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Center-to-limb variation of low-frequency Ca II line brightness oscillations in the solar chromosphere

✍ Scribed by Ozhogina, O. A.; Teplitskaya, R. B.

Book ID
125394679
Publisher
Springer
Year
2014
Tongue
English
Weight
686 KB
Volume
40
Category
Article
ISSN
1063-7737

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Existing models of the solar atmosphere predict a limb brightening in the far infrared wavelengths. At shorter wavelengths this effect is confined to the extreme limb but at 25 a it extends inward from the limb to cos 0 = 0.3. Observations of I(a)/I(1.0) were made with the McMath Solar Telescope thr