On the differential rotation of coronal holes.
Abstract
It is shown that the differential character of rotation of coronal holes is weakly pronounced (B ≡ 0.4) only near the solar minimum, i.e., in the period when the green corona also rotates rigidly. In other periods, coronal holes as well as the entire corona display a noticeable differential rotation (B ⪆ 1.0).
- Publication:
-
Byulletin Solnechnye Dannye Akademie Nauk SSSR
- Pub Date:
- 1988
- Bibcode:
- 1988BSolD1988...89O
- Keywords:
-
- Differential Rotation:Solar Coronal Holes;
- Solar Coronal Holes:Differential Rotation