๐”– Bobbio Scriptorium
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Some observations of solar radiation on wavelengths of 1.7 and 3.8 metres

โœ Scribed by Ryle, M.

Book ID
119741064
Publisher
Institution of Electrical Engineers
Year
1948
Weight
337 KB
Volume
95
Category
Article
ISSN
2054-0604

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๐Ÿ“œ SIMILAR VOLUMES

Radio interferometric observations of so
Radio interferometric observations of solar bursts at 3.7 and 11.1 cm wavelengths
โœ M. R. Kundu; P. E. Angerhofer ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 219 KB

Several solar active regions were observed during the 1976 vernal equinox with the 3-element interferometer of the National Radio Astronomy Observatory. The element spacings for these observations were 600, 2100, and 2700 m, resulting in maximum angular resolutions of about 3 arc sec at 3.7 cm and 8

Observations of the 7 March, 1970 total
Observations of the 7 March, 1970 total solar eclipse at wavelengths of 3.2 and 8.3 mm
โœ John P. Hagen; Paul N. Swanson; Robert W. Haas; Fred L. Wefer; Raymond W. Vogt ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 992 KB

The 7 March, 1970 total solar eclipse was observed at wavelengths of 3.2 and 8.3 mm; the object being to use the knife edge of the Moon as it passed across the Sun to improve angular resolution on the Sun. This in turn would provide a radial brightness distribution of the Sun with an angular resolut

Fine structure of a solar active region
Fine structure of a solar active region at 3.7 and 11.1 cm wavelengths
โœ M. R. Kundu; R. H. Becker; T. Velusamy ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 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

Fine structure of a solar flare region a
Fine structure of a solar flare region at 3.7 and 11.1 cm wavelengths
โœ M. R. Kundu; T. Velusamy; R. H. Becker ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 273 KB

On June 9, 1973, a flare associated burst was observed with the NRAO 3-element interferometer at 3.7 and 11.1 cm wavelength. The burst was of 'gradual rise and fall' type. Comparing the fringe amplitudes at 3.7 cm to the visibility computed for model flare regions we found that the precursor data ar