3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
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
-
Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
-
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.