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Improved solar coronal temperature for equal green and red line intensities

โœ Scribed by Udit Narain; Suresh Chandra


Publisher
Springer
Year
1976
Tongue
English
Weight
109 KB
Volume
47
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


An improved value of the temperature in the solar corona for equal green and red line intensities is obtained. This temperature is in better agreement with a quoted line-width value than the previous theoretical ones.

Recently Chandra and Narain (1976) presented an improved relation for the green-to-red line intensity ratio of Fe ions. Their relation is


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