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The spectrum of the slowly varying component of solar radio emission at wavelengths of 3.3 mm – 21 cm

✍ Scribed by A. Tlamicha

Publisher
Springer
Year
1968
Tongue
English
Weight
190 KB
Volume
5
Category
Article
ISSN
0038-0938

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✦ Synopsis

The spectrum and diameter of the source of the S-component emission (McMath Plage No. 244) observed on March 4, 1968 has been investigated at 3.3 ram, 4.3 ram, 8.5 mm, 2 cm, 9.1 cm, 21 cm, and 43 cm wavelengths.

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