Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-23T06:52:44.385Z Has data issue: false hasContentIssue false
  • English
  • Français

Detection Possibility of the Giant Rolls in the Sun

Published online by Cambridge University Press:  12 April 2016

Tünde Baranyi  and
András Ludmány
Tünde Baranyi
Affiliation:
Heliophysical Observatory of the Hungarian Academy of Sciences, H-4010 Debrecen, P.O.Box 30., Hungary
András Ludmány
Affiliation:
Heliophysical Observatory of the Hungarian Academy of Sciences, H-4010 Debrecen, P.O.Box 30., Hungary

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.

The expected giant convection pattern has been studied by using its probable twisting influence on the emerging magnetic fields. The studies carried out on extended computations and material have confirmed the previously found evidence for a pattern with longitudinal wavenumber 1=11 in the year 1977.

Type
I. Setting the stage: Sun, Stars Galaxies and the Universe
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 81 - 83
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Baranyi, T. and Ludmány, A. 1992, Solar Phys., in press.Google Scholar
Dezső, L., Kovács, .Á and Gerlei, O. 1987, Debrecen Photoheliographic Results 1977, Publ. Debrecen Obs., Heliographie Series No.1.Google Scholar
Gilman, P.A. and Miller, J. 1986, Astrophys.J.Suppl. 61, 585.Google Scholar
Glatzmaier, G. 1984, J.Comp.Phys. 55, 461.Google Scholar