Stagnant lid convection in bottom-heated thin 3-D spherical shells: Influence of curvature and implications for dwarf planets and icy moons-Reference-Cited by-同舟云学术

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Stagnant lid convection in bottom-heated thin 3-D spherical shells: Influence of curvature and implications for dwarf planets and icy moons

Published:2014-08 Issue:8 Volume:119 Page:1895-1913
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Yao C.¹,Deschamps F.²,Lowman J. P.³,Sanchez-Valle C.¹,Tackley P. J.¹

Affiliation:

1. Department of Earth Sciences; Swiss Federal Institute of Technology Zurich; Zurich Switzerland

2. Institute of Earth Sciences; Academia Sinica; Taipei Taiwan

3. Department of Physical and Environmental Sciences; University of Toronto, Scarborough; Toronto Ontario Canada

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference32 articles.

1. Thermodynamic properties and thermal equations of the state of high-pressure ice phases;Chizhov;J. Appl. Mech. Tech. Phys.,1993

2. Heat transport by variable viscosity convection and implications for the Earth's thermal evolution;Christensen;Phys. Earth Planet. Inter.,1984

3. Transient high-Rayleigh-number thermal-convection with large viscosity variations;Davaille;J. Fluid Mech.,1993

4. Stagnant lid convection in 3D-Cartesian geometry: Scaling laws and applications to icy moons and dwarf planets;Deschamps;Phys. Earth Planet. Inter.,2014

5. Inversion of two-dimensional numerical convection experiments for a fluid with a strongly temperature-dependent viscosity;Deschamps;Geophys. J. Int.,2000

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4. Did the cessation of convection in Mercury's mantle allow for a dynamo supporting increase in heat loss from its core?;Earth and Planetary Science Letters;2021-10

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