Results 31 to 40 of about 563,653 (367)

Development of convection along the SPCZ within a Madden-Julian oscillation [PDF]

open access: yes, 1996
A subtropical Rossby wave propagation mechanism is proposed to account for the poleward and eastward progression of intraseasonal convective anomalies along the South Pacific Convergence Zone (SPCZ) that is observed in a significant proportion of Madden ...
Ardanuy   +25 more
core   +2 more sources

Stellar Fluxes as Probes of Convection in Stellar Atmospheres [PDF]

open access: yes, 2006
Convection and turbulence in stellar atmospheres have a significant effect on the emergent flux from late-type stars. The theoretical advancements in convection modelling over recent years have proved challenging for the observers to obtain measurements ...
Adelman   +10 more
core   +2 more sources

Modulation of the Bifurcation in Radiative‐Convective Equilibrium by Gray‐Zone Cloud and Turbulence Parameterizations

open access: yesJournal of Advances in Modeling Earth Systems, 2021
This study investigates the mechanisms by which small‐scale turbulence and cloud physics determine the organization of large‐scale convection in radiative‐convective equilibrium (RCE), an idealization of the tropical atmosphere.
Xiaoming Shi, Yiyuan Fan
doaj   +1 more source

Comparison of two- and three-dimensional compressible convection in a pre-main sequence star [PDF]

open access: yesA&A 638, A15 (2020), 2020
Extending our recent studies of two-dimensional stellar convection to 3D, we compare three-dimensional hydrodynamic simulations to identically set-up two-dimensional simulations, for a realistic pre-main sequence star. We compare statistical quantities related to convective flows including: average velocity, vorticity, local enstrophy, and penetration ...
arxiv   +1 more source

Convection and oscillations [PDF]

open access: yesAstronomische Nachrichten, 2010
AbstractIn this short review on stellar convection dynamics I address the following, currently very topical, issues: (1) the surface effects of the Reynolds stresses and nonadiabaticity on solar‐like pulsation frequencies, and (2) oscillation mode lifetimes of stochastically excited oscillations in red giants computed with different time‐dependent ...
openaire   +4 more sources

Global climate impacts of stochastic deep convection parameterization in the NCAR CAM5

open access: yesJournal of Advances in Modeling Earth Systems, 2016
In this study, the stochastic deep convection parameterization of Plant and Craig (PC) is implemented in the Community Atmospheric Model version 5 (CAM5) to incorporate the stochastic processes of convection into the Zhang‐McFarlane (ZM) deterministic ...
Yong Wang, Guang J. Zhang
doaj   +1 more source

Test of the 'glymphatic' hypothesis demonstrates diffusive and aquaporin-4-independent solute transport in rodent brain parenchyma

open access: yeseLife, 2017
Transport of solutes through brain involves diffusion and convection. The importance of convective flow in the subarachnoid and paravascular spaces has long been recognized; a recently proposed ‘glymphatic’ clearance mechanism additionally suggests that ...
Alex J Smith   +4 more
doaj   +1 more source

Resistive and magnetized accretion flows with convection

open access: yes, 2012
We considered the effects of convection on the radiatively inefficient accretion flows (RIAF) in the presence of resistivity and toroidal magnetic field. We discussed the effects of convection on transports of angular momentum and energy.
A.A. Esin   +24 more
core   +1 more source

Convection in the Moon [PDF]

open access: yesNature, 1962
It is natural to inquire whether thermal convection is occurring in the Moon through solid state creep processes. The primary evidence is the departure of the Moon from the figure of hydrostatic equilibrium, but certain difficulties in the thermal history of the Moon are eased by assuming heat transfer by convection. If convection exists in the Moon it
openaire   +2 more sources

Circling in on Convective Organization [PDF]

open access: yesGeophysical Research Letters, 2019
AbstractCold pools (CPs) contribute to convective organization. However, it is unclear by which mechanisms organization occurs. By using a particle method to track CP gust fronts in large eddy simulations, we characterize the basic collision modes between CPs.
Haerter, Jan O.   +3 more
openaire   +6 more sources

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