The radio brightness distribution at 29 mm, 23.5 mm and 21.2 mm is calculated employing a statistical technique to account for the presence of spicules randomly occurring along the ray path. The results indicate limb brightening at each wavelength when the Avery and House (1969) spicule model is emp
Solar limb brightening at 3.1 cm
โ Scribed by M. Felli; G. Tofani
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 195 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0038-0938
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