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Line-of-Sight Velocity Field of Synodic Solar Rotation

  • A. Kubičela
  • M. Karabin
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 96)

Abstract

Angular velocity of synodic solar rotation have been treated as vectors. A colinear and a perpendicular components with respect to the solar rotation axis have been found. Consequently, factor cos 7 . O 25 has been introduced into the apparent effect of the Earth’s orbital motion. An alternating term has been also added in the expression of the synodic line-of-sight velocity of an arbitrary photospheric point.

Keywords

Angular Velocity Solar Disk Solar Rotation Solar Equator Peripheral Velocity 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Beckers, J.M.: 1978, Osservatorio Astrofis. Catania, Pub1. 162, pp. 166–177.Google Scholar
  2. Kubičela, A.: 1982, Hvar Obs. Bull. Suppl., 1. in press.Google Scholar
  3. KubiEela, A. and Karabin, M.: 1977, Solar Phys. 54, pp.5O5–5O9.ADSCrossRefGoogle Scholar

Copyright information

© D. Reidel Publishing Company 1982

Authors and Affiliations

  • A. Kubičela
    • 1
  • M. Karabin
    • 2
  1. 1.Astronomical ObservatoryBelgradeYugoslavia
  2. 2.Institute of AstronomyFaculty of SciencesBelgradeYugoslavia

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