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 …
Comparing the statistics of interstellar turbulence in simulations and observations-Solenoidal versus compressive turbulence forcing
C Federrath, J Roman-Duval, RS Klessen… - Astronomy & …, 2010 - aanda.org
Context. Density and velocity fluctuations on virtually all scales observed with modern
telescopes show that molecular clouds (MCs) are turbulent. The forcing and structural …
telescopes show that molecular clouds (MCs) are turbulent. The forcing and structural …
The statistics of supersonic isothermal turbulence
We present results of large-scale three-dimensional simulations of supersonic Euler
turbulence with the piecewise parabolic method and multiple grid resolutions up to 2048 3 …
turbulence with the piecewise parabolic method and multiple grid resolutions up to 2048 3 …
Large-eddy simulations of magnetohydrodynamic turbulence in heliophysics and astrophysics
We live in an age in which high-performance computing is transforming the way we do
science. Previously intractable problems are now becoming accessible by means of …
science. Previously intractable problems are now becoming accessible by means of …
The fractal density structure in supersonic isothermal turbulence: solenoidal versus compressive energy injection
C Federrath, RS Klessen, W Schmidt - The Astrophysical Journal, 2009 - iopscience.iop.org
In a systematic study, we compare the density statistics in high-resolution numerical
experiments of supersonic isothermal turbulence, driven by the usually adopted solenoidal …
experiments of supersonic isothermal turbulence, driven by the usually adopted solenoidal …
Numerical dissipation vs. subgrid-scale modelling for large eddy simulation
This study presents an alternative way to perform large eddy simulation based on a targeted
numerical dissipation introduced by the discretization of the viscous term. It is shown that this …
numerical dissipation introduced by the discretization of the viscous term. It is shown that this …
Hyperviscosity, Galerkin truncation, and bottlenecks in turbulence
It is shown that the use of a high power α of the Laplacian in the dissipative term of
hydrodynamical equations leads asymptotically to truncated inviscid conservative dynamics …
hydrodynamical equations leads asymptotically to truncated inviscid conservative dynamics …
Energy spectrum in high-resolution direct numerical simulations of turbulence
A study is made about the energy spectrum E (k) of turbulence on the basis of high-
resolution direct numerical simulations (DNSs) of forced incompressible turbulence in a …
resolution direct numerical simulations (DNSs) of forced incompressible turbulence in a …
Two regimes of turbulent fragmentation and the stellar initial mass function from primordial to present-day star formation
P Padoan, Å Nordlund, AG Kritsuk… - The Astrophysical …, 2007 - iopscience.iop.org
Abstract The Padoan and Nordlund model of the stellar initial mass function (IMF) is derived
from low-order statistics of supersonic turbulence, neglecting gravity (eg, gravitational …
from low-order statistics of supersonic turbulence, neglecting gravity (eg, gravitational …
Dust diffusion in protoplanetary disks by magnetorotational turbulence
A Johansen, H Klahr - The Astrophysical Journal, 2005 - iopscience.iop.org
We measure the turbulent diffusion coefficient of dust grains embedded in magnetorotational
turbulence in a protoplanetary disk directly from numerical simulations and compare it to the …
turbulence in a protoplanetary disk directly from numerical simulations and compare it to the …