On the propagation of low energy solar protons in the interplanetary medium

Details On the propagation of low energy solar protons in the interplanetary medium On the propagation of low energy solar protons in the interplanetary medium

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....5.1761a&link_type=abstract

Presented at the 14th Intern. Cosmic Ray Conf., Munich, 15-29 Aug. 1975

Mathematics

Logic

Heos B Satellite, Interplanetary Medium, Particle Trajectories, Solar Protons, Anisotropy, Particle Energy, Particle Flux Density, Satellite Observation, Solar Wind, Topology

Scientific paper

The fluxes and anisotropies of low energy solar protons (less than 10 MeV) observed on two occasions when the HEOS-2 spacecraft encountered solar proton streams are studied taking into account the interplanetary magnetic field and plasma conditions existing at those times. (Plasma and magnetic field measurements are available from the same satellite). The variations in the streaming pattern are used to infer the topological structure of the interplanetary medium. The observed results are compared to existing models of particle propagation between the sun and the earth.

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