HIGH-RESOLUTION CALCULATIONS OF THE SOLAR GLOBAL CONVECTION WITH THE REDUCED SPEED OF SOUND TECHNIQUE. I. THE STRUCTURE OF THE CONVECTION AND THE MAGNETIC FIELD WITHOUT THE ROTATION-Reference-Cited by-同舟云学术

HIGH-RESOLUTION CALCULATIONS OF THE SOLAR GLOBAL CONVECTION WITH THE REDUCED SPEED OF SOUND TECHNIQUE. I. THE STRUCTURE OF THE CONVECTION AND THE MAGNETIC FIELD WITHOUT THE ROTATION

Published:2014-04-11 Issue:1 Volume:786 Page:24
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Hotta H.,Rempel M.,Yokoyama T.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/786/i=1/a=24/pdf

Reference44 articles.

1. Modeling the Near-Surface Shear Layer: Diffusion Schemes Studied With CSS

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3. NONLINEAR SMALL-SCALE DYNAMOS AT LOW MAGNETIC PRANDTL NUMBERS

4. Magnetic structures in a dynamo simulation

5. Dynamo Action in the Solar Convection Zone and Tachocline: Pumping and Organization of Toroidal Fields

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