Hostname: page-component-848d4c4894-2pzkn Total loading time: 0 Render date: 2024-05-06T13:06:59.408Z Has data issue: false hasContentIssue false
  • English
  • Français

Solar Ca II K Resonance Line Polarization

Published online by Cambridge University Press:  25 April 2016

D. E. Rees  and
G. J. Saliba
D. E. Rees
Affiliation:
Department of Applied Mathematics, University of Sydney
G. J. Saliba
Affiliation:
Department of Applied Mathematics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

The Ca II K line serves as an important tool in determining the physics of the photosphere-chromosphere region of the solar atmosphere (Cram 1983). To date detailed analyses have centred on the study of line intensity profiles.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 186 - 188
Copyright
Copyright © Astronomical Society of Australia 1983

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Auer, L. H., Rees, D. E., and Stenflo, J. O., Astron. Astrophys., 88, 302 (1980).Google Scholar
Cram, L. E., Proc. Astron. Soc. Aust., 5, (1983).Google Scholar
Gingerich, O., Noyes, R. W., and Kalkofen, W., Solar Phys., 18, 347 (1971).Google Scholar
Rees, D. E., and Saliba, G. J., Astron. Astrophys., 115, 1 (1982).Google Scholar
Stenflo, J. O., Astron. Astrophys., 84, 68 (1980).Google Scholar
Vernazza, J. E., Avrett, E. H., and Loeser, R., Astrophys. J. Suppl. Ser., 45, 635 (1981).Google Scholar