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Solar XUV limb brightening observations

โœ Scribed by George L. Withbroe


Publisher
Springer
Year
1970
Tongue
English
Weight
590 KB
Volume
11
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


Limb brightening of XUV lines of the ions Cm Nm, Niv, Ore, Oiv, Ov and Silv is compared with that predicted by a modified version of a coronal model developed by Dupree and Goldberg. Systematic differences between the predicted and observed limb brightening are found. These differences can be eliminated by introducing into the model the effects of spicules that extend up into the chromospheric-coronal transition region. The spicules are assumed to be opaque to radiation between 500 and 900A. because of absorption in the hydrogen Lyman continuum.


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