A new cosmic ray modulation model for the 11-year and 22-year cycles

Details A new cosmic ray modulation model for the 11-year and 22-year cycles A new cosmic ray modulation model for the 11-year and 22-year cycles

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3694p&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

A heliospheric cosmic ray modulation model based on the numerical solution of Parker's transport equation will be presented. The model is developed to simulate time-dependent modulation for cosmic ray protons and electrons for full 11-year and 22-year cosmic ray cycles. The details of the model will be discuss and the results of the simulation will be compared to the observed 11-year and 22-year cycles and to the observed charge-sign dependence along the Ulysses trajectory.

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