Abstract
An investigation of electron acceleration in the auroral precipitation region of the magnetosphere is made. In particular a determination of the mechanisms that could produce the observed power law distribution in energy and the positive slope in the distribution function are described.
Original language | English |
---|---|
Pages (from-to) | 24-27 |
Number of pages | 4 |
Journal | Physica Scripta |
Volume | T82 |
DOIs | |
Publication status | Published - 1999 |
Keywords
- auroral phenomena
- magnetosphere
- energetic particle precipitation