Intermittent deviation from average dispersion curves reveals differences between the dynamics of magnetohydrodynamic turbulence and hydrodynamic turbulence. Turbulent dispersion is typically measured by the average separation of a group of Lagrangian tracer particles from each other as the particles move in a turbulent flow. On average, the particles will increase their separation as time evolves. However, due to the intermittent nature of turbulence, radical deviations from this behavior can be observed when considering individual groups of particles. When the group consists only of two particles, those two particles sometimes can move toward each other for short periods of time, decreasing their separation. When the group consists instea...
The relative dispersion of pairs of inertial particles in incompressible, homogeneous, and isotropic...
The statistical geometry of dispersing Lagrangian clusters of four particles (tetrahedra) is studied...
Transport of mass, heat and momentum in turbulent flows by far exceeds that in stable laminar fluid ...
Intermittent deviation from average dispersion curves reveals differences between the dynamics of ma...
Large-scale magnetic fields thread through the electrically conducting matter of the interplanetary ...
Measurements in the heliosphere and high‐resolution fluid simulations give clear indications for the...
Magnetohydrodynamic(MHD)turbulence is studied from the Lagrangian viewpoint by following fluid parti...
Turbulence plays a fundamental role in many astrophysical flows such as convection in stars, stella...
This is a contributed talk, presented at the 2017 AGU Fall Meeting in New Orleans, USA in the sessio...
A comparison of turbulent diffusion and pair-dispersion in homogeneous, macroscopically isotropic Na...
We present a numerical study of two-particle dispersion from point sources in three-dimensional inco...
The properties of magnetohydrodynamic (MHD) turbulence under the influence of a strong mean magnetic...
Some of the concepts underlying particle dispersion due to turbulence are reviewed. The traditional ...
A higher-order multiscale analysis of spatial anisotropy in inertial range magnetohydrodynamic turbu...
Results from Direct Numerical Simulations of particle relative dispersion in three dimensional homog...
The relative dispersion of pairs of inertial particles in incompressible, homogeneous, and isotropic...
The statistical geometry of dispersing Lagrangian clusters of four particles (tetrahedra) is studied...
Transport of mass, heat and momentum in turbulent flows by far exceeds that in stable laminar fluid ...
Intermittent deviation from average dispersion curves reveals differences between the dynamics of ma...
Large-scale magnetic fields thread through the electrically conducting matter of the interplanetary ...
Measurements in the heliosphere and high‐resolution fluid simulations give clear indications for the...
Magnetohydrodynamic(MHD)turbulence is studied from the Lagrangian viewpoint by following fluid parti...
Turbulence plays a fundamental role in many astrophysical flows such as convection in stars, stella...
This is a contributed talk, presented at the 2017 AGU Fall Meeting in New Orleans, USA in the sessio...
A comparison of turbulent diffusion and pair-dispersion in homogeneous, macroscopically isotropic Na...
We present a numerical study of two-particle dispersion from point sources in three-dimensional inco...
The properties of magnetohydrodynamic (MHD) turbulence under the influence of a strong mean magnetic...
Some of the concepts underlying particle dispersion due to turbulence are reviewed. The traditional ...
A higher-order multiscale analysis of spatial anisotropy in inertial range magnetohydrodynamic turbu...
Results from Direct Numerical Simulations of particle relative dispersion in three dimensional homog...
The relative dispersion of pairs of inertial particles in incompressible, homogeneous, and isotropic...
The statistical geometry of dispersing Lagrangian clusters of four particles (tetrahedra) is studied...
Transport of mass, heat and momentum in turbulent flows by far exceeds that in stable laminar fluid ...