Galactic cosmic ray intensity dynamics in the presence of large-scale solar wind disturbances

Details Galactic cosmic ray intensity dynamics in the presence of large-scale solar wind disturbances Galactic cosmic ray intensity dynamics in the presence of large-scale solar wind disturbances

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009astl...35..701p&link_type=abstract

Astronomy Letters, Volume 35, Issue 10, pp.701-711

Astronomy and Astrophysics

Astronomy

Scientific paper

We have developed a method of relativistic particle trajectories to model the cosmic ray intensity dynamics in the presence of solar wind disturbances. The probability of detecting the precursors of disturbances has been found to depend on various conditions. In general, the dynamics of the distribution of precursors at the magnetospheric surface is in agreement with measurements.

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