Abstract
- Received 9 March 2018
DOI:https://doi.org/10.1103/PhysRevFluids.3.059901
©2018 American Physical Society
Physics Subject Headings (PhySH)
Fluid Dynamics
Erratum: Onset of low Prandtl number thermal convection in thin spherical shells [Phys. Rev. Fluids 3, 024801 (2018)]
F. Garcia, F. R. N. Chambers, and A. L. Watts
Phys. Rev. Fluids 3, 059901 – Published 18 May 2018
Images
Figure 1
(a) Estimates of Ta and for stellar convective oceans and parameter values of the current (red) and previous (green) numerical studies of thermal convection, which are clearly still far from stellar conditions. (b) The same as (a) but for Ta and Pr. The estimated region of stability of the different convective instabilities SC (with stripes), EA (plain), and antisymmetric polar (AP)/SP (cross hatched) is also shown.
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