Spectroscopic Observations of Coronal Emission Lines and their Relation to Soft X-ray Images

Details Spectroscopic Observations of Coronal Emission Lines and their Relation to Soft X-ray Images Spectroscopic Observations of Coronal Emission Lines and their Relation to Soft X-ray Images

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..113i&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.113-116.

Computer Science

3

Scientific paper

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.

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