AP-8 trapped proton environment for solar maximum and solar minimum

Details AP-8 trapped proton environment for solar maximum and solar minimum AP-8 trapped proton environment for solar maximum and solar minimum

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7718983s&link_type=abstract

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Computer Programs, Periodic Variations, Proton Flux Density, Solar Flux, Solar Protons, Trapped Particles, Azur Satellite, Data Systems, Magnetic Fields, Ov-3 Satellites, Solar Cycles

Scientific paper

Data sets from Ov-3 and Azur indicate a need for improvement in models of the stably trapped proton flux with energies between 0.1 and 400 MeV. Two computer accessible models are described: AP8MAX and AP8MIN. The models are presented in the form of nomographs, B-L plots, R-lambda plots, and equatorial radial profiles. Nomographs of the orbit-integrated fluxes are also discussed. The models are compared with each other, with the data, and with previous AP models. Requirements for future improvements include more complete data coverage and periodic comparisons with new data sets as they become available. The machine-sensible format in which the models are available are described.

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