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A comparison of no-slip, stress-free and inviscid models of rapidly rotating fluid in a spherical shell

We investigate how the choice of either no-slip or stress-free boundary conditions affects numerical models of rapidly rotating flow in Earth’s core by computing solutions of the weakly-viscous magnetostrophic equations within a spherical shell, driven by a prescribed body force. For non-axisymmetri...

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Pubblicato in:Sci Rep
Autori principali: Livermore, Philip W., Bailey, Lewis M., Hollerbach, Rainer
Natura: Artigo
Lingua:Inglês
Pubblicazione: Nature Publishing Group 2016
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Accesso online:https://ncbi.nlm.nih.gov/pmc/articles/PMC4793234/
https://ncbi.nlm.nih.gov/pubmed/26980289
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/srep22812
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