Fine structure of polarized flare elements
Abstract
The investigation of linear polarization of solar emission features is being continued. From the spectral observations in the Hα line obtained with high spatial resolution it was found that in a distance scale of some arcsecond in some flare knots not only the value but also the sign of the polarization determined by the authors 1983 is changed. In the flare region some emission knots like moustaches or grains of continuous emission show strong polarization.
- Publication:
-
Izvestiya Ordena Trudovogo Krasnogo Znameni Krymskoj Astrofizicheskoj Observatorii
- Pub Date:
- 1985
- Bibcode:
- 1985IzKry..70....3B
- Keywords:
-
- Emission Spectra;
- H Alpha Line;
- Linear Polarization;
- Polarization Characteristics;
- Solar Flares;
- Solar Spectra;
- Fine Structure;
- Spectrophotometry;
- Solar Physics