Spatial variation of cosmic rays near the heliospheric current sheet

Details Spatial variation of cosmic rays near the heliospheric current sheet Spatial variation of cosmic rays near the heliospheric current sheet

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..449j&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 449-452 (SEE N85-34729 23-92)

Statistics

Computation

Current Sheets, Diffusion Coefficient, Galactic Cosmic Rays, Heliosphere, Interplanetary Magnetic Fields, Magnetic Equator, Solar Magnetic Field, Cycles, Dependence, Models, Modulation

Scientific paper

A quantitative comparison between theoretical predictions and observations of the intensity of galactic cosmic rays near the interplanetary current sheet is reported. Comparison of model calculations is made with a statistical analysis of observations of galactic cosmic rays at Earth and the simultaneous position of the current sheet. An ensemble of different current sheet inclinations is used, in order to make the analysis of the computations approximate the method used to analyses the data.

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