Separate regime transitions for heat and momentum transport in laboratory-numerical models of planetary core convection
Emily Kate Hawkins1, Jonathan Shuo Cheng2, Timothy Pilegard3, Stephan Stellmach4 and Jonathan M Aurnou1, (1)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (2)Eindhoven University of Technology, Department of Applied Physics and J.M. Burgers Center for Fluid Dynamics, Eindhoven, Netherlands, (3)L3 OceanServer Technology, Imperial Beach, CA, United States, (4)University of Münster, Institute for Geophysics, Münster, Germany
