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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Published in | The Astrophysical journal Vol. 940; no. 2; pp. 123 - 130 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.12.2022
IOP Publishing |
Subjects | |
Online Access | Get full text |
ISSN | 0004-637X 1538-4357 |
DOI | 10.3847/1538-4357/ac9bfc |
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