Hostname: page-component-6bf8c574d5-gr6zb Total loading time: 0 Render date: 2025-02-22T22:01:59.521Z Has data issue: false hasContentIssue false
  • English
  • Français

On the contribution of solar activity to the ultraviolet spectrum of the Sun

Published online by Cambridge University Press:  14 August 2015

A. V. Bruns ,
V. K. Prokofiev  and
A. B. Severny
A. V. Bruns
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.
V. K. Prokofiev
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.
A. B. Severny
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.

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.

As measured from space, the contribution of one moderate flare to the emission spectrum of the Sun in the far-ultraviolet (304 Å, Lyman continuum, etc.) is comparable with the emission of the whole undisturbed solar disc.

Type
Part II: Stellar Line Spectra
Information
Symposium - International Astronomical Union , Volume 36: Ultraviolet Stellar Spectra and Related Ground-Based Observations , 1970 , pp. 256 - 259
Copyright
Copyright © Reidel 1970 

References

Bruns, A. V., Prokofiev, V. K., and Severny, A. B.: 1968, XI COSPAR, Tokyo, May.Google Scholar
Hall, L. A. and Hinteregger, H. E.: 1968, XI COSPAR, Tokyo, May.Google Scholar