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Correlated brightness variations in solar radiative output from the photosphere to the corona

✍ Scribed by Lean, J. L.; Mariska, J. T.; Strong, K. T.; Hudson, H. S.; Acton, L. W.; Rottman, G. J.; Woods, T. N.; Willson, R. C.


Book ID
119692681
Publisher
American Geophysical Union
Year
1995
Tongue
English
Weight
443 KB
Volume
22
Category
Article
ISSN
1944-8007

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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