Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-02T20:42:14.371Z Has data issue: false hasContentIssue false
  • English
  • Français

Forbidden Line Excitation Data for Certain Coronal Lines

Published online by Cambridge University Press:  25 May 2016

S. J. Czyzak ,
L. H. Aller  and
R. N. Euwema
S. J. Czyzak
Affiliation:
Astronomy Dept., The Ohio State University, Columbus, Ohio, U.S.A.
L. H. Aller
Affiliation:
Astronomy Dept., University of California, Los Angeles, Calif., U.S.A.
R. N. Euwema
Affiliation:
Aerospce Research Laboratories, Wright Patterson Air Force Base, Ohio, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Plasma diagnostics of the active corona require data on transition probabilities and collision cross sections for relevant coronal emission lines. Atomic parameters pertaining to a number of coronal transitions have been derived as follows:

Type
Part II The Flash Phase of Solar Flares
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 155
Copyright
Copyright © Reidel 1974