Spherical geometry convection in a fluid with an Arrhenius thermal viscosity dependence: The impact of core size and surface temperature on the scaling of stagnant-lid thickness and internal temperature-Reference-Cited by-同舟云学术

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Spherical geometry convection in a fluid with an Arrhenius thermal viscosity dependence: The impact of core size and surface temperature on the scaling of stagnant-lid thickness and internal temperature

Published:2024-04 Issue: Volume:349 Page:107157
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:

Javaheri Pejvak,Lowman Julian P.,Tackley Paul J.

Funder

Natural Sciences and Engineering Research Council of Canada

Publisher

Elsevier BV

Reference54 articles.

1. High-contrast, high-angular resolution view of the GJ 367 exoplanet system;Brandner;Mon. Not. R. Astron. Soc.,2022

2. Geodynamic diagnostics, scientific visualisation and staglab 3.0;Crameri;Geosci. Model Dev.,2018

3. Scientific Colour Maps;Crameri,2023

4. The misuse of colour in science communication;Crameri;Nat. Commun.,2020

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

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