Cosmic ray modulation and the heliosphere

Details Cosmic ray modulation and the heliosphere Cosmic ray modulation and the heliosphere

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc...27.....e&link_type=abstract

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

Physics

Scientific paper

We reproduce the long term temporal variations of galactic cosmic ray intensity applying a semi-empirical 1-D diffusion-convection model. We use a shell-like model in which each magnetized shell modulates the cosmic ray intensity during its travel from the Sun to the heliospheric boundary. The cosmic ray intensity at the Earth's orbit is the result of the successive dynamic influence of all shells between the Earth and the heliospheric boundary. Our results are in very good agreement with ground-based observations from Climax and Huancayo cosmic ray stations.

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