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
โฆ LIBER โฆ
Solar limb brightening and enhancement measurements at 1.2 mm
โ Scribed by R. A. Newstead
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 438 KB
- Volume
- 6
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Solar intensity measurements at a mean wavelength of 1.2 mm were made using a 1.6 m Cassegrain telescope. The measurements included a series of scans made during the partial solar eclipse of May 20th, 1966.
A high degree of solar limb brightening is inferred from the measured intensity distribution. The ratio of the disk-averaged brightness temperature to the central brightness temperature at 1.2 mm is calculated to be 1.11 4-0.02.
A fairly intense solar outburst, of approximate duration 50 rain, was observed towards the end of the eclipse.
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Solar enhancements at 1.2 mm wavelength
โ
J. E. Beckman; C. D. Clark
๐
Article
๐
1971
๐
Springer
๐
English
โ 868 KB