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)


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.




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  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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