1994•International Astronomical Union ColloquiumRequires access

Possible Influence of Large Structures of Coronal Magnetic Fields on the Propagation of Solar Cosmic Rays

S. Fischer, M. Vandas, Eduard V. Vashenyuk

Abstract

Abstract An investigation of mutual positions of footpoints of the Earth in the solar corona and the heliospheric current sheet (for both relativistic and nonrelativistic solar cosmic ray events) has not revealed any apparent dependence of observed SCR increases on the coronal distance of footpoints from the neutral line.

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Key concepts: Physics, Heliospheric current sheet, Cosmic ray, Astrophysics, Corona (planetary geology), Nanoflares, Coronal mass ejection, Coronal hole