We study of the effect of turbulence on heat transfer within magnetized plasmas for energy injection velocities both larger and smaller that the Alfven speed. We find that in the latter regime the heat transfer is partially suppressed, while in the former regime the effects of turbulence depend on the intensity of driving. In fact, the scale l at which the turbulent velocity is equal the Alfven velocity is a new important parameter. When the electron mean free path is larger than l, the stronger the the turbulence, the lower thermal conductivity by electrons is. The turbulent motions, however, induces their own advective heat transport, which, for the parameters of intracluster medium (ICM) provides effective heat diffusivity that exceeds t...
The scaling of turbulence-driven heat transport with system size in magnetically confined plasmas is...
The basic character of diffusive transport in a magnetised plasma depends on what kind of transport ...
Turbulent heat transfer and heat conductivity effects on magnetospheric temperature distributio
Recent work on Alfvenic turbulence by Goldreich & Sridhar (1995; GS) suggests that the energy cascad...
Previous formulations of heating and transport associated with strong magnetohydrodynamic (MHD) turb...
A decrease in global energy confinement with increase in the heating power is observed in the L...
Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta plasmas, bu...
In conventional gases and plasmas, it is known that heat fluxes are proportional to temperature grad...
In many magnetized, dilute astrophysical plasmas, thermal conduction occurs almost exclusively paral...
Particle heating in advection-dominated accretion flows (ADAFs) by nonlinear MHD (Alfvenic) turbulen...
Transport equations for electron thermal energy in the high $\beta_e$ intracluster medium (ICM) are ...
The theory of magnetohydrodynamic (MHD) turbulence predicts that Alfv\'enic and slow-mode-like compr...
The role of thermal conduction in regulating the thermal behavior of cooling flows in galaxy cluster...
I review particle heating by MHD turbulence in collisionless plasmas appropriate to advection-domina...
International audienceThe role of thermal conduction in regulating the thermal behavior of cooling f...
The scaling of turbulence-driven heat transport with system size in magnetically confined plasmas is...
The basic character of diffusive transport in a magnetised plasma depends on what kind of transport ...
Turbulent heat transfer and heat conductivity effects on magnetospheric temperature distributio
Recent work on Alfvenic turbulence by Goldreich & Sridhar (1995; GS) suggests that the energy cascad...
Previous formulations of heating and transport associated with strong magnetohydrodynamic (MHD) turb...
A decrease in global energy confinement with increase in the heating power is observed in the L...
Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta plasmas, bu...
In conventional gases and plasmas, it is known that heat fluxes are proportional to temperature grad...
In many magnetized, dilute astrophysical plasmas, thermal conduction occurs almost exclusively paral...
Particle heating in advection-dominated accretion flows (ADAFs) by nonlinear MHD (Alfvenic) turbulen...
Transport equations for electron thermal energy in the high $\beta_e$ intracluster medium (ICM) are ...
The theory of magnetohydrodynamic (MHD) turbulence predicts that Alfv\'enic and slow-mode-like compr...
The role of thermal conduction in regulating the thermal behavior of cooling flows in galaxy cluster...
I review particle heating by MHD turbulence in collisionless plasmas appropriate to advection-domina...
International audienceThe role of thermal conduction in regulating the thermal behavior of cooling f...
The scaling of turbulence-driven heat transport with system size in magnetically confined plasmas is...
The basic character of diffusive transport in a magnetised plasma depends on what kind of transport ...
Turbulent heat transfer and heat conductivity effects on magnetospheric temperature distributio