2.3.2 spase://NASA/NumericalData/IMP8/GME/PT30M IMP 8 Goddard Medium Energy (GME) 30-min energetic particle rates and fluxes 2021-04-27T15:38:11Z This CDAWeb-accessible data set contains 30-minute, spin-averaged count rates and fluxes, and their statistical uncertainties, of energetic particles from the IMP8 GME experiment. Included are fluxes of: protons in 30 energy bins from 0.88-1.15 to 327-485 MeV; alpha particles in 21 energy bins from 1.14-1.36 to 63.3-81.0 MeV/n; and 0.3-18 MeV electrons. Also included are count rates for each of 7 sensors and for 11 multi-sensor coincidence modes. Proton and alpha particle fluxes, for every other energy bin, are given at the FTPBrowser and MSSP interfaces identified below. Acknowledge Robert E. McGuire, the PI. spase://SMWG/Person/Robert.E.McGuire PrincipalInvestigator NSSDC Master Catalog https://nssdc.gsfc.nasa.gov/nmc/experiment/display.action?id=1973-078A-09 CDAWeb Skeleton Table https://spdf.gsfc.nasa.gov/pub/software/cdawlib/0SKELTABLES/i8_h0_gme_00000000_v01.skt spase://VEPO/NumericalData/IMP8/GME/PT30M spase://VSPO/NumericalData/IMP8/GME/PT30M spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/imp/imp8/particles_gme/data/flux/gme_h0/ ftp access to 6-month CDF files HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/imp/imp8/particles_gme/data/flux/gme_h0/ In CDF via HTTP from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=I8_H0_GME&index=sp_phys I8_H0_GME Subset, plot and list via CDAWeb; ASCII output option CDF 200 MB Acknowledge Robert E. McGuire, the PI, and CDAWeb spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi I8_H0_GME Web Service to this product using the HAPI interface. CSV Acknowledge Robert E. McGuire, the PI, and CDAWeb spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPBrowser https://omniweb.sci.gsfc.nasa.gov/ftpbrowser/imp8_gme_30m.html Subset, plot and list H and He fluxes Multi-Source Spectral Plot https://omniweb.sci.gsfc.nasa.gov/ftpbrowser/flux_spectr_m.html Spectral plots and power law fits for arbitrary durations for H and He fluxes Text Acknowledge Robert E. McGuire, the PI, SPDF and the service used spase://SMWG/Instrument/IMP8/MCGUIRE EnergeticParticles 1973-11-01T00:00:00 2001-10-26T00:00:00 PT30M Heliosphere.NearEarth Proton fluxes Spin-integrated fluxes of protons, at 30-min resolution, in 30 energy bins ranging from 0.88-1.15 MeV to 327-485 MeV, and statistical uncertainties in these fluxes PT30M 1/sec-cm**2-ster-MeV 30 2 Array of fluxes and corresponding uncertainties at 30 energy windows Proton NumberFlux 1 0.88 485 MeV Alpha particle fluxes Spin-integrated fluxes of alpha particles, at 30-min resolution, in 21 energy bins ranging from 1.14-1.36 MeV/n to 63.3-81.0 MeV/n, and statistical uncertainties in these fluxes PT30M 1/sec-cm**2-ster-MeV/n 21 2 Array of fluxes and corresponding uncertainties at 21 energy windows AlphaParticle NumberFlux 2 1.14 81 MeV/n Electron fluxes Spin-integrated fluxes of 3-18 MeV electrons, at 30-min resolution, and statistical uncertainties in these fluxes PT30M 1/sec-cm**2-ster-MeV 2 Array of one flux and its corresponding uncertainty Electron NumberFlux 3 18 MeV Electron background fluxes Spin-integrated fluxes considered as background for 3-18 MeV electron flux, at 30-min resolution, and statistical uncertainties in these fluxes PT30M 1/sec-cm**2-ster-MeV 2 Array of one flux and its corresponding uncertainty Electron NumberFlux