Results 1 to 10 of about 34,696 (227)
Modeling the Formation of Clouds in Brown Dwarf Atmospheres [PDF]
Because the opacity of clouds in substellar mass object (SMO) atmospheres depends on the composition and distribution of particle sizes within the cloud, a credible cloud model is essential for accurately modeling SMO spectra and colors. We present a one-
Burrows, Adam +4 more
core +2 more sources
Internal Ocean‐Atmosphere Variability in Kilometer‐Scale Radiative‐Convective Equilibrium
We describe internal, low‐frequency variability in a 21‐year simulation with a cloud‐resolving model. The model domain is the length of the equatorial Pacific and includes a slab ocean, which permits coherent cycles of sea surface temperature (SST ...
Adam B. Sokol +3 more
doaj +1 more source
Deep convection over tropical oceans often appears intensified at the edge of convectively active regions, both in idealized studies and in observations.
J. M. Windmiller, C. Hohenegger
doaj +1 more source
We present a new approach to study the properties of the sun. We consider small variations of the physical and chemical properties of the sun with respect to Standard Solar Model predictions and we linearize the structure equations to relate them to the ...
Ricci, B., Villante, F. L.
core +1 more source
Study of the average vertical distribution of temperature in the martian atmosphere final report [PDF]
Convective-radiative equilibrium model for computing temperature profile - vertical temperature distribution in Martian ...
Mariano, J. F., Ohring, G.
core +1 more source
Self‐Aggregation of Convective Clouds With Interactive Sea Surface Temperature
This study investigates the feedbacks between an interactive sea surface temperature (SST) and the self‐aggregation of deep convective clouds, using a cloud‐resolving model in nonrotating radiative‐convective equilibrium.
S. Shamekh +3 more
doaj +1 more source
Thermal Structure and Radius Evolution of Irradiated Gas Giant Planets
We consider the thermal structure and radii of strongly irradiated gas giant planets over a range in mass and irradiating flux. The cooling rate of the planet is sensitive to the surface boundary condition, which depends on the detailed manner in which ...
Lars Bildsten, Marcy G. W., Phil Arras
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Aerosol‐cloud interactions are a persistent source of uncertainty in climate research. This study presents findings from a model intercomparison project examining the impact of aerosols on clouds and climate in convection‐permitting radiative‐convective ...
Guy Dagan +20 more
doaj +1 more source
Using a nonhydrostatic model based on a version of Geophysical Fluid Dynamics Laboratory's FV3 dynamical core at a cloud‐resolving resolution in radiative‐convective equilibrium (RCE) configuration, the sensitivity of the mean RCE climate to the ...
Usama M. Anber +3 more
doaj +1 more source
Quantifying Convective Aggregation Using the Tropical Moist Margin's Length
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
doaj +1 more source

