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Lunar Occupation of a Solar Active Region at 4 cm Wavelength

✍ Scribed by KUNDU, M. R.; VELUSAMY, T.

Book ID
109661229
Publisher
Nature Publishing Group
Year
1968
Tongue
English
Weight
207 KB
Volume
217
Category
Article
ISSN
0028-0836

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πŸ“œ SIMILAR VOLUMES

Fine structure of a solar active region
Fine structure of a solar active region at 3.7 and 11.1 cm wavelengths
✍ M. R. Kundu; R. H. Becker; T. Velusamy πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 698 KB

The three-element interferometer of the National Radio Astronomy Observatory was used to observe the Sun at 3.7 and 11.1 cm wavelengths during the period June 5-9, 1973. The baselines of the interferometer were 900, 1800 and 2700 meters, with maximum angular resolution of 3" at 3.7 and 9" at 11.1 cm

Polarization of solar active regions at
Polarization of solar active regions at 3.5 millimeter wavelength
✍ M. R. Kundu; T. Gergely πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 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.