3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Poster (WITHDRAWN)

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

Speakers

  • Dr. Davide GRANDI

Primary authors

Co-authors

Abstract content

We developed a 2D model Stochastic Montecarlo 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 distancies from the sun (i.e. at planets distance) and we compared our results for both solar polarities with measurements of CR protons at the Earth distance, 1AU.