OSO-IV observations of the equatorial limb brightening of XUV resonance lines of Nv, O w, Ne vii, Mg x and Si xii are interpreted with a modified version of a coronal model developed by Dupree and Goldberg (1967). Good agreement is obtained between the observed limb brightening and that predicted by
Solar XUV limb brightening observations
โ 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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โฆ 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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