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  • GHRSST Level 4 OSPO Global Foundation Sea Surface Temperature Analysis (GDS version 2)

    https://cmr.earthdata.nasa.gov/search/concepts/C1597990346-NOAA_NCEI.xml
    Description:

    A Group for High Resolution Sea Surface Temperature (GHRSST) Level 4 sea surface temperature analysis produced daily on an operational basis at the Office of Satellite and Product Operations (OSPO) using optimal interpolation (OI) on a global 0.054 degree grid. The Geo-Polar Blended Sea Surface Temperature (SST) Analysis combines multi-satellite retrievals of sea surface temperature into a single analysis of SST. This analysis uses both daytime and nighttime data from sensors that include the Advanced Very High Resolution Radiometer (AVHRR), the Visible Infrared Imager Radiometer Suite (VIIRS), the Geostationary Operational Environmental Satellite (GOES) imager, the Japanese Advanced Meteorological Imager (JAMI) and in situ data from ships, drifting and moored buoys. This analysis was specifically produced to be used as a lower boundary condition in Numerical Weather Prediction (NWP) models. This dataset adheres to the GHRSST Data Processing Specification (GDS) version 2 format specifications.

    Links: Temporal Extent: Spatial Extent:
    Minimum Bounding Rectangle: -90 -180 90 180

    NOAA_NCEI Short Name: gov.noaa.nodc.GHRSST-Geo_Polar_Blended-OSPO-L4-GLOB Version ID: netCDF-4 Unique ID: C1597990346-NOAA_NCEI

  • GHRSST Level 4 OSPO Global Nighttime Foundation Sea Surface Temperature Analysis (GDS version 2)

    https://cmr.earthdata.nasa.gov/search/concepts/C1597990351-NOAA_NCEI.xml
    Description:

    A Group for High Resolution Sea Surface Temperature (GHRSST) Level 4 sea surface temperature analysis produced daily on an operational basis at the Office of Satellite and Product Operations (OSPO) using optimal interpolation (OI) on a global 0.054 degree grid. The Geo-Polar Blended Sea Surface Temperature (SST) Analysis combines multi-satellite retrievals of sea surface temperature into a single analysis of SST. This analysis includes only nighttime data from sensors that include the Advanced Very High Resolution Radiometer (AVHRR), the Visible Infrared Imager Radiometer Suite (VIIRS), the Geostationary Operational Environmental Satellite (GOES) imager, the Japanese Advanced Meteorological Imager (JAMI) and in situ data from ships, drifting and moored buoys. This analysis was specifically produced to be used as a lower boundary condition in Numerical Weather Prediction (NWP) models. This dataset adheres to the GHRSST Data Processing Specification (GDS) version 2 format specifications.

    Links: Temporal Extent: Spatial Extent:
    Minimum Bounding Rectangle: -90 -180 90 180

    NOAA_NCEI Short Name: gov.noaa.nodc.GHRSST-Geo_Polar_Blended_Night-OSPO-L4-GLOB Version ID: 2 Unique ID: C1597990351-NOAA_NCEI

  • SatCORPS CERES GEO Edition 4 Meteosat-11 Northern Hemisphere Version 1.2

    https://cmr.earthdata.nasa.gov/search/concepts/C1584977040-LARC_ASDC.xml
    Description:

    CER_GEO_Ed4_MET11_NH_V01.2 is the Satellite ClOud and Radiation Property retrieval System (SatCORPS) Clouds and the Earth's Radiant Energy System (CERES) Geostationary Satellite (GEO) Edition 4 Meteosat-11 over the Northern Hemisphere (NH) Version 1.2 data product. Data was collected using the Spinning Enhanced Visible and Infrared Imager (SEVIRI) Instrument on the Meteosat-11 platform. Data collection for this product is in progress. Note : Version 1.2 is identical to version 1.0 . No changes have been made to the retrieval algorithm. This data set is comprised of cloud micro-physical and radiation properties derived hourly from GOES-11 geostationary satellite imager data using the Langley Research Center (LaRC) SATCORPS algorithms in support of the CERES project. The cloud micro-physical and radiation properties from each active geostationary satellite are merged together to create hourly global cloud properties that are used to estimate fluxes between CERES instrument measurements to account for the changing diurnal cycle. The data set is arranged as files for each hour and in netCDF-4 format. The observations are at 4-km resolution (at nadir) and are sub-sampled to 8 km. CERES is a key component of the Earth Observing System (EOS) program. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions are a follow-on to the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, protoflight model (PFM), was launched on November 27, 1997 as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the Earth Observing System (EOS) flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board Earth Observing System (EOS) Aqua on May 4, 2002. The CERES FM5 instrument was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The newest CERES instrument (FM6) was launched on board the Joint Polar-Orbiting Satellite System 1 (JPSS-1) satellite, now called NOAA-20, on November 18, 2017.

    Links: Temporal Extent: Spatial Extent:
    Minimum Bounding Rectangle: 0 -50 60 60

    LARC_ASDC Short Name: CER_GEO_Ed4_MET11_NH Version ID: V01.2 Unique ID: C1584977040-LARC_ASDC

  • SatCORPS CERES GEO Edition 4 Meteosat-11 Southern Hemisphere Version 1.2

    https://cmr.earthdata.nasa.gov/search/concepts/C1584977041-LARC_ASDC.xml
    Description:

    CER_GEO_Ed4_MET11_SH_V01.2 is the Satellite ClOud and Radiation Property retrieval System (SatCORPS) Clouds and the Earth's Radiant Energy System (CERES) Geostationary Satellite (GEO) Edition 4 Meteosat-11 over the Southern Hemisphere (SH) Version 1.2 data product. Data was collected using the Spinning Enhanced Visible and Infrared Imager (SEVIRI) Instrument on the Meteosat-11 platform. Data collection for this product is in progress. Note : Version 1.2 is identical to version 1.0 . No changes in retrieval algorithm. This data set is comprised of cloud micro-physical and radiation properties derived hourly from Meteosat-11 geostationary satellite imager data using the Langley Research Center (LARC) SATCORPS algorithms in support of the CERES project. The cloud micro-physical and radiation properties from each active geostationary satellite are merged together to create hourly global cloud properties that are used to estimate fluxes between CERES instrument measurements to account for the changing diurnal cycle. The data set is arranged as files for each hour and in netCDF-4 format. The observations are at 3-km resolution (at nadir) and are sub-sampled to 6 km. CERES is a key component of the Earth Observing System (EOS) program. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions are a follow-on to the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, protoflight model (PFM), was launched on November 27, 1997 as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the Earth Observing System (EOS) flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board Earth Observing System (EOS) Aqua on May 4, 2002. The CERES FM5 instrument was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The newest CERES instrument (FM6) was launched on board the Joint Polar-Orbiting Satellite System 1 (JPSS-1) satellite, now called NOAA-20, on November 18, 2017.

    Links: Temporal Extent: Spatial Extent:
    Minimum Bounding Rectangle: -60 -50 0 60

    LARC_ASDC Short Name: CER_GEO_Ed4_MET11_SH Version ID: V01.2 Unique ID: C1584977041-LARC_ASDC