May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ohbp.conf..165k&link_type=abstract
"In: The outer heliosphere: beyond the planets. Based on the spring school "Die äußere Heliosphäre - Jenseits der Planeten, in B
Physics
1
Galactic Cosmic Rays
Scientific paper
This chapter gives a brief review of galactic cosmic rays. It starts with observations made on the Earth, in near-Earth space and at larger distances and higher heliographic latitudes. In the subsequent sections, the physical processes leading to modulation, that are scattering at magnetic field irregularities, convection with the solar wind, drifts in the large-scale heliospheric magnetic field, and adiabatic deceleration, will be attempts to solve this equation will be presented. A comparison with observations shows that the basic understanding of the modulation process seems to be fairly well developed, although details, in particular the relative importance of drifts, still are subject to debate.
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