Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-13T01:03:16.621Z Has data issue: false hasContentIssue false
  • English
  • Français

Density Diagnostics of Solar Emission Lines from the Nitrogen-like Mg VI Ion

Published online by Cambridge University Press:  19 July 2016

P.K. Raju  and
R. Vasundhara
P.K. Raju
Affiliation:
Indian Institute of Astrophysics Bangalore-560034, India
R. Vasundhara
Affiliation:
Indian Institute of Astrophysics Bangalore-560034, India

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.

The variation of theoretical line intensity ratios with electron density for Mg VI ion are presented. This study indicates that the line intensity ratios for Mg VI can be used to infer electron density for solar plasma.

Type
VIII. Solar Flares
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 443 - 444
Copyright
Copyright © Kluwer 1990 

References

Dwivedi, B.N. and Raju, P.K. (1988) ‘Density diagnostics of solar emission lines from introgen-like ions’, Adv. Space Res. 8, 11 (179)–11 (183).CrossRefGoogle Scholar