Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3826c&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
4
Scientific paper
The modulation of cosmic rays in the heliosphere is directly related to the structure and strength of the interplanetary magnetic field which at 1 AU is primarily caused by variations of the solar magnetic field. In this study we examine how the field evolves over timescales of months, and how the cosmic rays respond to these variations, for several interesting periods, including the onset of cycle 23. Also considered is the contribution of coronal mass ejections to the interplanetary magnetic field.
Cane Hilary V.
Richardson Ian G.
Wibberenz Gerd
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