Probing flare temperatures using AIA dispersion effects and RHESSI imaging/spectroscopy
Abstract
Diffraction patterns that occur as a result of very intense, often saturated emission can provide many useful tools not ordinarily available. Specifically, analyzing dispersion features of high order diffraction patterns can provide useful insight into the thermal distributions of plasma within a structure. Here, we analyze the diffraction patterns of multiple SDO/AIA wavelength bands to more than 40 orders. Combining these results with imaging and spectroscopy from RHESSI enabled us to probe temperature and emission measure distributions within saturated flare sources.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2010
- Bibcode:
- 2010AGUFMSH23A1828R
- Keywords:
-
- 7519 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Flares;
- 7549 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Ultraviolet emissions;
- 7594 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Instruments and techniques