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On the temperature distribution in the solar corona

โœ Scribed by H. P. Mital; Udit Narain

Publisher
Springer
Year
1978
Tongue
English
Weight
145 KB
Volume
56
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

An improved value of coronal temperature is obtained by the degree of ionization method taking various processes into consideration. Comparison with some of the existing results has also been made.

The problem of establishing the temperature distribution in solar corona has been of interest to many workers in this field, since long. It has generally been dealt with in two ways, namely Doppler broadening method of spectral lines

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