Image Details

Choose export citation format:

Effects of the Librationally Induced Flow in Mercury’s Fluid Core with an Outer Stably Stratified Layer

  • Authors: Fleur Seuren, Santiago A. Triana, Jérémy Rekier, Ankit Barik, Tim Van Hoolst

Fleur Seuren et al 2023 The Planetary Science Journal 4 .

  • Provider: AAS Journals

Caption: Figure 7.

Structure of the core flow in response to the m = 2 libration forcing for Ek = 10−9, with (left) the radial (u r ) and horizontal (﹩{({{u}_{\theta }}^{2}+{{u}_{\phi }}^{2})}^{1/2}﹩) as a function of the radial coordinate near the CMB and (right) the radial vorticity ﹩{\xi }_{r}=\hat{{\boldsymbol{r}}}\,\cdot \,{\boldsymbol{\nabla }}\times u﹩ at the (local) maximum of horizontal kinetic energy that is indicated by the vertical lines in the left figures. The top panels correspond to the fluid motions in a neutrally stratified core (N 0 = 0), and the bottom panels correspond to the motions in a core with a stably stratified outer layer with N 0 = 100.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse