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Geostationary Operational Environmental Satellite, R-Series (GOES-R) Space Environment In-Situ Suite (SEISS) Level 2 Products
The Space Environment In-Situ Suite (SEISS) is comprised of four sensors that monitor proton, electron, and heavy ion fluxes in the magnetosphere. These four sensors are the Energetic Heavy Ion Sensor (EHIS), the Magnetospheric Particle Sensors - High and Low (MPS-HI and MPS-LO), and the Solar and Galactic Proton Sensor (SGPS). There are two SGPS units on each satellite, one looking westward and one looking eastward. SEISS L2 data are used by NOAA’s Space Weather Prediction Center to drive the solar radiation storm alerts, based on NOAA’s space weather scales and the >2 MeV electron radiation belt alert, and to improve energetic particle forecasts. These SEISS Level 2 (L2) data include several different products: one and five-minute averages of fluxes from MPS-HI, MPS-LO and SGPS; one and five-minute integral fluxes from SGPS; density and temperature moments from MPS-HI and MPS-LO; solar particle event detection and rate of rise; and linear energy transfer from EHIS heavy ions. Data are in netCDF-4 format.
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GOES-R Series Level 1b SEISS Magnetospheric Particle Sensor High Energy (MPS-HI) Product in Daily Aggregations
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The GOES-R Magnetospheric Electrons and Protons: Medium and High Energy (MPSH) Product consists of fluxes of medium and high energy electrons and protons derived from in situ measurements of electron and proton count rates. The Magnetospheric Particle Sensor High (MPS-HI) makes these measurements. MPS-HI consists of ten solid state telescopes, five for electrons and five for protons, that define a 170-degree fan-like field-of-regard in the north-south plane. Differential and integral electron fluxes are reported at eleven energy bands from each electron telescope. Ten of the energy bands are evenly spaced logarithmically spanning from 50 keV to 4 MeV with differential electron flux being reported. The eleventh energy band collects electrons with energies greater than 2 MeV with electron integral flux being reported. In addition, differential proton fluxes are reported at eleven energy bands from each proton telescope. The eleven proton energy bands are evenly spaced logarithmically and range from 80 keV to 12 MeV. In addition, the product contains ionizing radiation doses in two energy deposition ranges, 50 keV to 1 MeV (low linear energy transfer, LOLET) and 1 MeV to 50 MeV (high linear energy transfer, HILET). The product also contains processing and data quality metadata, satellite state and location information, and data required for the generation of level 2 products. Measurement resolution is one second. NOAA's National Centers for Environmental Information (NCEI) has created these daily files by aggregating the official L1b files produced by the GOES-R Ground System. The granular L1b files each span 30 seconds of observations.
NOAA GOES-R Series Magnetometer (MAG) Instrument Calibration Data
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The Magnetometer Instrument Engineering Telemetry Data file contains data used to support the generation of the Magnetometer Level 1b product, and monitor and evaluate the health and performance of the two magnetometers. This data is transmitted to the ground in raw digital counts, and subsequently converted into physical units by the ground system. Some of the data pertains to the temperature of components of the magnetometers. This includes temperatures for the electronics and sensors. Other telemetry includes reference voltages and temperature dependent scale factors and offsets relating raw observed counts to magnetic field units (nanoteslas) for the two magnetometers. The Magnetometer Calibration Data file contains raw observation counts and data acquisition status from the inboard and outbound magnetometers for a one second interval during a calibration maneuver. Nominally, this file contains ten observation samples acquired at one-tenth of a second intervals.
SatCORPS CERES GEO Edition 4 MTSAT-2R Southern Hemisphere Version 1.0
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CER_GEO_Ed4_MTS02_SH_V01 is the Satellite Cloud and Radiation Property retrieval System (SatCORPS) Clouds and the Earth's Radiant Energy System (CERES) Geostationary Satellite (GEO) Edition 4 Multi-functional Transport Satellite 2 Replacement (MTSAT-2R) over the Southern Hemisphere (SH) Version 1.0 data product. Data was collected using the Visible and Infrared Spin Scan Radiometer (VISSR) Instrument on The Multi-functional Transport Satellite 2 (MTSAT-2) platform. This data set comprises cloud micro-physical and radiation properties derived hourly from MTSAT-2 geostationary satellite imager data using the Langley Research Center (LARC) SATCORPS algorithms supporting the CERES project. Each active geostationary satellite's cloud microphysical and radiation properties are merged to create hourly global cloud properties that 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 Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, the proto flight 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 onboard the Earth Observing System (EOS) flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched onboard Earth Observing System (EOS) Aqua on May 4, 2002. The CERES FM5 instrument was launched onboard the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The newest CERES instrument (FM6) was launched onboard the Joint Polar-Orbiting Satellite System 1 (JPSS-1) satellite, now called NOAA-20, on November 18, 2017.
SatCORPS CERES GEO Edition 4 GOES-15 Southern Hemisphere Version 1.0
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CER_GEO_Ed4_GOE15_SH_V01 is the Satellite Cloud and Radiation Property retrieval System (SatCORPS) Clouds and the Earth's Radiant Energy System (CERES) Geostationary Satellite (GEO) Edition 4 Geostationary Operational Environmental Satellite 15 (GOES-15) over the Southern Hemisphere (SH) Version 1.0 data product. Data was collected using the GOES-15 Imager on the GOES-15 Platform. Data collection for this product is complete. This data set comprises cloud micro-physical and radiation properties derived hourly from GOES-15 geostationary satellite imager data using the Langley Research Center (LARC) SATCORPS algorithms supporting the CERES project. The cloud micro-physical and radiation properties from each active geostationary satellite are merged to create hourly global cloud properties that 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 Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, the proto flight 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.
SatCORPS CERES GEO Edition 4 GOES-14 Southern Hemisphere Version 1.0
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CER_GEO_Ed4_GOE14_SH_V01 is the Satellite Cloud and Radiation Property retrieval System (SatCORPS) Clouds and the Earth's Radiant Energy System (CERES) Geostationary Satellite (GEO) Edition 4 Geostationary Operational Environmental Satellite 14 (GOES-14) over the Southern Hemisphere (SH) Version 1.0 data product. Data was collected using the GOES-I-M Imager on the GOES-14 Platform. Data collection for this product is complete. This data set comprises cloud micro-physical and radiation properties derived hourly from GOES-14 geostationary satellite imager data using the Langley Research Center (LARC) SATCORPS algorithms supporting the CERES project. Each active geostationary satellite's cloud micro-physical and radiation properties are merged to create hourly global cloud properties that 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 Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, the 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.
Space Weather Follow On (SWFO) Level 2 Retrospective data from the Compact Coronagraph-1 (CCOR1) on Geostationary Operational Environmental Satellite 19 (GOES-19)
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This data collection consists of archived Space Weather Follow On (SWFO) Level 2 Retrospective data from the Compact Coronagraph-1 (CCOR1) on Geostationary Operational Environmental Satellite 19 (GOES-19). The archival process includes daily files. The CCOR-1 instrument generates 96 files per day per level in one tar file that contains FITS. These data are produced by the CCOR-1 instrument aboard the GOES-19 spacecraft. The instrument observes broadband optical light that is scattered from coronal electrons and heliospheric dust. GOES-19 launched in late April 2024. Other products available are auxiliary files (pkt-l0_g19, orb-pr_g19, and sc-att_g19); CCOR1 files (ccor1-l0a_g19, ccor1-l0b_g19, ccor1-l1a_g19, ccor1-l1b_g19, ccor1-l2_g19, and ccor1-l3_g19); and, National Centers for Environmental Data (NCEI) Retrospective Science products (sci_ccor1-l1a_g19, sci_ccor1-l1b_g19, sci_ccor1-l3_g19, sci_ccor1-dm_g19, and sci_ccor1-mm_g19).
Space Weather Follow On (SWFO) Level 3 Retrospective data from the Compact Coronagraph-1 (CCOR1) on Geostationary Operational Environmental Satellite 19 (GOES-19)
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This data collection consists of archived Space Weather Follow On (SWFO) Level 3 Retrospective data from the Compact Coronagraph-1 (CCOR1) on Geostationary Operational Environmental Satellite 19 (GOES-19). The archival process includes daily files. The CCOR-1 instrument generates 96 files per day per level in one tar file that contains FITS. These data are produced by the CCOR-1 instrument aboard the GOES-19 spacecraft. The instrument observes broadband optical light that is scattered from coronal electrons and heliospheric dust. GOES-19 launched in late April 2024. Other products available are auxiliary files (pkt-l0_g19, orb-pr_g19, and sc-att_g19); CCOR1 files (ccor1-l0a_g19, ccor1-l0b_g19, ccor1-l1a_g19, ccor1-l1b_g19, ccor1-l2_g19, and ccor1-l3_g19); and, National Centers for Environmental Data (NCEI) Retrospective Science products (sci_ccor1-l1a_g19, sci_ccor1-l1b_g19, sci_ccor1-l2_g19, sci_ccor1-dm_g19, and sci_ccor1-mm_g19).