ALMA CO(3-2) observations with MCMC retrievals show latitudinal temperature trends on Neptune, including a cold southern polar layer at 300-600 mbar, consistent with Voyager at 10-100 mbar but new at deeper levels.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
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.
A new correlation method applied to Cassini/VIMS data measures Jupiter zonal winds at multiple altitudes, revealing weaker tropospheric vertical shear than previously reported.
citing papers explorer
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Latitudinal variations in Neptune's temperature profile observed with ALMA
ALMA CO(3-2) observations with MCMC retrievals show latitudinal temperature trends on Neptune, including a cold southern polar layer at 300-600 mbar, consistent with Voyager at 10-100 mbar but new at deeper levels.
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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.
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Jovian Zonal Winds Revealed from Cassini/VIMS Observations
A new correlation method applied to Cassini/VIMS data measures Jupiter zonal winds at multiple altitudes, revealing weaker tropospheric vertical shear than previously reported.