2D stochastic simulation model of cosmic ray modulation: comparison with experimental data

Details 2D stochastic simulation model of cosmic ray modulation: comparison with experimental data 2D stochastic simulation model of cosmic ray modulation: comparison with experimental data

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..637b&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

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2

Galactic Cosmic Rays, Modulation, Heliosphere

Scientific paper

We developed a 2D stochastic simulation model for heliospheric propagation of galactic cosmic rays. The model solves numerically the transport equation of particles in the heliosphere. In the calculation we use also drift effects which are included through analytical effective drift velocities. We estimated the cosmic rays spectrum at 1 AU using this model formalism. The calculated spectra are compared with other models (CREME96) and with experimental data (IMP8 and AMS) for positive (A>0) and negative (A<0) solar periods.

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