  The differential intensities of Cosmic Rays at Earth were calculated using a
2D stochastic Montecarlo diffusion code and compared with observation data. We
evaluated the effect of stretched and compressed heliospheres on the Cosmic Ray
intensities at the Earth. This was studied introducing a dependence of the
diffusion parameter on the heliospherical size. Then, we found that the optimum
value of the heliospherical radius better accounting for experimental data. We
also found that the obtained values depends on solar activity. Our results are
compatible with Voyager observations and with models of heliospherical size
modulation.
