𝔖 Bobbio Scriptorium
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Observed and theoretical profiles of the Siiilines at λ1814

✍ Scribed by G. D. Finn; H. C. McAllister


Publisher
Springer
Year
1978
Tongue
English
Weight
546 KB
Volume
56
Category
Article
ISSN
0038-0938

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✦ Synopsis


Emission line spectra observed at the limb of the solar disc are presented for transitions of singly ionized silicon at ,~&1816.93, 1817.45 and 1808.01. The profiles show self-reversals in the line cores. A non-LTE analysis for a simplified model of the silicon ion is presented and calculated line profiles are compared with the observations. The study indicates that some modification of the Vernazza et al, (1973) model of the solar chromosphere in the transition region is needed to reconcile the calculated and observed profiles.


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