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1) GOES 10 High Energy Proton and Alpha Detector (HEPAD) data at 5 m Resolution in Spacecraft Coordinates maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/HEPAD/PT5M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 23:59:59 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
The GOES 10 High Energy Proton and Alpha Detector (HEPAD) provides flux measurements of high energy proton and alpha particles. This data set consists of protons in 4 energy channels from 350 to >700 MeV and the alpha particles consist of 2 energy channels from 2560 to >3400 MeV.

2) GOES 10 high-resolution magnetometer data maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/MAG/PT0.512S
Start:2006-12-31 23:59:58 Observatory:GOES 10 Cadence:0.512 seconds
Stop:2008-12-31 23:59:58 Instrument:GOES 10, Triaxial Fluxgate Magnetometer Resource:NumericalData
GOES 10 magnetic field data at 0.512 second time resolution. The vector magnetic field is given in the spacecraft (s/c) earth-referenced coordinate system: Hp, He, Hn, and Ht, where Hp is perpendicular to the satellite orbital plane, or parallel to Earth's spin axis in the case of a zero degree inclination orbit; He is perpendicular to Hp and directed earthwards; Hn is perpendicular to both Hp and He and directed eastwards; and Ht is the total field. This data product also provides GOES 10 satellite positions and velocities derived from SSCWEB GEI ephemeris, interpolated to one minute time resolution. The magnetometer data are downlinked from the spacecraft in real-time to the NOAA Space Weather Prediction Center (SWPC) in Boulder, CO. The data from the raw Command and Data Acquisition (CDA) telemetry stream are processed by pre-processors at SWPC and from there 1-minute averages are distributed to SWPC Space Weather Operations, as well a archived at NOAA?s National Geophysical Data Center (NGDC) and NASA?s Coordinated Data Analysis Web (http://cdaweb.gsfc.nasa.gov/). The raw high-resolution data are corrected and processed at NOAA?s SWPC, and later archived at NGDC. The major issue for processing the high-resolution data is correction for the magnetic signature of spacecraft torquer currents as briefly discussed in the magnetometer instrument descriptions. In normal operation, the magnetometer samples its three axes every 0.512 seconds, synchronized with the telemetry frames. The magnetometer has an anti-aliasing low-pass filter on each axis. As part of the attitude control on the spacecraft, there are two magnetic torquers. At the magnetometers, these torquers can generate magnetic fields larger than the ambient fields to be measured. Therefore signals from these torquer currents need to be removed. The torquer currents are measured at the same rate as the magnetometer rate, and the currents are used to correct the magnetometer measurements. However, the torquer currents were not low-pass filtered. As a result, large instantaneous steps in the torquer currents show up in the magnetometer data as a delayed, slowly rising wave with some ringing, just what one would expect from the magnetometer low-pass filters. The so-called ?Farthing coefficients? simulate, from a short past history of the torquer measurements, the effects of the magnetometer filters. The torquer current changes are asynchronous with the telemetry frames and the timing between these events must be measured to a eighth of a telemetry frame interval for good performance. The transient responses in changes in torquer currents are reduced, but not eliminated for large changes in torquer currents. There exists one opportunity at the beginning of each mission to perform a spacecraft rotation maneuver to determine magnetometer offsets. These offsets are used through the duration of each satellite's lifetime. Approximate coefficients are: * 0.8 milliampere per torquer current count * 4 counts per torquer current command step (3.2 milliampere per command step) * 410 milliamperes full scale current * 32 magnetometer counts per nT (approximate) * 8 torquer step counts can be up to approximately 0.5 nT (depends on axis, which torquer, which satellite, etc.)

3) GOES 10 Magnetometer 1-Minute Data maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/MAG/PT1M
Start:1999-03-21 00:00:30 Observatory:GOES 10 Cadence:1 minute
Stop:2006-06-22 23:59:30 Instrument:GOES 10, 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.

4) GOES 10 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/A/PT5M
Start:1998-08-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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.

5) GOES 10 Space Evironment Monitor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/G/PT1M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:1 minute
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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.

6) GOES 10 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/G/PT5M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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.

7) GOES 10 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/H/PT5M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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.

8) GOES 10 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/I/PT5M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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.

9) GOES 10 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/10/SEM/Z/PT5M
Start:1998-07-01 00:00:00 Observatory:GOES 10 Cadence:5 minutes
Stop:2009-12-31 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 10 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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