2.3.2 spase://NASA/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Solar Electron Proton Telescope (SEPT) 1-min Level 1 Electron and Proton Spectra 2021-04-27T15:38:11Z 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. Please acknowledge the IMPACT P.I., Janet Luhmann of UCB spase://SMWG/Person/Janet.G.Luhmann PrincipalInvestigator SEPT site at U. Kiel http://www2.physik.uni-kiel.de/stereo/index.php?doc=home CDAWeb Skeleton Table https://cdaweb.gsfc.nasa.gov/pub/software/cdawlib/0SKELTABLES/stb_l1_sept_00000000_v01.skt spase://VEPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M spase://VSPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=STB_L1_SEPT&index=sp_phys STB_L1_SEPT With subset, plot and ASCII list functions from CDAWeb FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/stereo/behind/l1/impact/sept/ HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/stereo/behind/l1/impact/sept/ In CDF via HTTP from SPDF CDF 3275 kB P1D Please acknowledge the P.I., Janet Luhmann of UCB, and CDAWeb at GSFC/SPDF spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi STB_L1_SEPT@0 STB_L1_SEPT@1 Web Service to this product using the HAPI interface. CSV Please acknowledge the P.I., Janet Luhmann of UCB, and CDAWeb at GSFC/SPDF spase://SMWG/Instrument/STEREO-B/IMPACT/SEPT EnergeticParticles 2006-11-13T00:00:00 -P5M PT1M Heliosphere.Remote1AU Electron spectrum viewing northward from ecliptic plane Spec_0_NS Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed northward from the ecliptic plane PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 electron fluxes -1.0e+31 Electron NumberFlux Electron spectrum viewing southward from ecliptic plane Spec_2_NS Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed southward from the ecliptic plane PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 electron fluxes -1.0e+31 Electron NumberFlux Proton spectrum viewing northward from ecliptic plane Spec_3_NS Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed northward from the ecliptic plane PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 proton fluxes -1.0e+31 Proton NumberFlux Proton spectrum viewing southward from ecliptic plane Spec_1_NS Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed southward from the ecliptic plane PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 proton fluxes -1.0e+31 Proton NumberFlux Electron spectrum viewing sunward along the Parker IMF angle Spec_2_E Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed sunward along the Parker IMF spiral angle PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 electron fluxes -1.0e+31 Electron NumberFlux Electron spectrum viewing antisunward along the Parker IMF angle Spec_0_E Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed antisunward along the Parker IMF spiral angle PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 electron fluxes -1.0e+31 Electron NumberFlux Proton spectrum viewing sunward along the Parker IMF angle Spec_1_E Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed sunward along the Parker IMF spiral angle PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 proton fluxes -1.0e+31 Proton NumberFlux Proton spectrum viewing antisunward along the Parker IMF angle Spec_3_E Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed antisunward along the Parker IMF spiral angle PT1M 1/(sec sr cm^2 MeV) 32 Set of 32 proton fluxes -1.0e+31 Proton NumberFlux