3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
Contribution Poster (WITHDRAWN)
SH.3.1
2D Stochastic Monte Carlo to evaluate the modulation of GCR for inner and outer solar system planets
Speakers
- Dr. Davide GRANDI
Primary authors
- Dr. Davide GRANDI (INFN Milano Bicocca, Milano, Italy)
Co-authors
- Dr. Piergiorgio RANCOITA (INFN Milano Bicocca, Milano, Italy)
- Prof. Massimo GERVASI (Universita' di Milano Bicocca, Milano, Italy)
- Dr. Pavol BOBIK (IEP SAS Kosice, Slovakia)
- Prof. Giuliano BOELLA (Universita' di Milano Bicocca, Milano, Italy)
- Dr. Simonetta PENSOTTI (INFN Milano Bicocca, Milano, Italy)
- Dr. Matteo J. BOSCHINI (INFN Milano Bicocca, Milano, Italy)
- Prof. Karel KUDELA (IEP SAS Kosice, Slovakia)
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.