Comparison Between the White-Light and Green Emission Coronae

Details Comparison Between the White-Light and Green Emission Coronae Comparison Between the White-Light and Green Emission Coronae

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aspc..205...32m&link_type=abstract

Last Total Solar Eclipse of the Millennium, ASP Conference Series, Vol. 205. Edited by W. Livingston and A. Özgüç. ISBN: 1-58

Computer Science

4

Scientific paper

We have carried out a region-distribution study of both the white-light corona and green emission corona (Fe XIV 530.3 nm). The goal has been to find a relation between both the white-light and green emission coronae. Using the non-eclipse observations of the white-light coronal images obtained at Mauna Loa Mark-III with the K-coronameter a comparison is made with the green emission corona intensity as observed at Lomnický štít coronal station. It was found that there is a strong relation between regions of maximum intensity of the white-light coronal structures and the green emission corona intensity.

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