Constraints for Electron Acceleration Models in Solar Flares from Microwave Observations with High Spatial Resolution
Abstract
In this study we show that different locations of acceleration/injection sites in flaring loops may produce different types of pitch-angle distributions of accelerated electrons and, as a consequence, very different spatial, spectral and polarization properties of the loop microwave emission. These properties can be detected using spatially resolved microwave observations of specific flaring loops and be used to choose the most suitable electron acceleration model.
- Publication:
-
Hinode-3: The 3rd Hinode Science Meeting
- Pub Date:
- August 2012
- Bibcode:
- 2012ASPC..454..321M