Physics
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh12c..10k&link_type=abstract
American Geophysical Union, Fall Meeting 2001, abstract #SH12C-10
Physics
2118 Energetic Particles, Solar, 2139 Interplanetary Shocks, 7513 Coronal Mass Ejections, 7514 Energetic Particles (2114)
Scientific paper
Interplanetary transport of energetic charged particles normally is treated in terms of focusing in the large scale magnetic field and pitch angle scattering at magnetic field inhomogenities. We have incorporated shocks as particle sources and shells of enhanced interplanetary scattering as well as coronal mass ejections (CMEs) as deformations of the interplanetary magnetic field into a numerical solution of the standard focued transport model to study particle propagation in the presence of multiple shocks and CMEs. Special attention is paid to the storage of particles betwenn pairs of shocks/CMEs because this seems to be important for particle acceleration and the creation of unusually large particle events. The reflection of particles from the leading shock has been identified as crucial parameter. Different physical scenarios (scattering in downstream turbulence, reflection at the converging field yround the CME) for this reflection are discussed.
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