The 1973-1984 Solar Modulation of Cosmic Ray Nuclei

Details The 1973-1984 Solar Modulation of Cosmic Ray Nuclei The 1973-1984 Solar Modulation of Cosmic Ray Nuclei

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..409g&link_type=abstract

Proceedings from the 19th International Cosmic Ray Conference, Volume 4 (SH Sessions), p.409

Physics

Scientific paper

Measurements of the intensity time variations and differential energy spectra during 1973 - 1984 are interpreted in the frame of a conventional model of solar modulation which assumes steady state (i.e. equilibrium) and absence of drifts. By using empirical diffusion coefficients and their time variations it is found that the model can reproduce at 1 AU the main features of time intensity variations and differential energy spectra of cosmic ray nuclei through the entire solar modulation cycle.

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