Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1039..258l&link_type=abstract
PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND: 7th Annual International Astrophysics Conference. AIP Confer
Astronomy and Astrophysics
Astrophysics
2
Particle Emission, Solar Wind, Planetary Bow Shocks, Interplanetary Shocks, Particle Acceleration, Coronal Mass Ejection, Magnetohydrodynamics And Plasmas
Scientific paper
A time-dependent focused transport model is used to model how solar wind protons are injected from the suprathermal tail of the solar wind distribution into diffusive shock acceleration at both a strong and a weak coronal mass ejection-driven shock. It is discussed how the temporal evolution of the injection and acceleration process can result in solar energetic particle spectra that differ substantially from the prediction of standard steady state diffusive shock acceleration models.
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