Hostname: page-component-84b7d79bbc-tsvsl Total loading time: 0 Render date: 2024-07-31T14:50:31.728Z Has data issue: false hasContentIssue false
  • English
  • Français

The Magnetic Fields at Different Levels in the Active Regions of the Solar Atmosphere

Published online by Cambridge University Press:  14 August 2015

T. T. Tsap
T. T. Tsap*
Affiliation:
Crimean Astrophysical Observatory, Nauchny, Crimea, 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.

The strengths of the longitudinal magnetic fields recorded at different depths of active regions with a double magnetograph of the Crimean Astrophysical Observatory are compared.

The recordings of the magnetic fields were made in the lines Fe Iλ5250Å, Ca Iλ6103Å, Na I D1, BIIλ4554Å, Mg Iλ5184Å, Hα, Hγ, Hδ.

It is shown, that there is a close correlation between the longitudinal magnetic field at different levels.

Type
Part III: Observations of Sunspot and Active Region Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 223 - 230
Copyright
Copyright © Reidel 1971 

References

Severny, A. B.: 1966, Astron. Zh. 43, 465.Google Scholar