2.3.2 spase://NASA/NumericalData/Wind/3DP/EESA_HIGH/SP/PT24S Wind 3DP 24-sec ESSA-HIGH Electron Omnidirectional Fluxes https://doi.org/10.48322/c201-q577 2021-05-31T12:34:56.789 2021-05-31T12:34:56.789 Updated to SPASE Version 2.3.2 if needed, Applied quality control for DOI usage, LFB Electron omnidirectional fluxes 100 eV-30 keV, often at 24 sec, EESA High, Wind 3DP - R. Lin (UC Berkeley) Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC Lin, Robert P.; Bale, Stuart D.; & Wilson III, Lynn B. 2021-01-01T00:00:00 NASA Space Physics Data Facility and the Space Sciences Laboratory, University of California, Berkeley spase://SMWG/Person/Robert.P.Lin PrincipalInvestigator spase://SMWG/Person/Stuart.D.Bale PrincipalInvestigator spase://SMWG/Person/Robert.E.McGuire GeneralContact Caveats to the use of Wind 3DP data https://spdf.gsfc.nasa.gov/pub/data/wind/3dp/wind3dp_caveats.pdf Caveats for the correct use of Wind 3DP datasets Wind 3DP home page at UCB http://sprg.ssl.berkeley.edu/wind3dp/ home page at UCB (with plotting and digital data) spase://VSPO/NumericalData/Wind/3DP/EESA_HIGH/SP/PT24S spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/wind/3dp/3dp_ehsp/ In CDF via ftp from SPDF HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/wind/3dp/3dp_ehsp/ In CDF via HTTP from SPDF CDF Please acknowledge the CDAWeb team at GSFC/SPDF. spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=WI_EHSP_3DP&index=sp_phys WI_EHSP_3DP Text spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi WI_EHSP_3DP Web Service to this product using the HAPI interface. CSV spase://SMWG/Instrument/Wind/3DP EnergeticParticles 1994-12-20T15:10:03.000Z -P30D PT24S Heliosphere.NearEarth With respect to time resolution: 24 sec timing changes and is not necessarily constant, depending on the mode that the instrument happens to be in. Not only does the period/interval between each point change, the duration over which the data were taken can change as well. Epoch Epoch Number of milliseconds since CDF_EPOCH: 0000-01-01T00:00:00.000. ms 1e-3>s 01-Jan-1956 00:00:00.000 01-Jan-2083 00:00:00.000 -1.0E31 Temporal Unix Time TIME Time since 1970-01-01T00:00:00Z in seconds s Temporal Electron Flux FLUX Electron differential number flux 100 eV - 30 keV, as a function of energy #/(cm^2*ster*eV*s) Electron NumberFlux Electron Energy ENERGY Average electron energy eV 15 The 15 average electron energies Electron Average Energy 100 30000 eV