Radial Intensity Profiles of Galactic Cosmic Rays in the Outer Heliosphere

Details Radial Intensity Profiles of Galactic Cosmic Rays in the Outer Heliosphere Radial Intensity Profiles of Galactic Cosmic Rays in the Outer Heliosphere

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3827m&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

This contribution describes our understanding of galactic cosmic ray (GCR) proton (H) and α particle (He++ ) intensities during the solar minimum conditions of 1987 and 1977/1997, with emphasis on the radial profiles in the outer heliosphere. This is done with a model that contains all the relevant physics of the solar wind termination shock with its acceleration and shock drift effects, the appropriate heliosheath modulation, drifts in the heliospheric magnetic field (HMF), as well as drifts along a wavy neutral sheet in the ecliptic plane.

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