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Theoretical line intensities from MgVI,SiVIII, and SX coronal ions |
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| Authors: | B N Dwivedi |
| Institution: | (1) Department of Applied Physics, Banaras Hindu University, Varanasi, India |
| Abstract: | Emission line intensities from MgVI, SiVIII, andSX ions of nitrogen sequence have been computed by use of the model atmosphere of Kopp and Orrall (1976) for the quiet Sun and coronal holes and compared with observational data available from rocket and satellite. |
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