The process of diffusive acceleration of charged particles in shocked plasmas is widely invoked in astrophysics to account for the ubiquitous presence of signatures of non-thermal relativistic electrons and ions in the universe. A key characteristic of this statistical energization mechanism is the
โฆ LIBER โฆ
Shock acceleration of solar cosmic rays
โ Scribed by E. G. Berezhko; S. N. Taneev
- Book ID
- 110135175
- Publisher
- Springer
- Year
- 2003
- Tongue
- English
- Weight
- 291 KB
- Volume
- 29
- Category
- Article
- ISSN
- 1063-7737
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