Metamorphosis of marginal thermal convection in rapidly rotating self-gravitating spherical shells

1994 ◽  
Vol 74 (1-4) ◽  
pp. 143-179 ◽  
Author(s):  
Wolfram R. Hirsching ◽  
Jun-Ichi Yano
Author(s):  
Mrs. Birgit Futterer ◽  
Dr. Marcus Gellert ◽  
Mr. Thomas von Larcher ◽  
Mr. Christoph Egbers

2017 ◽  
Vol 13 (S337) ◽  
pp. 336-337
Author(s):  
Ferran Garcia ◽  
Frank R. N. Chambers ◽  
Anna L. Watts

AbstractIn this study the onset of stress-free Boussinesq thermal convection in rotating spherical shells with aspect ratio η = rinner/router = 0.9, Prandtl numbers Pr ∈ [10−4, 10−1], and Taylor numbers Ta ∈ [104, 1012] is considered. We focus on the form of the convective cell pattern that develops, and on its time scales, since this may have observational consequences for thermonuclear burning and the development of burst oscillations in the exploding oceans of accreting neutron stars (Watts (2012)).


2008 ◽  
Vol 62 (4-5) ◽  
pp. 300-307 ◽  
Author(s):  
B. Futterer ◽  
M. Gellert ◽  
Th. von Larcher ◽  
C. Egbers

1983 ◽  
Vol 23 (1) ◽  
pp. 1-42 ◽  
Author(s):  
Abdelfattah Zebib ◽  
Gerald Schubert ◽  
James L. Dein ◽  
Ramesh C. Paliwal

2010 ◽  
Vol 229 (20) ◽  
pp. 7997-8010 ◽  
Author(s):  
F. Garcia ◽  
M. Net ◽  
B. García-Archilla ◽  
J. Sánchez

2004 ◽  
Vol 501 ◽  
pp. 43-70 ◽  
Author(s):  
E. DORMY ◽  
A. M. SOWARD ◽  
C. A. JONES ◽  
D. JAULT ◽  
P. CARDIN

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