Abstract
Using analytic theory, test-particle simulations, and self-consistent hybrid simulations, we show that quasi-perpendicular shocks - those which propagate nearly perpendicular to the upstream magnetic field - accelerate particles directly out of the incident thermal population to energies much higher than the upstream ram energy of the plasma. It has already been established that quasi-parallel shocks - those which propagate nearly in the same direction as the upstream magnetic field - efficiently accelerate particles directly out of the incident thermal population; however, this has not yet been established for quasi-perpendicular shocks. Our results can be understood within the framework of the diffusive shock acceleration theory. We find that the accelerated-particle spectrum obtained from a more-general self-consistent hybrid plasma simulation are quantitatively consistent with a less-sophisticated test-particle simulation. The implications of this are discussed.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 659-664 |
| Number of pages | 6 |
| Journal | Planetary and Space Science |
| Volume | 51 |
| Issue number | 11 |
| DOIs | |
| State | Published - Sep 2003 |
Keywords
- Collisionless shocks
- Cosmic rays
- Numerical simulation studies
- Particle acceleration
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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