Cosmic Ray Modulation and the Evolution of the Solar Magnetic Field

Physics

Scientific paper

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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.

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