2D Stochastic Monte Carlo to evaluate the modulation of GCR for inner and outer solar system planets

Details 2D Stochastic Monte Carlo to evaluate the modulation of GCR for inner and outer solar system planets 2D Stochastic Monte Carlo to evaluate the modulation of GCR for inner and outer solar system planets

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apsp.conf..881b&link_type=abstract

ASTROPARTICLE, PARTICLE AND SPACE PHYSICS, DETECTORS AND MEDICAL PHYSICS APPLICATIONS. Proceedings of the 10th Conference. Held

Physics

Medical Physics

Heliosphere, Cosmic Rays, Modulation

Scientific paper

We developed a 2D Stochastic Monte Carlo model for Cosmic Rays propagation in the Heliosphere. The model solves numerically the transport equation of particles in the heliosphere, including major processes affecting the heliospheric particle transport: diffusion, convection, adiabatic energy losses and drift of particles. We evaluated the modulated flux at several distances from the Sun (i.e. at planetary distances) and compared our results for both solar polarities with measurements of CR protons at the Earth distance, 1 AU.

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