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1)	GOES 8 Magnetometer 1-Minute Data
Resource ID:spase://VMO/NumericalData/GOES/8/MAG/PT1M
Start: 1995-12-01 00:00:30 Observatory: GOES 8 Cadence: 1 minute Stop: 2003-04-08 23:59:30 Instrument: GOES 8, Triaxial Fluxgate Magnetometer Resource: NumericalData
The NOAA Geostationary Operational Environment Satellite (GOES) key parameters. This data is a subset of the data available from the GOES Space Environment Monitor (SEM) instruments. It contains vector magnetic field in three coordinate systems: * (1) Spacecraft P,E,N * (2) GSM x,y,z and * (3) GSE x,y,z. Spacecraft magnetic field is defined as: * P - perpendicular to the spacecraft orbital plane or parallel to the Earth's spin axis in the case of a zero degree inclination orbit; * E - perpendicular to P and directed earhtwards; and * N - perpendicular to both P and E and directed eastwards.

2)	GOES 8 Space Evironment Monitor Data at 5 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/A/PT5M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 5 minutes Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 5 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the uncorrected alpha-particle fluxes for several energy ranges.

3)	GOES 8 Space Evironment Monitor Data at 1 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/G/PT1M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 1 minute Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 1 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the uncorrected proton fluxes for several energy ranges.

4)	GOES 8 Space Evironment Monitor Data at 5 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/G/PT5M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 5 minutes Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 5 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the uncorrected proton fluxes for several energy ranges.

5)	GOES 8 Space Evironment Monitor Data at 5 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/H/PT5M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 5 minutes Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 5 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the uncorrected proton and alpha particle fluxes for several energy ranges.

6)	GOES 8 Space Evironment Monitor Data at 5 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/I/PT5M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 5 minutes Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 5 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the corrected proton fluxes for several energy ranges.

7)	GOES 8 Space Evironment Monitor Data at 5 min Resolution
Resource ID:spase://VMO/NumericalData/GOES/8/SEM/Z/PT5M
Start: 1995-03-01 00:00:00 Observatory: GOES 8 Cadence: 5 minutes Stop: 2003-06-30 00:00:00 Instrument: Space Environment Monitor (SEM) Resource: NumericalData
This GOES 8 SEM data set contains various parameters at 5 min resolution. Within the data files is the Xray flux for two wavelength ranges, the magnetic field vectors, the >2 MeV uncorrected elecron fluxes, and the corrected proton fluxes for several energy ranges.

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