Skip to main content
SpringerLink
Log in

On the influence of seeing on photospheric velocity measurements

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

It is shown that the short-period fluctuations of photospheric velocity records can be explained by the scanning effect of atmospheric seeing (image motion) and the velocity gradients present on the solar surface. Some observations supporting this explanation are presented.

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

  • Deubner, F. L.: 1966, in The Fine Structure of the Solar Atmosphere (ed. by K.O. Kiepenheuer), Steiner, Wiesbaden, p. 26.

    Google Scholar 

  • Howard, R.: 1967, Solar Phys. 2, 3.

    Google Scholar 

  • Howard, R. and Livingston, W. C.: 1968, Solar Phys. 3, 439.

    Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Fraunhofer Institut, Freiburg, Germany

    Franz Ludwig Deubner

Authors
  1. Franz Ludwig Deubner
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

Mitteilungen aus dem Fraunhofer Institut Nr. 76.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Deubner, F.L. On the influence of seeing on photospheric velocity measurements. Sol Phys 3, 439–447 (1968). https://doi.org/10.1007/BF00171616

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00171616

Keywords

Search

Navigation