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Joule heating in the photosphere and chromosphere

โœ Scribed by Kan, J. R.; Yamauchi, M.

Book ID
119715983
Publisher
American Geophysical Union
Year
1989
Tongue
English
Weight
612 KB
Volume
94
Category
Article
ISSN
0148-0227

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We analyse Fe i lines observed during the 1961 eclipse at Bra6, Yugoslavia (see paper II: van Dessel et aL, 1973), using a computer program for the calculation of theoretical line intensities, which was described in Paper I (van Dessel, 1970). A few minor modifications to the physical input are disc

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Eclipse observations of total line intensities (Cr ~: two groups of lines; Ti II, Fe II and Cr iI: two lines each) are interpreted in terms of departures from LTE. The same method as described in Paper III is used. The HSRA model is used to compute the LTE populations. A distribution of NLTE-coeffi