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Polarization of solar active regions at 9.5 mm wavelength

โœ Scribed by M. R. Kundu; T. P. McCullough


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

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๐Ÿ“œ SIMILAR VOLUMES


Polarization of solar active regions at
โœ M. R. Kundu; T. Gergely ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 432 KB

A study of the circular polarization structure of solar active regions has been made from data obtained at 3.5 mm wavelength, using the 36 ft diameter radio telescope of the National Radio Astronomy Observatory at Kitt Peak, Arizona. The angular resolution of the telescope at this wavelength is 1:2.

Solar active regions at 9 and 3.5 mm wav
โœ M. R. Kundu; Sou-Yang Liu ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 374 KB

Some properties of solar active regions at 9 and 3.5 mm wavelengths under disturbed conditions are discussed. New regions develop or weak regions intensify at millimeter wavelengths as a result of flares at distant sites. The spectra of the peak flux density of moderately strong bursts observed at 9

Observations of a partial solar eclipse
โœ A. M. Flett; Patricia R. Foster; P. Strachan; D. C. Thornton ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 195 KB

Observations at 9 mm wavelength of the partial solar eclipse of February 25th 1971 were made to investigate possible limb brightening of the Sun. The results obtained show that less than 5 of the solar disc power can be contained in any such brightening.

Interferometer observations of the solar
โœ Ikuro Suzuki; Kin-Aki Kawabata; Hideo Ogawa ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 503 KB

The brightness distribution of the quiet Sun at 8.6 mm wavelength is synthesized from off-meridian observations using an eight element east-west interferometer with a maximum base line of 16.38 m (1913A). The observed brightness distribution is practically flat from the disk center to the optical li