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Observations on the slowly varying component of solar radio emission at decameter wavelengths

โœ Scribed by Ch. V. Sastry; R. K. Shevgaonkar; M. N. Ramanuja

Publisher
Springer
Year
1983
Tongue
English
Weight
491 KB
Volume
87
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

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

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