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Influence of temperature distribution in the chromosphere on the spectrum of the S-component of solar radio emission

✍ Scribed by M. N. Fasakhova; O. I. Yudin


Book ID
112466096
Publisher
Springer US
Year
1974
Tongue
English
Weight
161 KB
Volume
17
Category
Article
ISSN
0033-8443

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Fine structure of the S-component spectr
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Fine structure observations of the frequency spectrum of the S-component in the solar radio emission are described. Measurements were carried out in August 1976 and August 1977 using a 22 m parabolic antenna and a radiospectrograph operating over the frequency range 5.0 to 7.0 GHz, with the resoluti