLOUD",
"temporalExtentEnd": "",
"globalId": "7e127f29-be97-577e-ab9b-94dcfb73dfe9",
"abstract": "The MYD17A2HGF Version 6.1 Gross Primary Productivity (GPP) Gap-Filled product is a cumulative 8-day composite of values with 500 meter (m) pixel size based on the radiation use efficiency concept that can be potentially used as inputs to data models to calculate terrestrial energy, carbon, water cycle processes, and biogeochemistry of vegetation. The Aqua Moderate Resolution Imaging Spectroradiometer (MODIS) data product includes information about GPP and Net Photosynthesis (PSN). The PSN band values are the GPP less the Maintenance Respiration (MR). The data product also contains a PSN Quality Control (QC) layer. The quality layer contains quality information for both the GPP and the PSN.The MYD17A2HGF will be generated at the end of each year when the entire yearly 8-day [MYD15A2H](https://doi.org/10.5067/modis/myd15a2h.061) is available. Hence, the gap-filled MYD17A2HGF is the improved MYD17, which has cleaned the poor-quality inputs from 8-day Leaf Area Index and Fraction of Photosynthetically Active Radiation (LAI/FPAR) based on the Quality Control (QC) label for every pixel. If any LAI/FPAR pixel did not meet the quality screening criteria, its value is determined through linear interpolation. However, users cannot get MYD17A2HGF in near-real time because it will be generated only at the end of a given year.Known Issues* Operational and uncertainty issues are provided under Section 2 in the User Guide. * For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=MODIS&sat=Aqua&as=61).Improvments/Changes from Previous Version* The Version 6.1 Level-1B (L1B) products have been improved by undergoing various calibration changes that include: changes to the response-versus-scan angle (RVS) approach that affects reflectance bands for Aqua and Terra MODIS, corrections to adjust for the optical crosstalk in Terra MODIS infrared (IR) bands, and corrections to the Terra MODIS forward look-up table (LUT) update for the period 2012 - 2017.* A polarization correction has been applied to the L1B Reflective Solar Bands (RSB).* The product uses Climatology LAI/FPAR as back up to the operational LAI/FPAR.",
"shortName": "MYD17A2HGF",
"longName": "MODIS/Aqua Gross Primary Productivity Gap-Filled 8-Day L4 Global 500m SIN Grid V061",
"doi": "10.5067/MODIS/MYD17A2HGF.061"
}
|
node
|
66
|
[
"Dataset"
] |
{
"temporalExtentStart": "2012-01-19T00:00:00.000Z",
"daac": "LP DAAC",
"temporalFrequency": "daily",
"cmrId": "C2763380040-LPCLOUD",
"temporalExtentEnd": "2025-02-01T00:00:00.000Z",
"globalId": "b614de1a-f029-53f6-ae3e-476ae144fb60",
"abstract": "The VNP43D32 Version 1 data product was decommissioned on July 31, 2025. Users are encouraged to use the [VNP43D32](https://doi.org/10.5067/VIIRS/VNP43D32.002) and [VJ143D32](https://doi.org/10.5067/VIIRS/VJ143D32.002) Version 2 data products.The NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi NPP) Visible Infrared Imaging Radiometer Suite (VIIRS) Bidirectional Reflectance Distribution Function (BRDF) and Albedo Model Parameter 2 Near-Infrared (NIR) broadband product (VNP43D32) is produced daily using 16 days of data at 30 arc second (1,000 meter) resolution. Data are temporally weighted to the ninth day, which is reflected in the file name. The VNP43D product suite is provided in a Climate Modeling Grid (CMG), which covers the entire globe for use in climate simulation models. Due to the large file size, each VNP43D product contains just one data layer. Each of the three model parameters (isotropic, volumetric, and geometric) for each of the nine VIIRS moderate resolution bands along with the visible, NIR, and shortwave bands included in the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product is stored in a separate file as VNP43D01 through VNP43D36. In addition to the bands included in VNP43MA1, this product suite includes model parameters for the VIIRS Day/Night Band (DNB) as VNP43D37 through VNP43D39. Details regarding methodology are available on the [VNP43MA1](https://doi.org/10.5067/VIIRS/VNP43MA1.001) product page and in the Algorithm Theoretical Basis Document (ATBD).VNP43D32 is the BRDF volumetric parameter for the VIIRS NIR broadband (0.865 μm). The volumetric parameter, in conjunction with the isotropic and geometric parameters, is used to derive the BRDF/Albedo values for the VIIRS NIR broadband.Known Issues* The abnormally high activation of the high aerosol flag in the Collection 1 (C1) VNP09 product has impacted downstream products. The VNP43 BRDF/Albedo/NBAR product is affected by reducing the number of otherwise acceptable observations used as input to characterize surface anisotropy. This effect (most obvious over arid bright surfaces), results in a reduced number of high quality full BRDF model inversions. Therefore, users should be aware that bright arid surfaces (normally associated with high quality BRDF/Albedo/NBAR retrievals) are likely to be somewhat represented by lower quality results in C1. VNP09 has been corrected for Collection 2 (C2). Therefore, users should avoid substantive use of C1 VNP43 over arid regions (and wait for C2 products). In any event, users are **always strongly encouraged** to download and use the extensive QA data provided in VNP43[I-M]A2, in addition to the briefer mandatory QA provided as part of the VNP43[I-M]A1, 3 and 4 products.* For complete information about known issues please refer to the [MODIS/VIIRS Land Quality Assessment website](https://landweb.modaps.eosdis.nasa.gov/knownissue?sensor=VIIRS).",
"shortName": "VNP43D32",
"longName": "VIIRS/NPP BRDF/Albedo Parameter 2 NIR Daily L3 Global 30 ArcSec CMG V001",
"doi": "10.5067/VIIRS/VNP43D32.001"
}
|
NASA Knowledge Graph Dataset
Dataset Summary
The NASA Knowledge Graph Dataset is an expansive graph-based dataset designed to integrate and interconnect information about satellite datasets, scientific publications, instruments, platforms, projects, data centers, and science keywords. This knowledge graph is particularly focused on datasets managed by NASA's Distributed Active Archive Centers (DAACs), which are NASA's data repositories responsible for archiving and distributing scientific data. In addition to NASA DAACs, the graph includes datasets from 184 data providers worldwide, including various government agencies and academic institutions.
The primary goal of the NASA Knowledge Graph is to bridge scientific publications with the datasets they reference, facilitating deeper insights and research opportunities within NASA's scientific and data ecosystem. By organizing these interconnections within a graph structure, this dataset enables advanced analyses, such as discovering influential datasets, understanding research trends, and exploring scientific collaborations.
What's Changed (v1.2.0) - October 21, 2025
1. Node Changes
Total Nodes: Increased from 145,678 to 150,351 (+4,673)
New Node Counts:
- Dataset: Increased from 6,821 to 8,058 (+1,237)
- DataCenter: Decreased from 197 to 189 (-8)
- Instrument: Increased from 897 to 921 (+24)
- Platform: Increased from 451 to 455 (+4)
- Project: Increased from 351 to 415 (+64)
- Publication: Increased from 135,352 to 138,704 (+3,352)
- ScienceKeyword: Remained the same at 1,609
2. Relationship Changes
Total Relationships: Increased from 406,515 to 436,203 (+29,688)
Updated Relationship Counts:
- CITES: Increased from 208,429 to 208,616 (+187)
- HAS_APPLIEDRESEARCHAREA: Increased from 119,695 to 121,553 (+1,858)
- HAS_DATASET: Increased from 9,834 to 11,698 (+1,864)
- HAS_INSTRUMENT: Increased from 2,526 to 2,631 (+105)
- HAS_PLATFORM: Increased from 10,398 to 11,944 (+1,546)
- HAS_SCIENCEKEYWORD: Increased from 21,571 to 25,553 (+3,982)
- HAS_SUBCATEGORY: Remained the same at 1,823
- OF_PROJECT: Increased from 6,378 to 8,031 (+1,653)
- USES_DATASET: Increased from 25,861 to 44,354 (+18,493)
3. Property Changes
Removed Properties:
pagerank_publication_datasetand all derived PageRank fields.
Schema Updates:
- All node properties standardized to string type for cross-database compatibility.
- No new node types added; schema remains stable with seven main entity types.
- Relationship properties remain null across all types.
These changes reflect expansion in dataset-publication linkages, improved dataset completeness, and schema simplification for downstream applications.
Data Integrity
Each file in the dataset has a SHA-256 checksum to verify its integrity:
| File Name | SHA-256 Checksum |
|---|---|
graph.cypher |
ed4800be1a822822402083e6209a0b3dd1a1a697e0a44b19e74638cd8a2c3abe |
graph.graphml |
55d7c4fc1a29b692c909bd76f89b35d9b3705f41febcdb6261ae72bca533e086 |
graph.json |
4cb68b0d7e5f2b5a6823ee489a58938f534bc9bcbce53d6f8c03f31f8c23795e |
Verification
To verify the integrity of each file, calculate its SHA-256 checksum and compare it with the hashes provided above.
You can use the following Python code to calculate the SHA-256 checksum:
import hashlib
def calculate_sha256(filepath):
sha256_hash = hashlib.sha256()
with open(filepath, "rb") as f:
for byte_block in iter(lambda: f.read(4096), b""):
sha256_hash.update(byte_block)
return sha256_hash.hexdigest()
Dataset Structure
Nodes and Properties
The knowledge graph consists of seven main node types, each representing a different entity within NASA's ecosystem.
1. Dataset
Description: Represents satellite datasets, particularly those managed by NASA DAACs, along with datasets from other governmental and academic data providers.
Properties:
globalId(String)doi(String)shortName(String)longName(String)abstract(String)cmrId(String)daac(String)temporalFrequency(String)temporalExtentStart(String)temporalExtentEnd(String)
2. Publication
Description: Captures publications that reference or use datasets.
Properties:
globalId(String)doi(String)title(String)abstract(String)authors(String)year(String)
3. ScienceKeyword
Properties:
globalId(String)name(String)
4. Instrument
Properties:
globalId(String)shortName(String)longName(String)
5. Platform
Properties:
globalId(String)shortName(String)longName(String)Type(String)
6. Project
Properties:
globalId(String)shortName(String)longName(String)
7. DataCenter
Properties:
globalId(String)shortName(String)longName(String)url(String)
Statistics
Data Statistics
Total Counts
| Type | Count |
|---|---|
| Total Nodes | 150,351 |
| Total Relationships | 436,203 |
Node Label Counts
| Node Label | Count |
|---|---|
| Dataset | 8,058 |
| DataCenter | 189 |
| Project | 415 |
| Platform | 455 |
| Instrument | 921 |
| ScienceKeyword | 1,609 |
| Publication | 138,704 |
Relationship Label Counts
| Relationship Label | Count |
|---|---|
| CITES | 208,616 |
| HAS_APPLIEDRESEARCHAREA | 121,553 |
| HAS_DATASET | 11,698 |
| HAS_INSTRUMENT | 2,631 |
| HAS_PLATFORM | 11,944 |
| HAS_SCIENCEKEYWORD | 25,553 |
| HAS_SUBCATEGORY | 1,823 |
| OF_PROJECT | 8,031 |
| USES_DATASET | 44,354 |
Data Formats
The Knowledge Graph Dataset is available in three formats: JSON, GraphML, and Cypher. (Section content unchanged from previous version.)
Data Formats
The Knowledge Graph Dataset is available in three formats:
1. JSON
- File:
graph.json - Description: A hierarchical data format representing nodes and relationships. Each node includes its properties, such as
globalId,doi, andpagerank_global. - Usage: Suitable for web applications and APIs, and for use cases where hierarchical data structures are preferred.
Loading the JSON Format
To load the JSON file into a graph database using Python and multiprocessing you can using the following script:
import json
from tqdm import tqdm
from collections import defaultdict
from multiprocessing import Pool, cpu_count
from neo4j import GraphDatabase
# Batch size for processing
BATCH_SIZE = 100
# Neo4j credentials (replace with environment variables or placeholders)
NEO4J_URI = "bolt://<your-neo4j-host>:<port>" # e.g., "bolt://localhost:7687"
NEO4J_USER = "<your-username>"
NEO4J_PASSWORD = "<your-password>"
def ingest_data(file_path):
# Initialize counters and label trackers
node_label_counts = defaultdict(int)
relationship_label_counts = defaultdict(int)
node_count = 0
relationship_count = 0
with open(file_path, "r") as f:
nodes = []
relationships = []
# Read and categorize nodes and relationships, and count labels
for line in tqdm(f, desc="Reading JSON Lines"):
obj = json.loads(line.strip())
if obj["type"] == "node":
nodes.append(obj)
node_count += 1
for label in obj["labels"]:
node_label_counts[label] += 1
elif obj["type"] == "relationship":
relationships.append(obj)
relationship_count += 1
relationship_label_counts[obj["label"]] += 1
# Print statistics
print("\n=== Data Statistics ===")
print(f"Total Nodes: {node_count}")
print(f"Total Relationships: {relationship_count}")
print("\nNode Label Counts:")
for label, count in node_label_counts.items():
print(f" {label}: {count}")
print("\nRelationship Label Counts:")
for label, count in relationship_label_counts.items():
print(f" {label}: {count}")
print("=======================")
# Multiprocess node ingestion
print("Starting Node Ingestion...")
node_batches = [nodes[i : i + BATCH_SIZE] for i in range(0, len(nodes), BATCH_SIZE)]
with Pool(processes=cpu_count()) as pool:
list(
tqdm(
pool.imap(ingest_nodes_batch, node_batches),
total=len(node_batches),
desc="Ingesting Nodes",
)
)
# Multiprocess relationship ingestion
print("Starting Relationship Ingestion...")
relationship_batches = [
relationships[i : i + BATCH_SIZE]
for i in range(0, len(relationships), BATCH_SIZE)
]
with Pool(processes=cpu_count()) as pool:
list(
tqdm(
pool.imap(ingest_relationships_batch, relationship_batches),
total=len(relationship_batches),
desc="Ingesting Relationships",
)
)
def ingest_nodes_batch(batch):
with GraphDatabase.driver(NEO4J_URI, auth=(NEO4J_USER, NEO4J_PASSWORD)) as driver:
with driver.session() as session:
for node in batch:
try:
label = node["labels"][0] # Assumes a single label per node
query = f"""
MERGE (n:{label} {{globalId: $globalId}})
SET n += $properties
"""
session.run(
query,
globalId=node["properties"]["globalId"],
properties=node["properties"],
)
except Exception as e:
print(
f"Error ingesting node with globalId {node['properties']['globalId']}: {e}"
)
def ingest_relationships_batch(batch):
with GraphDatabase.driver(NEO4J_URI, auth=(NEO4J_USER, NEO4J_PASSWORD)) as driver:
with driver.session() as session:
for relationship in batch:
try:
rel_type = relationship[
"label"
] # Use the label for the relationship
query = f"""
MATCH (start {{globalId: $start_globalId}})
MATCH (end {{globalId: $end_globalId}})
MERGE (start)-[r:{rel_type}]->(end)
"""
session.run(
query,
start_globalId=relationship["start"]["properties"]["globalId"],
end_globalId=relationship["end"]["properties"]["globalId"],
)
except Exception as e:
print(
f"Error ingesting relationship with label {relationship['label']}: {e}"
)
if __name__ == "__main__":
# Path to the JSON file
JSON_FILE_PATH = "<path-to-your-graph.json>"
# Run the ingestion process
ingest_data(JSON_FILE_PATH)
2. GraphML
- File:
graph.graphml - Description: An XML-based format well-suited for complex graph structures and metadata-rich representations.
- Usage: Compatible with graph visualization and analysis tools, including Gephi, Cytoscape, and databases that support GraphML import.
Loading the GraphML Format
To import the GraphML file into a graph database with APOC support, use the following command:
CALL apoc.import.graphml("path/to/graph.graphml", {readLabels: true})
3. Cypher
- File:
graph.cypher - Description: A series of Cypher commands to recreate the knowledge graph structure.
- Usage: Useful for recreating the graph in any Cypher-compatible graph database.
Loading the Cypher Format
To load the Cypher script, execute it directly using a command-line interface for your graph database:
neo4j-shell -file path/to/graph.cypher
4. Loading the Knowledge Graph into PyTorch Geometric (PyG)
This knowledge graph can be loaded into PyG (PyTorch Geometric) for further processing, analysis, or model training. Below is an example script that shows how to load the JSON data into a PyG-compatible HeteroData object.
The script first reads the JSON data, processes nodes and relationships, and then loads everything into a HeteroData object for use with PyG.
import json
import torch
from torch_geometric.data import HeteroData
from collections import defaultdict
# Load JSON data from file
file_path = "path/to/graph.json" # Replace with your actual file path
graph_data = []
with open(file_path, "r") as f:
for line in f:
try:
graph_data.append(json.loads(line))
except json.JSONDecodeError as e:
print(f"Error decoding JSON line: {e}")
continue
# Initialize HeteroData object
data = HeteroData()
# Mapping for node indices per node type
node_mappings = defaultdict(dict)
# Temporary storage for properties to reduce concatenation cost
node_properties = defaultdict(lambda: defaultdict(list))
edge_indices = defaultdict(lambda: defaultdict(list))
# Process each item in the loaded JSON data
for item in graph_data:
if item['type'] == 'node':
node_type = item['labels'][0] # Assuming first label is the node type
node_id = item['id']
properties = item['properties']
# Store the node index mapping
node_index = len(node_mappings[node_type])
node_mappings[node_type][node_id] = node_index
# Store properties temporarily by type
for key, value in properties.items():
if isinstance(value, list) and all(isinstance(v, (int, float)) for v in value):
node_properties[node_type][key].append(torch.tensor(value, dtype=torch.float))
elif isinstance(value, (int, float)):
node_properties[node_type][key].append(torch.tensor([value], dtype=torch.float))
else:
node_properties[node_type][key].append(value) # non-numeric properties as lists
elif item['type'] == 'relationship':
start_type = item['start']['labels'][0]
end_type = item['end']['labels'][0]
start_id = item['start']['id']
end_id = item['end']['id']
edge_type = item['label']
# Map start and end node indices
start_idx = node_mappings[start_type][start_id]
end_idx = node_mappings[end_type][end_id]
# Append to edge list
edge_indices[(start_type, edge_type, end_type)]['start'].append(start_idx)
edge_indices[(start_type, edge_type, end_type)]['end'].append(end_idx)
# Finalize node properties by batch processing
for node_type, properties in node_properties.items():
data[node_type].num_nodes = len(node_mappings[node_type])
for key, values in properties.items():
if isinstance(values[0], torch.Tensor):
data[node_type][key] = torch.stack(values)
else:
data[node_type][key] = values # Keep non-tensor properties as lists
# Finalize edge indices in bulk
for (start_type, edge_type, end_type), indices in edge_indices.items():
edge_index = torch.tensor([indices['start'], indices['end']], dtype=torch.long)
data[start_type, edge_type, end_type].edge_index = edge_index
# Display statistics for verification
print("Nodes and Properties:")
for node_type in data.node_types:
print(f"\nNode Type: {node_type}")
print(f"Number of Nodes: {data[node_type].num_nodes}")
for key, value in data[node_type].items():
if key != 'num_nodes':
if isinstance(value, torch.Tensor):
print(f" - {key}: {value.shape}")
else:
print(f" - {key}: {len(value)} items (non-numeric)")
print("\nEdges and Types:")
for edge_type in data.edge_types:
edge_index = data[edge_type].edge_index
print(f"Edge Type: {edge_type} - Number of Edges: {edge_index.size(1)} - Shape: {edge_index.shape}")
Citation
Please cite the dataset as follows:
NASA Goddard Earth Sciences Data and Information Services Center (GES-DISC). (2024). Knowledge Graph of NASA Earth Observations Satellite Datasets and Related Research Publications [Data set]. DOI: 10.57967/hf/3463
BibTeX
@misc {nasa_goddard_earth_sciences_data_and_information_services_center__(ges-disc)_2024,
author = { {NASA Goddard Earth Sciences Data and Information Services Center (GES-DISC)} },
title = { nasa-eo-knowledge-graph },
year = 2024,
url = { https://huggingface.co/datasets/nasa-gesdisc/nasa-eo-knowledge-graph },
doi = { 10.57967/hf/3463 },
publisher = { Hugging Face }
}
References
For details on the process of collecting these publications, please refer to:
Gerasimov, I., Savtchenko, A., Alfred, J., Acker, J., Wei, J., & KC, B. (2024). Bridging the Gap: Enhancing Prominence and Provenance of NASA Datasets in Research Publications. Data Science Journal, 23(1). DOI: 10.5334/dsj-2024-001
For any questions or further information, please contact:
- Armin Mehrabian: armin.mehrabian@nasa.gov
- Irina Gerasimov: irina.gerasimov@nasa.gov
- Kendall Gilbert: kendall.c.gilbert@nasa.gov
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