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Ambiguity of the Solar Meridional Flow

Published online by Cambridge University Press:  27 November 2018

Vincent G. A. Böning Open the ORCID record for Vincent G. A. Böning [Opens in a new window]
Vincent G. A. Böning*
Affiliation:
Max-Planck-Institut für Sonnensystemforschung Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany email: boening@mps.mpg.de Kiepenheuer-Institut für Sonnenphysik Schöneckstr. 6, 79104 Freiburg, Germany
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Abstract

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Recent helioseismic estimates of the deep solar meridional flow have been contradictory. Using two years worth of GONG data, I show here that the detection of the meridional flow is ambiguous below about 0.85 solar radii.

Keywords

Sunhelioseismologymeridional flow
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 13 - 14
Copyright
Copyright © International Astronomical Union 2018 

References

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