Injection Efficiency of Low-energy Particles at Oblique Shocks with a Focused Transport Model
Abstract
There is strong evidence that a small portion of thermal and suprathermal particles from hot coronal material or remnants of previous solar energetic particle (SEP) events serve as the source of large SEP events (Desai et al. 2006). To build more powerful SEP models, it is necessary to model the detailed particle injection and acceleration process for source particles especially at lower energies. We present a test particle simulation on the injection and acceleration of low-energy suprathermal particles by Laminar nonrelativistic oblique shocks in the framework of the focused transport theory, which is proved to contain all necessary physics of shock acceleration, but avoid the limitation of diffusive shock acceleration (DSA). The injection efficiency as a function of Mach number, obliquity, injection speed, shock strength, cross-shock potential and the degree of turbulence is calculated. This test particle simulation proves that the focused transport theory is an extension of DSA theory with the capability of predicting the efficiency of particle injection. The results can be applied to modeling the SEP acceleration from source particles.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2013
- Bibcode:
- 2013AGUFMSH21A2071Z
- Keywords:
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- 7984 SPACE WEATHER Space radiation environment;
- 7514 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY Energetic particles;
- 7845 SPACE PLASMA PHYSICS Particle acceleration;
- 7811 SPACE PLASMA PHYSICS Discontinuities