Low-energy protons: Gradients in interplanetary space and distribution in the solar corona

Details Low-energy protons: Gradients in interplanetary space and distribution in the solar corona Low-energy protons: Gradients in interplanetary space and distribution in the solar corona

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..234s&link_type=abstract

In JPL A Close-up of the Sun p 234-239 (SEE N78-32964 23-92)

Physics

Anisotropy, Interplanetary Medium, Proton Energy, Proton Flux Density, Solar Corona, Solar Protons, Interplanetary Magnetic Fields, Mission Planning, Solar Probes, Spaceborne Telescopes, Spacecraft Orbits

Scientific paper

First and second order anisotropy measurements are proposed as a tool
for studying the coronal source function and interplanetary propagation
of low energy protons. Optimum orbit and attitude requirements are
suggested for a three telescope system. Some limitations with regard to
the lower energy limit for a feasible set-up are discussed.

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