Results 11 to 20 of about 197 (99)
This study examines how the congestus mode of tropical convection is expressed in numerical simulations of radiative‐convective equilibrium (RCE). We draw insights from the ensemble of cloud‐resolving models participating in the RCE Model Intercomparison
Adam B. Sokol, Dennis L. Hartmann
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The Diurnal Path to Persistent Convective Self‐Aggregation [PDF]
Clustering of tropical thunderstorms constitutes an important climate feedback because it influences the radiative balance. Convective self‐aggregation (CSA) is a profound modeling paradigm for explaining the clustering of tropical oceanic thunderstorms.
Gorm G. Jensen +2 more
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Cloud‐Radiation Interactions and Their Contributions to Convective Self‐Aggregation [PDF]
This study investigates the direct radiative‐convective processes that drive and maintain aggregation within convection‐permitting elongated channel (and smaller square) simulations of the UK Met Office Unified Model. Our simulations are configured using
Kieran N. Pope +3 more
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Forcing Convection to Aggregate Using Diabatic Heating Perturbations [PDF]
Tropical deep convection can aggregate into large clusters, which can have impacts on the local humidity and precipitation. Sea surface temperature (SST) gradients have been shown to organize convection, yet there has been little work done to investigate
Beth Dingley, Guy Dagan, Philip Stier
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Quantifying Convective Aggregation Using the Tropical Moist Margin's Length [PDF]
On small scales, the tropical atmosphere tends to be either moist or very dry. This defines two states that, on large scales, are separated by a sharp margin, well identified by the antimode of the bimodal tropical column water vapor distribution ...
Tom Beucler +2 more
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Circling in on Convective Self‐Aggregation [PDF]
AbstractIn radiative‐convective equilibrium simulations, convective self‐aggregation (CSA) is the spontaneous organization into segregated cloudy and cloud‐free regions. Evidence exists for how CSA is stabilized, but how it arises favorably on large domains is not settled. Using large‐eddy simulations, we link the spatial organization emerging from the
Nissen, Silas Boye, Haerter, Jan O.
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Tipping to an Aggregated State by Mesoscale Convective Systems
Radiative‐convective equilibrium simulations were suggested to resist self‐aggregation within a linearly stable regime at low surface temperatures. Recent numerical work shows that this linearly stable regime can rapidly transition to an aggregated state
I. L. Kruse, R. Fiévet, J. O. Haerter
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Sensitivity of Convective Self‐Aggregation to Subsidence
AbstractSimulations using the convection‐permitting MesoNH model with imposed vertical motion document the influence of large‐scale circulation on convective self‐aggregation. Results show that subsidence favors self‐aggregation in this model and that this sensitivity includes a hysteresis: for weak subsidence, only one stationary state is found ...
Bellon, Gilles, Coppin, David
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Distortions of the Rain Distribution With Warming, With and Without Self‐Aggregation
We investigate how mesoscale circulations associated with convective aggregation can modulate the sensitivity of the hydrologic cycle to warming. We quantify changes in the full distribution of rain across radiative‐convective equilibrium states in a ...
Benjamin Fildier +2 more
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A budget for the size of convective self‐aggregation [PDF]
There is no consensus on the physical mechanisms controlling the scale at which convective activity organizes near the Equator. Here, we introduce a diagnostic framework relating the evolution of the length‐scale of convective aggregation to the net radiative heating, the surface enthalpy flux, and horizontal energy transport.
Tom Beucler, Timothy Cronin
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