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Rayleigh–Taylor and Richtmyer–Meshkov instability induced flow, turbulence, and mixing. II
Y Zhou - Physics Reports, 2017 - Elsevier
Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …
pathways towards turbulent mixing layers, in many cases characterized by significant mass …
Closed-loop turbulence control: Progress and challenges
Closed-loop turbulence control is a critical enabler of aerodynamic drag reduction, lift
increase, mixing enhancement, and noise reduction. Current and future applications have …
increase, mixing enhancement, and noise reduction. Current and future applications have …
[КНИГА][B] Моделирование крупных вихрей в расчетах турбулентных течений
К Волков, В Емельянов - 2022 - books.google.com
В книге дается систематическое изложение вопросов, связанных с применением
метода моделирования крупных вихрей для расчетов турбулентных течений …
метода моделирования крупных вихрей для расчетов турбулентных течений …
[HTML][HTML] Recent advances on the numerical modelling of turbulent flows
This paper reviews the problems and successes of computing turbulent flow. Most of the flow
phenomena that are important to modern technology involve turbulence. The review is …
phenomena that are important to modern technology involve turbulence. The review is …
Turbulence theories and statistical closure approaches
Y Zhou - Physics Reports, 2021 - Elsevier
When discussing research in physics and in science more generally, it is common to ascribe
equal importance to the three components of the scientific trinity: theoretical, experimental …
equal importance to the three components of the scientific trinity: theoretical, experimental …
Dissipation in turbulent flows
JC Vassilicos - Annual review of fluid mechanics, 2015 - annualreviews.org
This article reviews evidence concerning the cornerstone dissipation scaling of turbulence
theory:, with C ϵ= const., ϵ the dissipation rate of turbulent kinetic energy, and an integral …
theory:, with C ϵ= const., ϵ the dissipation rate of turbulent kinetic energy, and an integral …
Theory of star formation
We review current understanding of star formation, outlining an overall theoretical framework
and the observations that motivate it. A conception of star formation has emerged in which …
and the observations that motivate it. A conception of star formation has emerged in which …
Astrophysical magnetic fields and nonlinear dynamo theory
The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …
generation and maintenance by turbulence. In the astrophysical context this generation is …
Estimation of the dissipation rate of turbulent kinetic energy: A review
A comprehensive literature review on the estimation of the dissipation rate of turbulent
kinetic energy is presented to assess the current state of knowledge available in this area …
kinetic energy is presented to assess the current state of knowledge available in this area …
Turbulent heating in galaxy clusters brightest in X-rays
Abstract The hot (107 to 108 kelvin), X-ray-emitting intracluster medium (ICM) is the
dominant baryonic constituent of clusters of galaxies. In the cores of many clusters, radiative …
dominant baryonic constituent of clusters of galaxies. In the cores of many clusters, radiative …