Possible Global Magneto-Fluid Structure of the Stellar Convection Zone
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/58/3/605/9714401/pasj58-0605.pdf
Reference35 articles.
1. Differential rotation and star-spot evolution on HK Aqr in 2001 and 2002
2. Mean Magnetic Field Generation in Sheared Rotators
3. A Vorticity–Magnetic Field Dynamo Instability
4. Convection driven zonal flows and vortices in the major planets
5. Dynamical variations of the differential rotation in the solar convection zone
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