Abstract
Microwave gyrosynchrotron radio emission generated by nonthermal electrons in twisted magnetic loops is modelled using the recently developed simulation tool GX Simulator. We consider isotropic and anisotropic pitch-angle distributions. The main scope of the work is to understand the impact of a twisted magnetic field topology on radio emission maps. We have found that nonthermal electrons inside twisted magnetic loops produce gyrosynchrotron radio emission with a particular polarisation distribution. The polarisation sign inversion line is inclined relatively to the axis of the loop. The radio emission source is more compact in the case of a less twisted loop, assuming an anisotropic pitch-angle distribution of nonthermal electrons.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1341-1355 |
| Number of pages | 15 |
| Journal | Solar Physics |
| Volume | 291 |
| Issue number | 5 |
| DOIs | |
| State | Published - May 1 2016 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Energetic particles
- Flares
- Radio
- X-rays