Penetration of Solar Protons and Alphas to the Geomagnetic Equator

Details Penetration of Solar Protons and Alphas to the Geomagnetic Equator Penetration of Solar Protons and Alphas to the Geomagnetic Equator

Sep 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968phrvl..21..929l&link_type=abstract

Physical Review Letters, vol. 21, Issue 13, pp. 929-933

Physics

3

Scientific paper

Simultaneous spectral observations of low-energy solar particles in interplanetary space and in the magnetosphere on the equator strongly imply that these particles have essentially free access to the outer magnetosphere through a very effective diffusion mechanism which preserves the spectral shapes and the flux magnitudes. These observations further imply that measurements of solar-particle arrival time over the polar caps are not sufficient to distinguish between open or closed magnetosphere models.

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