Galactic cosmic rays in the heliosphere

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Scientific paper

This review covers the sessions SH 3.1-3.5: ``Galactic cosmic rays in the heliosphere'' of the 26th International Cosmic Ray Conference held in Salt Lake City, Utah, in August 1999. The subtopics are modulation models, long-term variations, gradients, anisotropies, and spectra, composition & charge state. Noteworthy contributions include a number of new models, numerical simulations of transport coefficients-including the first of the drift coefficient-that highlight the continuing problems with perpendicular transport, various other attempts to pin down the spatial and rigidity dependence of the diffusion tensor, charge-dependent modulation and especially the role of the wavy current sheet, and the Gnevyshev gap during solar maximum conditions. .

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