Variability from Thermoresistive Instability in the Atmospheres of Hot Jupiters

The atmosphere of a hot Jupiter may be subject to a thermoresistive instability, in which the increasing electrical conductivity with temperature leads to runaway ohmic heating. We introduce a simplified model of the local dynamics in the equatorial region of a hot Jupiter that incorporates the back...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 940; no. 2; pp. 123 - 130
Main Authors Hardy, Raphaël, Cumming, Andrew, Charbonneau, Paul
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.12.2022
IOP Publishing
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ISSN0004-637X
1538-4357
DOI10.3847/1538-4357/ac9bfc

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