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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Radio occultations cannot separate Uranus or Neptune's internal spin from wind contributions to atmospheric shape, as the total rotation is already tightly constrained, though they can test wind assumptions and detect north-south asymmetries.
citing papers explorer
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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.
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Can radio occultations constrain Uranus or Neptune's internal rotation periods?
Radio occultations cannot separate Uranus or Neptune's internal spin from wind contributions to atmospheric shape, as the total rotation is already tightly constrained, though they can test wind assumptions and detect north-south asymmetries.