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 elimin
Solar XUV limb brightening observations
โ Scribed by George L. Withbroe
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 727 KB
- Volume
- 11
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 the model. The sensitivity of the predicted limb-brightening curves to changes in parameters describing the model is discussed. Coronal abundances for N, O, Ne, Mg, and Si are obtained.
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