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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

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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

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