Transfer of energy within coronal bright points according to the observation in optical spectra and microwave
Abstract
The paper is devoted to the coronal bright points. We carried out the analysis of the simultaneous observations in IR He λ10830 Å and microwaves at 5.2 and 1.76 cm. It was obtained that microwave sources correspond to the dark points in IR He λ10830 Å with line-of-sight velocities directed from a observer. The possible mechanism of the energy transport within the bright points are suggested.
- Publication:
-
Multi-Wavelength Investigations of Solar Activity
- Pub Date:
- 2004
- DOI:
- Bibcode:
- 2004IAUS..223..479P