TIROS/NOAA SEM MEPED Reprocessed Data Archive.
This is the Reprocessed Version of the Medium Energy Proton Electron Detector, MEPED, Data Archive from the TIROS/NOAA Spacecraft. The raw Data from the NOAA Archive have been processed to 1 min Resolution. Magnetic Field Parameters including Geocentric Solar Magnetospheric, GSM, Bx, By, Bz, B/Bmin, and L Shell Values are derived by using four Magnetic Field Models: 1) International Geomagnetic Reference Field, IGRF, 2) Tsyganenko 1989, T89, 3) Tsyganenko 1996, T96, and 4) Tsyganenko 2001, T01. The T89, T96, and T01 Magnetic Field Models have been driven with Solar Wind Input Parameters and Geomagnetic Indices obtained from the OMNI-2 Data Set. Detector Counts, Omnidirectional and Perpendicular Electron and Proton Fluxes are archived.
Processing was done by: S.F. Fung, L.C. Tan, and X. Shao, Space Physics Data Facility, Goddard Space Flight Center, NASA, Greenbelt, MD 20771, USA, e-mail: Shing.F.Fung@nasa.gov.Version:2.3.0
TIROS/NOAA SEM MEPED Reprocessed Data Archive.
This is the Reprocessed Version of the Medium Energy Proton Electron Detector, MEPED, Data Archive from the TIROS/NOAA Spacecraft. The raw Data from the NOAA Archive have been processed to 1 min Resolution. Magnetic Field Parameters including Geocentric Solar Magnetospheric, GSM, Bx, By, Bz, B/Bmin, and L Shell Values are derived by using four Magnetic Field Models: 1) International Geomagnetic Reference Field, IGRF, 2) Tsyganenko 1989, T89, 3) Tsyganenko 1996, T96, and 4) Tsyganenko 2001, T01. The T89, T96, and T01 Magnetic Field Models have been driven with Solar Wind Input Parameters and Geomagnetic Indices obtained from the OMNI-2 Data Set. Detector Counts, Omnidirectional and Perpendicular Electron and Proton Fluxes are archived.
Processing was done by: S.F. Fung, L.C. Tan, and X. Shao, Space Physics Data Facility, Goddard Space Flight Center, NASA, Greenbelt, MD 20771, USA, e-mail: Shing.F.Fung@nasa.gov.| Role | Person | |
|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Donald.J.Williams |
| 2. | GeneralContact | spase://SMWG/Person/Shing.F.Fung |
| 3. | MetadataContact | spase://SMWG/Person/Robert.E.McGuire |
| 4. | MetadataContact | spase://SMWG/Person/Lee.Frost.Bargatze |
NOAA/POES MEPED Data Documentation: NOAA-5 to NOAA-14 Data Reprocessed at GSFC/SPDF, authored by Tan, L.C., Fung, S.F., and X. Shao, internal White Paper hosted by the CDAWeb at Goddard Space Flight Center, GSFC.
Polar Orbiting Environmental Satellites, POES, Web Page hosted by the National Center for Environmental Information, NCEI, at the National Oceanic and Atmospheric Administration, NOAA
Access to Data in CDF Format via ftp from SPDF
Access to Data in CDF Format via http from SPDF
Access to ASCII, CDF, and Plots via NASA/GSFC CDAWeb
Epoch Time Tags
Time in PB5 Format: Year, Day, Milliseconds, Observation Time
Day of Year, DOY, Fractional
Spacecraft Position, Altitude, Geographic, GEO, Spherical Coordinates
Spacecraft Position, Latitude, Geographic, GEO, Spherical Coordinates
Spacecraft Position, Longitude, Geographic, GEO, Spherical Coordinates
Spacecraft Position, Magnetic Local Time, Solar Magnetospheric, SM, Spherical Coordinates
Pitch Angle for MEPED Proton and Electron 0° Telescopes
Pitch Angle for MEPED Proton 81° Telescope
Pitch Angle for MEPED Electron 83° Telescope
MEPED Detector, Data Quality Flag: 0=Good, -1=Bad
MEPED Count Rates 0° Telescopes, five Proton and three Electron Energy Bands, counts_0dg
MEPED Count Rates, 81° and 83° Telescopes, five Proton and three Electron Energy Bands
MEPED Count Rates, Omnidirectional Telescope, three Proton Energy Bands
MEPED calculated Perpendicular Proton Flux, five Energy Bands
MEPED calculated Perpendicular Electron Flux, three Energy Bands
MEPED calculated Omnidirectional Proton Flux, five Energy Bands from the 0° Telescope, the 81° Telescope, and three Omnidirectional Telescopes
MEPED calculated Omnidirectional Electron Flux, three Energy Bands from the 0° Telescope and the 83° Telescopes
Magnetic Field Vector, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the International Geomagnetic Reference Field, IGRF, Model
Ratio of the Magnetic Field Magnitude divided by the Minimum Magnitude on the Field Line, B/Bmin, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the International Geomagnetic Reference Field, IGRF, Model
Spacecraft Position, McIlwain L Shell Value, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the International Geomagnetic Reference Field, IGRF, Model
Magnetic Field Vector, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1989, T89, Model
Ratio of the Magnetic Field Magnitude divided by the Minimum Magnitude on the Field Line, B/Bmin, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1989, T89, Model
Spacecraft Position, McIlwain L Shell Value, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1989, T89, Model
Magnetic Field Vector, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1996, T96, Model
Ratio of the Magnetic Field Magnitude divided by the Minimum Magnitude on the Field Line, B/Bmin, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1996, T96, Model
Spacecraft Position, McIlwain L Shell Value, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 1996, T96, Model
Magnetic Field Vector, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 2001, T01, Model
Ratio of the Magnetic Field Magnitude divided by the Minimum Magnitude on the Field Line, B/Bmin, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 2001, T01, Model
Spacecraft Position, McIlwain L Shell Value, Geocentric Solar Magnetospheric, GSM, Cartesian Coordinates, calculated by using the Tsyganenko 2001, T01, Model