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1) STEREO-A IMPACT/LET 1-min Level 1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/LET/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO A Cadence:1 minute
Stop:2014-11-25 01:00:47 Instrument:STEREO-A IMPACT Low Energy Telescope Resource:NumericalData
The IMPACT Low Energy Telescope (LET) data consist of 1-min resolution unsectored fluxes and counts for each of 15 single-Z ionic species at each of a species-dependent number of energy bins ranging between 9 and 16, plus 16-sectored fluxes and counts for 5 ionic species or Z groups in one (H) or two (He4, CNO, NiMgSi, Fe) energy ranges. There is much fill data. (

2) STEREO-A IMPACT/SEPT 1-min Level 1 Electron and Proton Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/SEPT/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO A Cadence:1 minute
Stop:2014-11-25 01:00:47 Instrument:STEREO-A IMPACT SEPT Resource:NumericalData
The IMPACT Solar Electron Proton Telescope (SEPT) Level 1 data consist of electron and proton fluxes from each of 32 energy bands that span ~20 keV to 2000(electrons) or 7000(protons) keV. These spectra are determined each minute, in each of 4 directions with 60 deg fields of view (parallel and anti-parallel to the Parker magnetic field direction, and northward and southward from the ecliptic plane.

3) STEREO-A IMPACT/SIT 1-min Level 1 Multi-Z Ion Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/SIT/L1/PT1M
Start:2007-03-15 00:00:00 Observatory:STEREO A Cadence:1 minute
Stop:2014-11-25 01:00:46 Instrument:STEREO-A IMPACT SIT Resource:NumericalData
The IMPACT Suprathermal Ion Telescope (SIT) data consist of 1-min resolution ion fluxes of the following species (and numbers of energy bands, typically spanning ~0.04-9 MeV/n): H(12), 3He(10), 4He(16), C(17), O(16), NeS(16; neon through sulfur), Fe(14), UH(6; ultra heavy; 0.06-0.5 MeV/n), and associated uncertainties due to counting statistics.

4) STEREO-A IMPACT/STE 10-s Level 1 Electron Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-A/IMPACT/STE/L1/PT10S
Start:2006-11-01 00:00:00 Observatory:STEREO A Cadence:10 seconds
Stop:2009-08-04 00:00:00 Instrument:STEREO-A IMPACT STE Resource:NumericalData
The IMPACT Suprathermal Electron (STE) Telescope data consist of 10-sec resolution electron counts from each of 8 sensors in each of 32 energy bands that span 1.9 keV to 100 keV. Only four sensors provide unsaturated data that are scientifically usable.

5) STEREO-B IMPACT/LET 1-min Level 1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/LET/L1/PT1M
Start:2006-11-14 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2014-11-25 01:00:47 Instrument:STEREO-B IMPACT Low Energy Telescope Resource:NumericalData
The IMPACT Low Energy Telescope (LET) data consist of 1-min resolution unsectored fluxes and counts for each of 15 single-Z ionic species at each of a species-dependent number of energy bins ranging between 9 and 16, plus 16-sectored fluxes and counts for 5 ionic species or Z groups in one (H) or two (He4, CNO, NiMgSi, Fe) energy ranges. There is much fill data. (

6) STEREO-B IMPACT/SEPT 1-min Level 1 Electron and Proton Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M
Start:2006-11-13 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2014-11-25 01:00:47 Instrument:STEREO-B IMPACT SEPT Resource:NumericalData
The IMPACT Solar Electron Proton Telescope (SEPT) Level 1 data consist of electron and proton fluxes from each of 32 energy bands that span ~20 keV to 2000(electrons) or 7000(protons) keV. These spectra are determined each minute, in each of 4 directions with 60 deg fields of view (parallel and anti-parallel to the Parker magnetic field direction, and northward and southward from the ecliptic plane.

7) STEREO-B IMPACT/SIT 1-min Level 1 Multi-Z Ion Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/SIT/L1/PT1M
Start:2007-03-15 00:00:00 Observatory:STEREO B Cadence:1 minute
Stop:2014-11-25 01:00:47 Instrument:STEREO-B IMPACT SIT Resource:NumericalData
The IMPACT Suprathermal Ion Telescope (SIT) data consist of 1-min resolution ion fluxes of the following species (and numbers of energy bands, typically spanning ~0.04-9 MeV/n): H(12), 3He(10), 4He(16), C(17), O(16), NeS(16; neon through sulfur), Fe(14), UH(6; ultra heavy; 0.06-0.5 MeV/n), and associated uncertainties due to counting statistics.

8) STEREO-B IMPACT/STE 10-s Level 1 Electron Spectra maxmize
Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/STE/L1/PT10S
Start:2006-11-01 00:00:00 Observatory:STEREO B Cadence:10 seconds
Stop:2009-05-14 00:00:00 Instrument:STEREO-B IMPACT STE Resource:NumericalData
The IMPACT Suprathermal Electron (STE) Telescope data consist of 10-sec resolution electron counts from each of 8 sensors in each of 32 energy bands that span 1.9 keV to 100 keV. Only four sensors provide unsaturated data that are scientifically usable.

9) 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:2014-11-25 01:03:33 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).

10) 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:2014-11-25 01:03:35 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).

Showing 1 - 10