ﻻ يوجد ملخص باللغة العربية
Any magnetically confined plasma possesses a certain amount of available energy, defined as that part of the thermal energy that can be converted into instabilities and turbulence. Here, we present a calculation of the available energy carried by magnetically trapped electrons in a slender flux tube of collisionless plasma. This quantity is compared with nonlinear gyrokinetic simulations of the turbulent energy flux resulting from collisionless turbulence driven by a density gradient in various tokamak and stellarator devices. The numerical calculation of available energy is extremely fast and shows a strong correlation with energy fluxes found in the gyrokinetic simulations, which can be expressed as a simple power law and understood in terms of a phenomenological model.
The energy budget of a collisionless plasma subject to electrostatic fluctuations is considered, and the excess of thermal energy over the minimum accessible to it under various constraints that limit the possible forms of plasma motion is calculated
The concept of available energy of a collisionless plasma is discussed in the context of magnetic confinement. The available energy quantifies how much of the plasma energy can be converted into fluctuations (including nonlinear ones) and is thus a m
Identifying the sources of the highest energy cosmic rays requires understanding how they are deflected by the stochastic, spatially intermittent intergalactic magnetic field. Here we report measurements of energetic charged-particle propagation thro
This work addresses linear transport in turbulent media, with emphasis on neutral particle (atoms, molecules) transport in magnetized fusion plasmas. A stochastic model for turbulent plasmas, based upon a multivariate Gamma distribution, is presented
The effect of oscillatory shear flows on turbulent transport of passive scalar fields is studied by numerical computations based on the results provided by E. Kim [emph{Physics of Plasmas}, {bf 13}, 022308, 2006]. Turbulent diffusion is found to depe