Effective Drag in Rotating, Poorly Conducting Plasma Turbulence

Effective Drag in Rotating, Poorly Conducting Plasma Turbulence

<jats:title>Abstract</jats:title> <jats:p>Despite the increasing sophistication of numerical models of hot Jupiter atmospheres, the large timescale separation required in simulating the wide range in electrical conductivity between the dayside and nightside has made...

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Bibliographic Details
Main Authors: Benavides, Santiago J, Burns, Keaton J, Gallet, Basile, Flierl, Glenn R
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:English
Published: American Astronomical Society 2023
Online Access:https://hdl.handle.net/1721.1/148081

Internet

https://hdl.handle.net/1721.1/148081

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