Direct numerical simulations of the transition between rotation- to buoyancy-dominated regimes in rotating Rayleigh–Bénard convection-Reference-Cited by-同舟云学术

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Direct numerical simulations of the transition between rotation- to buoyancy-dominated regimes in rotating Rayleigh–Bénard convection

Published:2024-11 Issue: Volume:232 Page:125971
ISSN:0017-9310
Container-title:International Journal of Heat and Mass Transfer
language:en
Short-container-title:International Journal of Heat and Mass Transfer

Author:

Song Jiaxing^ORCID,Kannan Veeraraghavan^ORCID,Shishkina Olga^ORCID,Zhu Xiaojue^ORCID

Publisher

Elsevier BV

Reference88 articles.

1. Laboratory simulation of thermal convection in rotating planets and stars;Busse;Science,1976

2. Turbulent convection at very high Rayleigh numbers;Niemela;Nature,2000

3. Heat transfer and large scale dynamics in turbulent Rayleigh–Bénard convection;Ahlers;Rev. Modern Phys.,2009

4. Rotating convective turbulence in Earth and planetary cores;Aurnou;Phys. Earth Planet. Inter.,2015

5. Turbulent convective length scale in planetary cores;Guervilly;Nature,2019

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