Form of the anomalous cosmic ray spectrum at the solar wind termination shock

Details Form of the anomalous cosmic ray spectrum at the solar wind termination shock Form of the anomalous cosmic ray spectrum at the solar wind termination shock

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...10424879s&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue A11, p. 24879-24884

Physics

22

Interplanetary Physics: Cosmic Rays, Interplanetary Physics: Energetic Particles, Heliospheric, Interplanetary Physics: Heliopause And Solar Wind Termination

Scientific paper

New insights regarding the form of the accelerated anomalous cosmic ray spectrum at the solar wind termination shock, obtained from solutions of the cosmic ray transport equation, are presented. A simple analytical expression for the spectrum on the shock is derived, and its dependence on the acceleration parameters is shown. Particular attention is paid to the high-energy cutoff of this spectrum. This expression and its parameterization should be applicable for the acceleration of charged particles in any spherical shock.

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