Wind speed measurements in seven ultra-hot Jupiters decrease with temperature, consistent with magnetic drag and implying magnetic field strengths of a few gauss.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Tilted magnetic dipoles in hot Jupiter GCMs create north-south temperature asymmetries and wind deflections, while stronger fields increase phase curve amplitude and reduce hotspot offset.
citing papers explorer
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Magnetic field strengths of hot giant exoplanets consistent with Solar System values
Wind speed measurements in seven ultra-hot Jupiters decrease with temperature, consistent with magnetic drag and implying magnetic field strengths of a few gauss.
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Exploring the Impact of Tilted Magnetic Dipoles on the Atmospheric Dynamics of Hot Jupiters: Towards an Improved Magnetohydrodynamic Framework
Tilted magnetic dipoles in hot Jupiter GCMs create north-south temperature asymmetries and wind deflections, while stronger fields increase phase curve amplitude and reduce hotspot offset.