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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 6.

Total kinetic energy density of the librationally induced core flow as a function of the forcing frequency ω near Mercury’s observed libration frequency, ω = 0.67, indicated in each plot by the black vertical line. The top row gives the core response to the three types of libration forcing, m = 0 and ±2, in a neutrally stratified core (N 0 = 0 and r ICB = 0.4), and the bottom row shows the response in a core with an outer stably stratified layer (N 0 = 100, r ICB = 0.4, r C = 0.7, and h = 0.1). Different colored lines correspond to different Ekman numbers: Ek = 10−7 (blue), 10−8 (orange), and 10−9 (gray).

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