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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2026 2verdicts
UNVERDICTED 2representative citing papers
Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.
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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A New Scaling Law for Non-Dipolar Magnetic Fields in Rapidly Rotating Stars and Planets
Dynamo simulations show non-dipolar magnetic field strengths are comparable across dipolar and non-dipolar regimes when scaled by driving power, while the dipole component is an order of magnitude weaker in the non-dipolar regime.