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Solar radio emission at 1.2 mm wavelength

โœ Scribed by M. R. Kundu


Publisher
Springer
Year
1971
Tongue
English
Weight
416 KB
Volume
21
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Solar enhancements at 1.2 mm wavelength
โœ J. E. Beckman; C. D. Clark ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 868 KB

Solar observations through the atmospheric pass-band centred at 250 GHz have been made in the form of isophote maps. These show chromospheric features which have higher brightness temperatures than the mean disc temperature by up to 10 %. Examination of corresponding maps at lower frequencies and al

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The results are given of observation of solar radio emission of the S-component at 8.15 ram-2 and 2.25 ram-2 made with the 22 m radio telescope of the Crimean Astrophysical Observatory. Solar radio images are obtained at both wavelengths. The data are presented of radio emission intensity and bright

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Quasi-periodic solar emission has been observed with a radio spectrograph operating at 18-28 MHz during weak decametric continuum on August 22, 1972. The continuum activity was observed simultaneously on fixed frequency receivers at 18 MHz and at 26 MHz. The pulsations showed a mean period of 4 s an