An alternative approach to the modelling of galactic cosmic ray intensities in the heliosphere

Details An alternative approach to the modelling of galactic cosmic ray intensities in the heliosphere An alternative approach to the modelling of galactic cosmic ray intensities in the heliosphere

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19..901r&link_type=abstract

Advances in Space Research, Volume 19, Issue 6, p. 901-904.

Physics

6

Scientific paper

The first results from a different approach in the search for solutions of the transport equation to describe particle spectra measured during consecutive solar minimum periods, are presented. A simple two-dimensional no-drift model with kappa_rr independent of r and theta satisfactorily decribes the proton data measured at different radial distances during consecutive solar minimum periods. The negative latitudinal gradient between Voyagers 1 and 2 in 1987 is successfully modelled due to a latitudinally dependent solar wind speed.

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