Simulation of SEP Acceleration and Transport at CME-driven Shocks

Details Simulation of SEP Acceleration and Transport at CME-driven Shocks Simulation of SEP Acceleration and Transport at CME-driven Shocks

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..781..201k&link_type=abstract

THE PHYSICS OF COLLISIONLESS SHOCKS: 4th Annual IGPP International Astrophysics Conference. AIP Conference Proceedings, Volume

Astronomy and Astrophysics

Astronomy

7

Solar Cosmic Ray Particles, Solar Corona, Acceleration, Shock Waves, Solar Wind, Magnetic Fields, Astronomy Computing, Computer Aided Analysis, Particle Acceleration, Planetary Bow Shocks, Interplanetary Shocks, Interplanetary Magnetic Fields

Scientific paper

Our code of solar energetic particle (SEP) acceleration and transport developed in Arizona is combined with the realistic CME simulations of Michigan, using the solar wind and magnetic field data of the Michigan CME-simulation as input to the SEP code. We suggest that, in addition to the acceleration at the shock significant acceleration may also occur in the sheet behind the shock, where magnetic field lines are compressed as they are bent around the expanding cloud. We consider field aligned motion and cast the proper Fokker-Planck equation into a non-inertial comoving frame, that follows field lines as they evolve. Illustrative simulation results are presented.

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