Large-Scale Shining Chains on the Solar Disk: Nobeyama Radioheliograph Data
Abstract
Consideration of the Nobeyama radioheliograms at 17 GHz with a restricted range of the brightness temperature (Tb≈ (5-20)× 103 K) revealed a novel phenomenon of the large-scale solar activity: long-living (days) and transient (hours) microwave shining chains of characteristic sizes comparable with the solar disk diameter and consisting of 30--60'' blobs.
- Publication:
-
Proceedings of the Nobeyama Symposium
- Pub Date:
- December 1999
- Bibcode:
- 1999spro.proc..175C