An alternative approach to the modeling of anomalous cosmic ray intensities in the heliosphere

Details An alternative approach to the modeling of anomalous cosmic ray intensities in the heliosphere An alternative approach to the modeling of anomalous cosmic ray intensities in the heliosphere

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19..805s&link_type=abstract

Advances in Space Research, Volume 19, Issue 5, p. 805-808.

Computer Science

4

Scientific paper

We have done a numerical solution of the cosmic ray transport equation to simulate a heliosphere containing a discontinuous solar wind termination shock in the outer heliosphere. Our previous studies demonstrated how hydrogen spectra could be explained by a no-drift modulation model, including an estimate of the size of the relative contribution of the anomalous H component. In this contribution we concentrate on a simplified diffusion model which allows us to better study the effects of particle drifts on anomalous cosmic rays.

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