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A Self-Consistent Model Atmosphere Program with Applications to Solar 0I Resonance Lines
Published online by Cambridge University Press: 08 February 2017
Abstract
Profiles and total intensities are computed for solar 01 resonance lines at λ1302 and λ1305 using a model atmosphere program that includes non-LTE effects in both hydrogen and oxygen and that includes microturbulence both as a line broadening mechanism and as a contribution to the gas pressure. Good agreement is obtained between computed and observed intensities. The computed profiles appear to have too much 'self-reversal.
- Type
- Part A. Type of Problems that Exist
- Information
- International Astronomical Union Colloquium , Volume 2: Spectrum Formation in Stars With Steady-State Extended Atmospheres , August 1970 , pp. 65 - 84
- Copyright
- Copyright © 1970
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