Interpreting Cosmic Rays in the Current Anomalous Sunsport Minimum (Invited)

Details Interpreting Cosmic Rays in the Current Anomalous Sunsport Minimum (Invited) Interpreting Cosmic Rays in the Current Anomalous Sunsport Minimum (Invited)

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.u34a..08j&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #U34A-08

Physics

Plasma Physics

[7536] Solar Physics, Astrophysics, And Astronomy / Solar Activity Cycle, [7807] Space Plasma Physics / Charged Particle Motion And Acceleration

Scientific paper

The current anomalous sunspot minimum provide a uniquie opportunity to study solar modulation of cosmic rays in a new range of parameter space. In this talk, our present basic understanding of cosmic-ray transport will be discussed. Possible interpratations of the observed properties of cosmic ray intensity are discussed in terms of the observed solar wind and its magnetic field. Both the low solar- wind velocity and the low value of the magnetic field may contribute to the observed high cosmic-ray intensity. The time delay between the variation in the solar-wind parameters and the cosmic-ray intensity will also be discussed as a constraint on possible interpretations.

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