Penetrative Convection in Partly Stratified Rapidly Rotating Spherical Shells
Many celestial objects are thought to host interfaces between convective and stable stratified interior regions. The interaction between both, e.g., the transfer of heat, mass, or angular momentum depends on whether and how flows penetrate into the stable layer. Powered from the unstable, convective...
Main Authors: | Wieland Dietrich, Johannes Wicht |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2018-11-01
|
Series: | Frontiers in Earth Science |
Subjects: | |
Online Access: | https://www.frontiersin.org/article/10.3389/feart.2018.00189/full |
Similar Items
-
Convection in rotating non-uniformly stratified spherical fluid shells: a systematic parameter study
by: Ján ŠIMKANIN, et al.
Published: (2009-09-01) -
Effects of Shell Thickness on Cross-Helicity Generation in Convection-Driven Spherical Dynamos
by: Luis Silva, et al.
Published: (2020-12-01) -
Convection in a differentially heated rotating spherical shell of Boussinesq fluid with radiative forcing
by: Babalola, David
Published: (2013) -
Hydromagnetic dynamos in rotating spherical fluid shells in dependence on the Prandtl number, density stratification and electromagnetic boundary conditions
by: Tomáš ŠOLTIS, et al.
Published: (2014-12-01) -
Dynamic Analysis of Thin CompositeCylindrical and Spherical Shells
by: Qusai H. Jebur
Published: (2008-01-01)