Improvements to Stellar Structure Models, Based on a Grid of 3D Convection Simulations. I. $T(\tau)$-Relations [PDF]
, 2014 Relations between temperature, T, and optical depth, tau, are often used for describing the photospheric transition from optically thick to optically thin in stellar structure models.
Asplund, Martin +4 more
core +1 more source
Geophysical Research Letters, 2022 The nature of convective organization remains elusive, despite its importance in understanding the role of clouds in climate systems. This study reports a new type of large‐scale structure formed by the self‐organization of deep moist atmospheric ...
Tomoro Yanase +3 more
doaj +1 more source
The Impact of a Land‐Sea Contrast on Convective Aggregation in Radiative‐Convective Equilibrium
Journal of Advances in Modeling Earth Systems, 2023 Convective aggregation is an important atmospheric phenomenon which frequently occurs in idealized models in radiative‐convective equilibrium (RCE), where the effects of land, rotation, sea surface temperature gradients, and the diurnal cycle are often ...
Beth Dingley +3 more
doaj +1 more source
Convective cores in galactic cooling flows [PDF]
, 2000 We use hydrodynamic simulations with adaptive grid refinement to study the dependence of hot gas flows in X-ray luminous giant elliptical galaxies on the efficiency of heat supply to the gas. We consider a number of potential heating mechanisms including
Alexei Kritsuk +40 more
core +5 more sources
Cloud‐Radiation Interactions and Their Contributions to Convective Self‐Aggregation
Journal of Advances in Modeling Earth Systems, 2021 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
doaj +1 more source
Self-Organization of Atmospheric Macroturbulence into Critical States of Weak Nonlinear Eddy–Eddy Interactions [PDF]
, 2006 It is generally held that atmospheric macroturbulence can be strongly nonlinear. Yet weakly nonlinear models successfully account for scales and structures of baroclinic eddies in Earth's atmosphere.
Schneider, Tapio, Walker, Christopher C.
core +1 more source
Instabilities and Evolution of Radiative-Convective Equilibrium
, 2023 See README for more ...
Bolei, , Zhe-Min, , Ji
openaire +1 more source
Sensitivity of Convective Self‐Aggregation to Domain Size
Journal of Advances in Modeling Earth Systems, 2019 A 3‐D cloud‐resolving model has been used to investigate the domain size dependence of simulations of convective self‐aggregation (CSA) in radiative‐convective equilibrium. We investigate how large a domain is needed to allow multiple convective clusters
Casey R. Patrizio, David A. Randall
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The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and General Properties [PDF]
, 2013 We present the Stagger-grid, a comprehensive grid of time-dependent, 3D hydrodynamic model atmospheres for late-type stars with realistic treatment of radiative transfer, covering a wide range in stellar parameters. This grid of 3D models is intended for
Asplund, M. +7 more
core +1 more source
Ensemble of Radiative‐Convective Equilibrium Simulations Near the Aggregated and Scattered Boundary
Geophysical Research Letters, 2021 An ensemble of 10 radiative‐convective equilibrium (RCE) simulations near the sharp transition zone between scattered and aggregated states are examined in a square‐domain cloud‐resolving model.
Ching‐Shu Hung, Hiroaki Miura
doaj +1 more source