Zonal asymmetries in midlatitude flow produce an upstream displacement of blocking frequency under Arctic warming via reduced carrying capacity and threshold onset in the Traffic Jam theory, as diagnosed in asymmetric aquaplanet experiments.
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4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
years
2026 4verdicts
UNVERDICTED 4representative citing papers
3D GCM simulations favor a thick (>=10 bar), CO2-rich (>1% mixing ratio) atmosphere for 55 Cancri e that matches JWST spectra while ruling out thin or CO/CO2-poor cases.
In a Held-Suarez GCM, abrupt transition to equatorial superrotation is controlled by meridional temperature gradient and bottom friction through competition between tropical wave-jet and extratropical wave absorption feedbacks.
Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.
citing papers explorer
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Zonal asymmetries control the response of atmospheric blocking to Arctic warming in an aquaplanet experiment
Zonal asymmetries in midlatitude flow produce an upstream displacement of blocking frequency under Arctic warming via reduced carrying capacity and threshold onset in the Traffic Jam theory, as diagnosed in asymmetric aquaplanet experiments.
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Reinterpreting the JWST Observations of 55 Cancri e with a Non-Grey General Circulation Model
3D GCM simulations favor a thick (>=10 bar), CO2-rich (>1% mixing ratio) atmosphere for 55 Cancri e that matches JWST spectra while ruling out thin or CO/CO2-poor cases.
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Factors governing the existence of an abrupt transition to superrotation in an idealized GCM
In a Held-Suarez GCM, abrupt transition to equatorial superrotation is controlled by meridional temperature gradient and bottom friction through competition between tropical wave-jet and extratropical wave absorption feedbacks.
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Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.