✦ LIBER ✦

Solar limb brightening at millimeter wavelengths

✍ Scribed by P. M. Kalaghan

Publisher: Springer
Year: 1974
Tongue: English
Weight: 397 KB
Volume: 39
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00162424

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✦ Synopsis

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 employed. This contradicts the results of Lantos and Kundu (1972) whose method of computation is shown to be inadequate.

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