Large Convective Events and Their Aftermath in a Rotating Star
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/486/i=2/a=1058/pdf
Reference21 articles.
1. Baker, N. H. 1987, in Physical Processes in Comets, Stars, and Active Galaxies, ed. W. Hillebrandt, E. Meyer-Hofmeister, & H.C. Thomas (Berlin: Springer), 105
2. Turbulent Compressible Convection with Rotation. I. Flow Structure and Evolution
3. Turbulent Convection: Old and New Models
4. Differential rotation and turbulent convection: A new Reynolds stress model and comparison with solar data
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1. Solar Modal Structure of the Engineering Environment;Proceedings of the IEEE;2007-05
2. Eigenoscillations of the differentially rotating Sun;Astronomy & Astrophysics;2002-03
3. Linearr‐Mode Oscillations in a Differentially Rotating Star;The Astrophysical Journal;1998-08
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