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1) Cluster Rumba Digital Wave Processor (DWP) prime parameter data at about 4 sec resolution (spin averaged) in GSE Coordinates maxmize
Resource ID:spase://VMO/NumericalData/Cluster-Rumba/DWP/PrimeParameter/PT4S
Start:2000-11-01 00:00:00 Observatory:Cluster FM5 (Rumba) Cadence:4 seconds
Stop:2009-12-30 23:59:59 Instrument:Digital Wave Processor (DWP) Resource:NumericalData
Cluster Rumba Digital Wave Processor (DWP) data set contains various instrument status and data status flags as well as particle correlator information.

2) Cluster Salsa Digital Wave Processor (DWP) prime parameter data at about 4 sec resolution (spin averaged) in GSE Coordinates maxmize
Resource ID:spase://VMO/NumericalData/Cluster-Salsa/DWP/PrimeParameter/PT4S
Start:2000-11-01 00:00:00 Observatory:Cluster FM6 (Salsa) Cadence:4 seconds
Stop:2009-12-30 23:59:59 Instrument:Digital Wave Processor (DWP) Resource:NumericalData
Cluster Salsa Digital Wave Processor (DWP) data set contains various instrument status and data status flags as well as particle correlator information.

3) Cluster Samba Digital Wave Processor (DWP) prime parameter data at about 4 sec resolution (spin averaged) in GSE Coordinates maxmize
Resource ID:spase://VMO/NumericalData/Cluster-Samba/DWP/PrimeParameter/PT4S
Start:2000-11-01 00:00:00 Observatory:Cluster FM7 (Samba) Cadence:4 seconds
Stop:2009-12-30 23:59:59 Instrument:Digital Wave Processor (DWP) Resource:NumericalData
Cluster Samba Digital Wave Processor (DWP) data set contains various instrument status and data status flags as well as particle correlator information.

4) Cluster Tango Digital Wave Processor (DWP) prime parameter data at about 4 sec resolution (spin averaged) in GSE Coordinates maxmize
Resource ID:spase://VMO/NumericalData/Cluster-Tango/DWP/PrimeParameter/PT4S
Start:2000-11-01 00:00:00 Observatory:Cluster FM8 (Tango) Cadence:4 seconds
Stop:2009-12-30 23:59:59 Instrument:Digital Wave Processor (DWP) Resource:NumericalData
Cluster Tango Digital Wave Processor (DWP) data set contains various instrument status and data status flags as well as particle correlator information.

5) Cluster Digital Wave Processor (DWP) summary parameter data at about 60 sec resolution (spin averaged) in GSE Coordinates maxmize
Resource ID:spase://VMO/NumericalData/Cluster/DWP/SummaryParameter/PT60S
Start:2000-11-01 00:00:00 Observatory:Cluster FM5 (Rumba) Cadence:60 seconds
Stop:2009-12-30 23:59:59 Instrument:Digital Wave Processor (DWP) Resource:NumericalData
Cluster Digital Wave Processor (DWP) data set contains various instrument status and data status flags as well as particle correlator information.

6) 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.

7) 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.

8) 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.

9) 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.

10) 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.

11) 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.

12) 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.

13) GOES 11 Energetic Particle Sensor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/EPS/PT1M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:1 minute
Stop:2011-02-28 23:59:59 Instrument:Environment Monitor Resource:NumericalData
The energetic particle sensor data consists of electron and proton data. The electrons consists of 3 energy flux channels with energies greater than 0.6 MeV. The proton fluxes consist of 7 energy channels from 0.6 to 500 MeV.

14) GOES 11 Energetic Particle Sensor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/EPS/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2011-02-28 23:59:59 Instrument:Environment Monitor Resource:NumericalData
The energetic particle sensor data consists of electron, proton, and alpha particle data. The electrons consists of 3 energy flux channels with energies greater than 0.6 MeV. The protons consist of 7 energy channels from 0.6 to 500 MeV and the alpha particles consist of 6 energy channels from 4 to 500 MeV.

15) GOES 11 High Energy Proton and Alpha Detector (HEPAD) data at 5 m Resolution in Spacecraft Coordinates maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/HEPAD/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2011-02-28 23:59:59 Instrument:Environment Monitor Resource:NumericalData
The GOES 11 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.

16) GOES 11 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/A/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

17) GOES 11 Space Evironment Monitor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/G/PT1M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:1 minute
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

18) GOES 11 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/G/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

19) GOES 11 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/H/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

20) GOES 11 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/I/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

21) GOES 11 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/11/SEM/Z/PT5M
Start:2000-07-01 00:00:00 Observatory:GOES 11 Cadence:5 minutes
Stop:2010-12-31 00:00:00 Instrument:Environment Monitor Resource:NumericalData
This GOES 11 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.

22) GOES 12 Energetic Particle Sensor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/EPS/PT1M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:1 minute
Stop:2010-08-31 23:59:59 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
The energetic particle sensor data consists of electron and proton data. The electrons consists of 3 energy flux channels with energies greater than 0.6 MeV. The proton fluxes consist of 7 energy channels from 0.6 to 500 MeV.

23) GOES 12 Energetic Particle Sensor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/EPS/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-08-31 23:59:59 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
The energetic particle sensor data consists of electron, proton, and alpha particle data. The electrons consists of 3 energy flux channels with energies greater than 0.6 MeV. The protons consist of 7 energy channels from 0.6 to 500 MeV and the alpha particles consist of 6 energy channels from 4 to 500 MeV.

24) GOES 12 High Energy Proton and Alpha Detector (HEPAD) data at 5 m Resolution in Spacecraft Coordinates maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/HEPAD/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-08-31 23:59:59 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
The GOES 12 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.

25) GOES 12 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/A/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

26) GOES 12 Space Evironment Monitor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/G/PT1M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:1 minute
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

27) GOES 12 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/G/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

28) GOES 12 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/H/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

29) GOES 12 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/I/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

30) GOES 12 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/12/SEM/Z/PT5M
Start:2003-01-01 00:00:00 Observatory:GOES 12 Cadence:5 minutes
Stop:2010-09-30 00:00:00 Instrument:Space Environment Monitor (SEM) Resource:NumericalData
This GOES 12 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.

31) GOES 9 Energetic Particle Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/EPS/PT1M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-07-31 23:59:59 Instrument:Space Environment Monitor Resource:NumericalData
The energetic particle sensor (now called EP8 instead of EPS or EPM) data consists of electron, proton, and alpha particle data. The electrons consists of 3 energy flux channels with energies greater than 0.6 MeV. The protons consist of 7 energy channels from 0.6 to 500 MeV and the alpha particles consist of 6 energy channels from 4 to 500 MeV.

32) GOES 9 High Energy Proton and Alpha Detector (HEPAD) data at 5 m Resolution in Spacecraft Coordinates maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/HEPAD/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-07-31 23:59:00 Instrument:Space Environment Monitor Resource:NumericalData
The GOES 9 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.

33) GOES 9 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/A/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

34) GOES 9 Space Evironment Monitor Data at 1 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/G/PT1M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:1 minute
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

35) GOES 9 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/G/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

36) GOES 9 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/H/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

37) GOES 9 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/I/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

38) GOES 9 Space Evironment Monitor Data at 5 min Resolution maxmize
Resource ID:spase://VMO/NumericalData/GOES/9/SEM/Z/PT5M
Start:1996-04-01 00:00:00 Observatory:GOES 9 Cadence:5 minutes
Stop:1998-08-31 00:00:00 Instrument:Space Environment Monitor Resource:NumericalData
This GOES 9 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.

39) STEREO WAVES (SWAVES) PDF Dynamic Spectrogram Plots both Ahead and Behind s/c maxmize
Resource ID:spase://VWO/DisplayData/STEREO/SWAVES/DS.Color.PDF.P1D
Start:2006-10-27 20:24:42 Observatory:STEREO A Cadence:1 minute
Stop:2014-11-26 01:03:32 Instrument:STEREO-A Waves (SWAVES) Resource:DisplayData
This dataset contains 24 hour duration dynamic spectrogram plots from the combined STEREO A and B Waves instrument. The plots are provided in several file formats (PNG, Postscript and PDF) and there are renditions in color and grayscale with and without additional lines of time series data indicating the instrument operating status. These plots all reside within the same directory structure subdivided by year. The "new" subdirectory contain plots at a higher resolution but currently are not available for dates early in the mission. These data consist of output from the SWAVES HFR and LFR receivers. ? the High Frequency Receivers (HFR) - for spectral analysis and direction finding of radio noise generated from a few solar radii (16 MHz) to about half an Astronomical Unit (125 kHz) ? the Low Frequency Receiver (LFR) - for spectral analysis and direction finding from about half an Astronomical Unit (160 kHz) to one AU (2.5 kHz).

40) STEREO WAVES (SWAVES) Radio Intensity Spectra, both Ahead and Behind s/c maxmize
Resource ID:spase://VWO/NumericalData/STEREO/SWAVES/DS.Combined.PT1M
Start:2006-10-27 20:24:42 Observatory:STEREO A Cadence:1 minute
Stop:2014-11-26 01:03:34 Instrument:STEREO-A Waves (SWAVES) Resource:NumericalData
The CDF file contains 1 minute averaged radio intensity data from both the Ahead and Behind s/c. A description of the STEREO/WAVES instrument is provided in: Bougeret, J.L, et al. (2008), S/WAVES: The Radio and Plasma Wave Investigation on the STEREO Mission, Space Science Reviews, 136, 487-528. The STEREO / WAVES (SWAVES) instruments provide unique and critical observations for all primary science objectives of the STEREO mission, the generation of CMEs, their evolution, and their interaction with Earth's magnetosphere. SWAVES can probe a CME from lift-off to Earth by detecting the coronal and interplanetary (IP) shock of the most powerful CMEs, providing a radial profile through spectral imaging, determining the radial velocity from ~2 RS (from center of sun) to Earth, measuring the density of the volume of the heliosphere between the sun and Earth, and measuring important in situ properties of the IP shock, magnetic cloud, and density compression in the fast solar wind stream that follows. SWAVES measures the fluctuation electric field present on three orthogonal monopole antennas mounted on the back (anti-sunward) surface of the spacecraft. Each monopole antenna unit is a 6 m long Beryllium-Copper (BeCu) ?stacer? spring. The three units deploy from a common baseplate that also accommodates the preamplifier housing. The 6 m length was chosen to put the antenna quarter-wave resonance near the top of the SWAVES HFR2 frequency band. These data consist of output from the SWAVES HFR and LFR receivers. ? the High Frequency Receivers (HFR) - for spectral analysis and direction finding of radio noise generated from a few solar radii (16 MHz) to about half an Astronomical Unit (125 kHz) ? the Low Frequency Receiver (LFR) - for spectral analysis and direction finding from about half an Astronomical Unit (160 kHz) to one AU (2.5 kHz).

41) THEMIS-A: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature. maxmize
Resource ID:spase://VMO/NumericalData/THEMIS/A/MOM/PT3S
Start:2007-08-02 00:00:30 Observatory:THEMIS-A Cadence:3 seconds
Stop:2014-11-26 01:02:46 Instrument:THEMIS-A: On Board moments: ESA and SST Electron/Ion moments density, flux, velocity, pressure and temperature. Resource:NumericalData
THEMIS-A On Board moments. On board data outputs include number density, particle flux, energy flux, and a six component symetric momentum flux tensor. Other moments are calculated from these partial moments on the ground adding total pressure, velocity, plasma temperature (measured as a three dimensional energy vector), and a six component symetric pressure tensor to the list of data products. Number density and total pressure are scalar outputs. Velocity is calculated in DSL, GSE, GSM, and MFA coordinates (coordinate descriptions are listed below in Table 1). Magnetic Field Aligned pressure tensor and temperature are calculated as well. All quantities are calculated for both ions and electrons from a combination of ESA and SST data. Moments data are taken at spin resolution in all ESA survey modes except burst. The spacecraft potential, as measure by the EFI, is used to correct for spacecraft charging by shifting the particle energies for calculation; this eliminates contamination from photo-electrons. Also, weighting factors are used to account for instrument specific energy and angle efficiency variations. Table 1: Coordinate Descriptions. Despun Sun - L-vector (DSL): Z-axis points towards the spin axis, the Y-axis is obtained from the cross product of Z and the Spacecraft-Sun direction as viewed from the probe. The X-axis sits in the Z-axis-Sun plane and completes a right handed system. Geocentric Solar Ecliptic (GSE): Z-axis is normal to the solar ecliptic, the X-axis points from earth towards the Sun, and Y complets a right handed system. Geocentric solar Magnetosphereic (GSM): X-axis points from Earth to the Sun, the Y-axis is orthogonal to the Earth's magnetic dipole and points towards the dusk side, and the X-Z plane contains the dipole axis. Magnetic Field Aligned (MFA): Z-axis points along magnetic field lines, the Y-axis is the orthonormal cross product of the Z-axis and a vector pointing towards the Sun, and the X-axis completes the right handed system.

42) THEMIS-B: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature. maxmize
Resource ID:spase://VMO/NumericalData/THEMIS/B/MOM/PT3S
Start:2007-08-10 00:02:05 Observatory:THEMIS-B Cadence:3 seconds
Stop:2014-11-26 01:02:43 Instrument:THEMIS-B: On Board moments: ESA and SST Electron/Ion moments density, flux, velocity, pressure and temperature. Resource:NumericalData
THEMIS-B On Board moments. On board data outputs include number density, particle flux, energy flux, and a six component symetric momentum flux tensor. Other moments are calculated from these partial moments on the ground adding total pressure, velocity, plasma temperature (measured as a three dimensional energy vector), and a six component symetric pressure tensor to the list of data products. Number density and total pressure are scalar outputs. Velocity is calculated in DSL, GSE, GSM, and MFA coordinates (coordinate descriptions are listed below in Table 1). Magnetic Field Aligned pressure tensor and temperature are calculated as well. All quantities are calculated for both ions and electrons from a combination of ESA and SST data. Moments data are taken at spin resolution in all ESA survey modes except burst. The spacecraft potential, as measure by the EFI, is used to correct for spacecraft charging by shifting the particle energies for calculation; this eliminates contamination from photo-electrons. Also, weighting factors are used to account for instrument specific energy and angle efficiency variations. Table 1: Coordinate Descriptions. Despun Sun - L-vector (DSL): Z-axis points towards the spin axis, the Y-axis is obtained from the cross product of Z and the Spacecraft-Sun direction as viewed from the probe. The X-axis sits in the Z-axis-Sun plane and completes a right handed system. Geocentric Solar Ecliptic (GSE): Z-axis is normal to the solar ecliptic, the X-axis points from earth towards the Sun, and Y complets a right handed system. Geocentric solar Magnetosphereic (GSM): X-axis points from Earth to the Sun, the Y-axis is orthogonal to the Earth's magnetic dipole and points towards the dusk side, and the X-Z plane contains the dipole axis. Magnetic Field Aligned (MFA): Z-axis points along magnetic field lines, the Y-axis is the orthonormal cross product of the Z-axis and a vector pointing towards the Sun, and the X-axis completes the right handed system.

43) THEMIS-C: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature. maxmize
Resource ID:spase://VMO/NumericalData/THEMIS/C/MOM/PT3S
Start:2007-08-10 00:00:32 Observatory:THEMIS-C Cadence:3 seconds
Stop:2014-11-26 01:02:40 Instrument:THEMIS-C: On Board moments: ESA and SST Electron/Ion moments density, flux, velocity, pressure and temperature. Resource:NumericalData
THEMIS-C On Board moments. On board data outputs include number density, particle flux, energy flux, and a six component symetric momentum flux tensor. Other moments are calculated from these partial moments on the ground adding total pressure, velocity, plasma temperature (measured as a three dimensional energy vector), and a six component symetric pressure tensor to the list of data products. Number density and total pressure are scalar outputs. Velocity is calculated in DSL, GSE, GSM, and MFA coordinates (coordinate descriptions are listed below in Table 1). Magnetic Field Aligned pressure tensor and temperature are calculated as well. All quantities are calculated for both ions and electrons from a combination of ESA and SST data. Moments data are taken at spin resolution in all ESA survey modes except burst. The spacecraft potential, as measure by the EFI, is used to correct for spacecraft charging by shifting the particle energies for calculation; this eliminates contamination from photo-electrons. Also, weighting factors are used to account for instrument specific energy and angle efficiency variations. Table 1: Coordinate Descriptions. Despun Sun - L-vector (DSL): Z-axis points towards the spin axis, the Y-axis is obtained from the cross product of Z and the Spacecraft-Sun direction as viewed from the probe. The X-axis sits in the Z-axis-Sun plane and completes a right handed system. Geocentric Solar Ecliptic (GSE): Z-axis is normal to the solar ecliptic, the X-axis points from earth towards the Sun, and Y complets a right handed system. Geocentric solar Magnetosphereic (GSM): X-axis points from Earth to the Sun, the Y-axis is orthogonal to the Earth's magnetic dipole and points towards the dusk side, and the X-Z plane contains the dipole axis. Magnetic Field Aligned (MFA): Z-axis points along magnetic field lines, the Y-axis is the orthonormal cross product of the Z-axis and a vector pointing towards the Sun, and the X-axis completes the right handed system.

44) THEMIS-D: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature. maxmize
Resource ID:spase://VMO/NumericalData/THEMIS/D/MOM/PT3S
Start:2007-08-09 23:59:56 Observatory:THEMIS-D Cadence:3 seconds
Stop:2014-11-26 01:02:33 Instrument:THEMIS-D: On Board moments: ESA and SST Electron/Ion moments density, flux, velocity, pressure and temperature. Resource:NumericalData
THEMIS-D On Board moments. On board data outputs include number density, particle flux, energy flux, and a six component symetric momentum flux tensor. Other moments are calculated from these partial moments on the ground adding total pressure, velocity, plasma temperature (measured as a three dimensional energy vector), and a six component symetric pressure tensor to the list of data products. Number density and total pressure are scalar outputs. Velocity is calculated in DSL, GSE, GSM, and MFA coordinates (coordinate descriptions are listed below in Table 1). Magnetic Field Aligned pressure tensor and temperature are calculated as well. All quantities are calculated for both ions and electrons from a combination of ESA and SST data. Moments data are taken at spin resolution in all ESA survey modes except burst. The spacecraft potential, as measure by the EFI, is used to correct for spacecraft charging by shifting the particle energies for calculation; this eliminates contamination from photo-electrons. Also, weighting factors are used to account for instrument specific energy and angle efficiency variations. Table 1: Coordinate Descriptions. Despun Sun - L-vector (DSL): Z-axis points towards the spin axis, the Y-axis is obtained from the cross product of Z and the Spacecraft-Sun direction as viewed from the probe. The X-axis sits in the Z-axis-Sun plane and completes a right handed system. Geocentric Solar Ecliptic (GSE): Z-axis is normal to the solar ecliptic, the X-axis points from earth towards the Sun, and Y complets a right handed system. Geocentric solar Magnetosphereic (GSM): X-axis points from Earth to the Sun, the Y-axis is orthogonal to the Earth's magnetic dipole and points towards the dusk side, and the X-Z plane contains the dipole axis. Magnetic Field Aligned (MFA): Z-axis points along magnetic field lines, the Y-axis is the orthonormal cross product of the Z-axis and a vector pointing towards the Sun, and the X-axis completes the right handed system.

45) THEMIS-E: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature. maxmize
Resource ID:spase://VMO/NumericalData/THEMIS/E/MOM/PT3S
Start:2007-08-10 00:00:16 Observatory:THEMIS-E Cadence:3 seconds
Stop:2014-11-26 01:02:30 Instrument:THEMIS-E: On Board moments: ESA and SST Electron/Ion moments density, flux, velocity, pressure and temperature. Resource:NumericalData
THEMIS-E On Board moments. On board data outputs include number density, particle flux, energy flux, and a six component symetric momentum flux tensor. Other moments are calculated from these partial moments on the ground adding total pressure, velocity, plasma temperature (measured as a three dimensional energy vector), and a six component symetric pressure tensor to the list of data products. Number density and total pressure are scalar outputs. Velocity is calculated in DSL, GSE, GSM, and MFA coordinates (coordinate descriptions are listed below in Table 1). Magnetic Field Aligned pressure tensor and temperature are calculated as well. All quantities are calculated for both ions and electrons from a combination of ESA and SST data. Moments data are taken at spin resolution in all ESA survey modes except burst. The spacecraft potential, as measure by the EFI, is used to correct for spacecraft charging by shifting the particle energies for calculation; this eliminates contamination from photo-electrons. Also, weighting factors are used to account for instrument specific energy and angle efficiency variations. Table 1: Coordinate Descriptions. Despun Sun - L-vector (DSL): Z-axis points towards the spin axis, the Y-axis is obtained from the cross product of Z and the Spacecraft-Sun direction as viewed from the probe. The X-axis sits in the Z-axis-Sun plane and completes a right handed system. Geocentric Solar Ecliptic (GSE): Z-axis is normal to the solar ecliptic, the X-axis points from earth towards the Sun, and Y complets a right handed system. Geocentric solar Magnetosphereic (GSM): X-axis points from Earth to the Sun, the Y-axis is orthogonal to the Earth's magnetic dipole and points towards the dusk side, and the X-Z plane contains the dipole axis. Magnetic Field Aligned (MFA): Z-axis points along magnetic field lines, the Y-axis is the orthonormal cross product of the Z-axis and a vector pointing towards the Sun, and the X-axis completes the right handed system.

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