Skip to main content
Log in

On temperature in line-gap regions

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

The small regions in the photosphere where many absorption lines weaken have been investigated by several authors. Sheeley attempted to explain the weakening of neutral lines in terms of a temperature increase on the basis of a simple theoretical model. It is shown that this model is not applicable but that a modified theory is able to interpret the observed behaviour of both neutral and ionized lines in terms of a temperature increase of a few percent.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Additional information

Mitteilungen aus dem Fraunhofer Institut, Nr. 98.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Grossmann-Doerth, U. On temperature in line-gap regions. Sol Phys 13, 287–291 (1970). https://doi.org/10.1007/BF00153549

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00153549

Keywords

Navigation