Observational aspects of the study of plasma turbulence in solar flares.
Abstract
Using two techniques (the polarization method and the Baranger-Mozer method) a study has been made of plasma turbulence in solar emission features. The study suggests the conclusion that the 0.02 - 0.03 plasma turbulence level (E = 1 - 2 kV cm-1) seems to be the highest achieved in flares.
- Publication:
-
Journal of Quantitative Spectroscopy and Radiative Transfer
- Pub Date:
- July 1990
- DOI:
- 10.1016/0022-4073(90)90099-R
- Bibcode:
- 1990JQSRT..44..177F
- Keywords:
-
- Plasma Diagnostics;
- Plasma Frequencies;
- Plasma Turbulence;
- Solar Flares;
- Spectral Line Width;
- Balmer Series;
- Chromosphere;
- Plasma Oscillations;
- Solar Physics;
- Solar Flares: Plasma;
- Solar Flares: Turbulence