Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-30T00:49:47.987Z Has data issue: false hasContentIssue false
  • English
  • Français

Variations in the mean line of sight velocity of the Sun: 1976–1985

Published online by Cambridge University Press:  03 August 2017

A. Jiménez ,
P.L. Pallé ,
C. Régulo ,
T. Roca Cortés ,
Y.P. Elsworth ,
G.R. Isaak ,
S.M. Jefferies ,
C.P. McLeod ,
R. New  and
H.B. van der Raay
A. Jiménez
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
P.L. Pallé
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
C. Régulo
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
T. Roca Cortés
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de La Laguna, Tenerife, Spain
Y.P. Elsworth
Affiliation:
Department of Physics, University of Birmingham, U.K.
G.R. Isaak
Affiliation:
Department of Physics, University of Birmingham, U.K.
S.M. Jefferies
Affiliation:
Department of Physics, University of Birmingham, U.K.
C.P. McLeod
Affiliation:
Department of Physics, University of Birmingham, U.K.
R. New
Affiliation:
Department of Physics, University of Birmingham, U.K.
H.B. van der Raay
Affiliation:
Department of Physics, University of Birmingham, U.K.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Measurements of the line of sight velocity of the sun with respect to earth have been obtained at Izaña (Tenerife) during the years 1976 to 1985. The mean values found for each year show a trend of ~30 m/s from minimum to maximum. Their mean value is of 583.1 ± .2 m/s which is 92% of the gravitational red shift predicted by theory and their variation seems to be related to the solar cycle with the clear exception of 1985. The most likely interpretation is that the velocity limb shift effect, averaged over the whole sun, is the cause of the slight disagreement with theory and this effect changes with time.

Type
Chapter 3: Longterm Variations in the Sun
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 215 - 218
Copyright
Copyright © Reidel 1988 

References

Beckers, J.M., Nelson, G.D.: 1978. Sol. Phys., 58, 243 Google Scholar
Brookes, J.R., Issak, G.R., van der Raay, H.B.: 1978. MNRAS, 185, 1 CrossRefGoogle Scholar
Claverie, A., Isaak, G.R., Mc Leod, C.P., van der Raay, H.B., Pallé, P.L., Roca Cortés, T.: 1982. Nature, 299, 709 Google Scholar