Rotating convective turbulence in Earth and planetary cores-Reference-Cited by-同舟云学术

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Rotating convective turbulence in Earth and planetary cores

Published:2015-09 Issue: Volume:246 Page:52-71
ISSN:0031-9201
Container-title:Physics of the Earth and Planetary Interiors
language:en
Short-container-title:Physics of the Earth and Planetary Interiors

Author:

Aurnou J.M.,Calkins M.A.,Cheng J.S.,Julien K.,King E.M.,Nieves D.,Soderlund K.M.,Stellmach S.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Physics and Astronomy (miscellaneous),Geophysics,Astronomy and Astrophysics

Reference130 articles.

1. The Boussinesq and anelastic liquid approximations for convection in the Earths core;Anufriev;Phys. Earth Planet. Inter.,2005

2. Quasigeostrophic models of convection in rotating spherical shells;Aubert;Geochem. Geophys. Geosys.,2003

3. The magnetic structure of convection-driven numerical dynamos;Aubert;Geophys. J. Int.,2008

4. Bottom-up control of geomagnetic secular variation by the Earth’s inner core;Aubert;Nature,2013

5. Experiments on convection in Earth’s core tangent cylinder;Aurnou;Earth Planet. Sci. Lett.,2003

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2. Shadowgraph Measurements of Rotating Convective Planetary Core‐Style Flows;Journal of Geophysical Research: Planets;2024-09

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4. Direct numerical simulations of rapidly rotating Rayleigh–Bénard convection with Rayleigh number up to;Journal of Fluid Mechanics;2024-06-25

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