Spectroscopic Observations of Coronal Emission Lines and their Relation to Soft X-ray Images
Abstract
Spectroscopic observations of coronal emission lines were carried out to obtain the plasma distribution at different temperatures. Images in FeXIV5303A(green), FeX6374A(red) and CaXV5694A(yellow) are compared with the soft X-ray images taken with the Soft X-ray Telescope on board Yohkoh. It is found that the distributions of green and red lines are quit different from that of the soft X-rays, while the yellow line shows quite similar distribution.
- Publication:
-
Proceedings of Kofu Symposium
- Pub Date:
- July 1994
- Bibcode:
- 1994kofu.symp..113I