TURBULENT CROSS-HELICITY IN THE MEAN-FIELD SOLAR DYNAMO PROBLEM
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/743/i=2/a=160/pdf
Reference47 articles.
1. Solar internal rotation rate and the latitudinal variation of the tachocline
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5. Parity properties of an advection-dominated solar $\mathsf{\alpha^2 \Omega}$-dy na mo
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1. Advances in mean-field dynamo theory and applications to astrophysical turbulence;Journal of Plasma Physics;2018-08
2. Solar Kinetic Energy and Cross Helicity Spectra;The Astrophysical Journal;2018-07-31
3. Generation of a Large-scale Magnetic Field in a Convective Full-sphere Cross-helicity Dynamo;The Astrophysical Journal;2018-05-17
4. A NEW SIMPLE DYNAMO MODEL FOR STELLAR ACTIVITY CYCLE;The Astrophysical Journal;2016-06-14
5. EFFECTS OF ANISOTROPIES IN TURBULENT MAGNETIC DIFFUSION IN MEAN-FIELD SOLAR DYNAMO MODELS;The Astrophysical Journal;2014-03-25
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