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Hot Jupiter Magnetospheres
ASTROPHYSICAL JOURNAL, no. 2 (2011)
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The upper atmospheres of close-in gas giant exoplanets ("hot Jupiters") are subjected to intense heating and tidal forces from their parent stars. The atomic (H) and ionized (H+) hydrogen layers are sufficiently rarefied that magnetic pressure may dominate gas pressure for expected planetary magnetic field strength. We examine the structu...More
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