Skip to main content
SpringerLink
Log in

On green-to-red line intensity ratio in the solar corona

  • Research Notes
  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

An improved formula for the green-to-red line intensity ratio in the solar corona is proposed. The results are compared with those given by the previous expression.

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

Access this article

Log in via an institution

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

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  • Narain, U. and Chandra, S.: 1975, Astrophys. J. 200, 234.

    Google Scholar 

  • Schwartz, S. B.: 1959, Ph.D. Thesis, University of Colorado.

  • Schwartz, S. B. and Zirin, H.: 1959, Astrophys. J. 130, 384.

    Google Scholar 

  • Zirker, J. B.: 1970, Solar Phys. 11, 68.

    Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Atomic and Molecular Physics Research Group, Physics Department, Meerut College, 250001, Meerut, India

    S. Chandra & U. Narain

Authors
  1. S. Chandra
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. U. Narain
    View author publications

    You can also search for this author in PubMed Google Scholar

Rights and permissions

Reprints and permissions

About this article

Cite this article

Chandra, S., Narain, U. On green-to-red line intensity ratio in the solar corona. Sol Phys 46, 183–184 (1976). https://doi.org/10.1007/BF00157565

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00157565

Keywords

Search

Navigation