Significance of observations for modeling of sunspots and their groups development
Abstract
The model of magnetic lines of force spread in a regular sunspot contradicting the observable distribution of bright penumbral fibrils in regular spots close to the solar limb is discussed as well as the dynamical effects seen in the photosphere due to the sunspots motion and collision.
- Publication:
-
Hvar Observatory Bulletin
- Pub Date:
- 1982
- Bibcode:
- 1982HvaOB...6..101B