The influence of the Earth's magnetosphere on the high-energy solar protons

Details The influence of the Earth's magnetosphere on the high-energy solar protons The influence of the Earth's magnetosphere on the high-energy solar protons

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..363b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 363-366 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Earth Magnetosphere, Flux Density, Geomagnetism, High Energy Electrons, Polar Regions, Solar Protons, Earth Atmosphere, Energetic Particles, Energy Spectra, Flux (Rate), Magnetic Storms, Penumbras

Scientific paper

In the Earth's polar regions the intensity of the solar protons with the energy above the critical energy of geomagnetic cutoff is the same as in the interplanetary space. The penumbra in the polar regions is small and the East-West effect is also small. However the geomagnetic cutoff rigidity Rc in polar regions is difficult to calculate because it is not sufficient to include only the internal sources of the geomagnetic field. During the magneto-quiescent periods the real value of Rc can be less by 0.1 GV than the calculated value because of the external sources. During the geomagnetic storms the real value of Rc is still lower.

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