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Slowly varying component spectrum of the solar radio emission at millimetre wavelengths

โœ Scribed by V. A. Efanov; A. G. Kislyakov; I. G. Moiseev

Publisher
Springer
Year
1972
Tongue
English
Weight
476 KB
Volume
24
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

Spectrum of slowly varying component of
Spectrum of slowly varying component of solar radio emission on millimeter wavelengths
โœ Atsushi Tsuchiya; Kozo Takahashi ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 146 KB

The spectrum of the S-component of solar radio emission has been investigated at 4 GHz, 17 GHz, 35 GHz, 70 GHz, and 94 GHz. The spectrum for a spot group which appeared late in March 1966 (McMath plage No. 8223), seems to be fiat at the frequencies above about 35 GHz. This implies that the emission

Observations and interpretation of the s
Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengths
โœ Ch. V. Sastry; K. S. Dwarkanath; R. K. Shevgaonkar; V. Krishan ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 517 KB

We have observed the slowly varying component of solar radio emission at a frequency of 34.5 MHz with half power beam widths of 26'/40' in the east-west and north-south directions, respectively. It is found that the observed brightness temperatures vary within the limits of 0.3x 106 K to 1.5 x 106 K