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Temperature Diagnostics of the Upper Photosphere

Published online by Cambridge University Press:  08 February 2017

N. G. Shchukina ,
T. G. Shcherbina  and
R. J. Rutten
N. G. Shchukina
Affiliation:
1Main Astronomical Observatory, Academy of Sciences of the Ukrainian SSR, 252127 Kiev, USSR
T. G. Shcherbina
Affiliation:
1Main Astronomical Observatory, Academy of Sciences of the Ukrainian SSR, 252127 Kiev, USSR
R. J. Rutten
Affiliation:
2Sterrekundig Instituut, Postbus 80000, 3508 TA Utrecht, The Netherlands

Abstract

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We use NLTE modelling of the alkali resonance lines and of C I and 0 I high-excitation multiplets to test their quality as temperature diagnostics of the upper photosphere, in the context of Avrett's NLTE recovery of the LTE Holweger-Müller model below the temperature minimum and Ayres' bifurcation into hot and cool components above the temperature minimum.

Type
I. Global Properties of the Photosphere
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 29 - 34
Copyright
Copyright © Kluwer 1990 

References

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