Skip to main content
SpringerLink
Log in

Photoelectric measurement of the coronal emission line λ 5303 by an automatic coronal photometer

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

Abstract

A 5303 Å-photometer was constructed for the 20 cm coronagraph of the Wendelstein solar observatory. Details of the photometer, the method of measurement and an example for measured isophotes are given. The Wendelstein photometer is compared with the 5303 Å-Sac Peak photometer.

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

  • Fisher, R. R.: 1974, Solar Phys. 36, 343.

    Google Scholar 

  • Hügel, R.: 1975, Thesis, München.

  • Solar-Geophysical Data: 1976, Prompt Reports, No. 388, Part I.

  • Spannagl, C.: 1977, Thesis, München.

Download references

Author information

Authors and Affiliations

  1. Universitäts-Sternwarte, Scheinerstraβe 1, D-8000, 80, München, FRG

    Christian Spannagl

Authors
  1. Christian Spannagl
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

Mitteilungen der Sternwarte München Bd. 2 Nr. 5.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Spannagl, C. Photoelectric measurement of the coronal emission line λ 5303 by an automatic coronal photometer. Sol Phys 58, 319–321 (1978). https://doi.org/10.1007/BF00157277

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00157277

Keywords

Search

Navigation