Evolution and characteristics of forced shear flows in polytropic atmospheres: large and small Péclet number regimes-Reference-Cited by-同舟云学术

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Evolution and characteristics of forced shear flows in polytropic atmospheres: large and small Péclet number regimes

Published:2018-10-05 Issue:1 Volume:482 Page:1338-1351
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Witzke V¹²^ORCID,Silvers L J¹,Favier B³

Affiliation:

1. Department of Mathematics, City, University of London, Northampton Square, London EC1V 0HB, UK

2. Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany

3. Aix-Marseille Université, CNRS, Ecole Centrale Marseille, IRPHE UMR 7342, 49 rue F. Joliot-Curie, F-13013 Marseille, France

Funder

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/1/1338/26278958/sty2698.pdf

Reference39 articles.

1. An Introduction to Atmospheric Physics

2. The radial gradient of the near-surface shear layer of the Sun

3. The Case for a Distributed Solar Dynamo Shaped by Near‐Surface Shear

4. An update of Leighton’s solar dynamo model

5. Helioseismic Constraints on the Structure of the Solar Tachocline

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