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| 1) | STEREO-B IMPACT/LET 1-min Level 1 Ion Fluxes |
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| Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/LET/L1/PT1M | ||||||||||||||||||
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| 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-B IMPACT/SEPT 1-min Level 1 Electron and Proton Spectra |
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| Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M | ||||||||||||||||||
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| 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-B IMPACT/SIT 1-min Level 1 Multi-Z Ion Spectra |
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| Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/SIT/L1/PT1M | ||||||||||||||||||
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| 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-B IMPACT/STE 10-s Level 1 Electron Spectra |
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| Resource ID:spase://VEPO/NumericalData/STEREO-B/IMPACT/STE/L1/PT10S | ||||||||||||||||||
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| 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. | ||||||||||||||||||
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