The GOES 15 Magnetospheric Electron Detector (MAGED) are essentially the same as the Energetic Particle Sensor (EPS) on GOES 8-12. For more information, please see Onsager et al. 1996, Operational uses of the GOES energetic particle detectors, in GOES 8 and Beyond, Proc. SPIE, Vol. 2812, edited by E. R. Washwell, pp. 281-290, Bellingham, WA. These data file contain mainly information on the electron count rates and fluxes from 30 to 50 keV. Data files contain long descriptive header.
Version:2.3.1
The GOES 15 Magnetospheric Electron Detector (MAGED) are essentially the same as the Energetic Particle Sensor (EPS) on GOES 8-12. For more information, please see Onsager et al. 1996, Operational uses of the GOES energetic particle detectors, in GOES 8 and Beyond, Proc. SPIE, Vol. 2812, edited by E. R. Washwell, pp. 281-290, Bellingham, WA. These data file contain mainly information on the electron count rates and fluxes from 30 to 50 keV. Data files contain long descriptive header.
| Role | Person | |
|---|---|---|
| 1. | PrincipalInvestigator | spase://SMWG/Person/Terry.Onsager |
| 2. | MetadataContact | spase://SMWG/Person/James.M.Weygand |
Information about the magnetometers onboard GOES 15
Direct link to the GOES 15 Magnetospheric Electron Detector (MAGED) data in CSV format as well as the energetic particle data from other GOES spacecraft. The data are sorted by year, month, spacecraft, and file type. The file names indicates the data type, spacecraft number, year, month, and resolution. For example, g15_maged_19me1_2s_20110617_20110617.csv, indicates GOES 15 magnetometer data at 2 s time resolution for 2011-06-17.
Time format in data files is year-month-day hour:minute:seconds.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 1 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 1 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 1 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 2 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 2 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 1 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 3 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 3 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 3 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 4 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 4 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 4 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 5 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 5 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 5 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 6 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 6 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 6 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 7 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 7 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 7 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 8 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 8 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 8 corrected for dead time errors but not other sources of contamination.
Quality flag non-zero value indicates data quality issue.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 9 not corrected for dead time errors or other sources of contamination.
Average count rate of electrons with energy from 30 to 50 keV measured by telescope 9 corrected for dead time errors but not other sources of contamination
Average flux of 40 keV electrons measured by telescope 9 corrected for dead time errors but not other sources of contamination.