This data set contains hourly, spin-averaged
fluxes of electrons from the IMP8 Cosmic Ray Nuclear Composition
experiment of U. Chicago and UNH. There are fluxes of electrons
in three energy bins: 0.7-2.0, 2-12, 12-50 MeV. These fluxes
were generated at GSFC/SPDF from count rates accessible from
UNH.
Version:2.2.9
This data set contains hourly, spin-averaged
fluxes of electrons from the IMP8 Cosmic Ray Nuclear Composition
experiment of U. Chicago and UNH. There are fluxes of electrons
in three energy bins: 0.7-2.0, 2-12, 12-50 MeV. These fluxes
were generated at GSFC/SPDF from count rates accessible from
UNH.
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | PrincipalInvestigator | spase://SMWG/Person/Clifford.Lopate |
SFDU-formatted file describing the CRNC instrument
and the 15-min data set of count rates and pulse height data from which the
hourly rates data set was created. Division of hourly rates by geometric
factor and energy band widths yielded the hourly fluxes.
ftp access to electron-specific subdirectory
holding annual ASCII files
In CDF via HTTP from SPDF
Subset, plot and list fluxes of protons, alpha
particles and electron, and count rates of heavies, via FTPBrowser
Time at start of flux average, as year, day, hour
year, day, hour
Fractional counting coverage (0-1) during this hour
Spin-integrated fluxes of electrons, at 1-hour resolution,
in three energy bins: 0.7-2.0, 2-12, 12-50 MeV
Array of fluxes at 3 energy windows