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 …

Closed-loop turbulence control: Progress and challenges

SL Brunton, BR Noack - Applied Mechanics …, 2015 - asmedigitalcollection.asme.org
Closed-loop turbulence control is a critical enabler of aerodynamic drag reduction, lift
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 …

[HTML][HTML] Recent advances on the numerical modelling of turbulent flows

CD Argyropoulos, NC Markatos - Applied Mathematical Modelling, 2015 - Elsevier
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 …

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 …

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 of star formation

CF McKee, EC Ostriker - Annu. Rev. Astron. Astrophys., 2007 - annualreviews.org
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 …

Astrophysical magnetic fields and nonlinear dynamo theory

A Brandenburg, K Subramanian - Physics Reports, 2005 - Elsevier
The current understanding of astrophysical magnetic fields is reviewed, focusing on their
generation and maintenance by turbulence. In the astrophysical context this generation is …

Estimation of the dissipation rate of turbulent kinetic energy: A review

G Wang, F Yang, K Wu, Y Ma, C Peng, T Liu… - Chemical Engineering …, 2021 - Elsevier
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 …

Turbulent heating in galaxy clusters brightest in X-rays

I Zhuravleva, E Churazov, AA Schekochihin, SW Allen… - Nature, 2014 - nature.com
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 …