Stagnant lid convection in bottom‐heated thin 3‐D spherical shells: Influence of curvature and implications for dwarf planets and icy moons - Yao - 2014 - Journal of Geophysical Research: Planets - Wiley Online Library
Department of Physical and Environmental Sciences, University of Toronto, Scarborough, Toronto, Ontario, Canada C. Sanchez-Valle Department of Earth Sciences, Swiss Federal Institute of Technology Zurich, Zurich, Switzerland P. J. Tackley Department of Earth Sciences, Swiss Federal Institute of Technology Zurich, Zurich, Switzerland Corresponding Author C. Yao Department of Earth Sciences, Swiss Federal Institute of Technology Zurich, Zurich, Switzerland Correspondence to: C. Yao, chloe.yao@erdw.ethz.ch F. Deschamps Institute of Earth Sciences, Academia Sinica, Taipei, Taiwan J. P. Lowman Department of Physical and Environmental Sciences, University of Toronto, Scarborough, Toronto, Ontario, Canada C. Sanchez-Valle Department of Earth Sciences, Swiss Federal Institute of Technology Zurich, Zurich, Switzerland P. J. Tackley Department of Earth Sciences, Swiss Federal Institute of Technology Zurich, Zurich, Switzerland Give access Share full-text access Use the link below to share a full
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