Microtearing turbulence: magnetic braiding and disruption limit - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue Physics of Plasmas Année : 2015

Microtearing turbulence: magnetic braiding and disruption limit

Résumé

A realistic reduced model involving a large poloidal spectrum of microtearing modes is used to probe the existence of some stochasticity of magnetic field lines. Stochasticity is shown to occur even for the low values of the magnetic perturbation δB/B devoted to magnetic turbulence that have been experimentally measured. Because the diffusion coefficient may strongly depend on the radial (or magnetic-flux) coordinate, being very low near some resonant surfaces, and because its evaluation implicitly makes a normal diffusion hypothesis, one turns to another indicator appropriate to diagnose the confinement: the mean residence time of magnetic field lines. Their computation in the microturbulence frame points to the existence of a disruption limit, namely of a critical order of magnitude of δB/B above which stochasticity is no longer benign yet leads to a macroscopic loss of confinement in some tens to hundred of electron toroidal excursions. Since the level of magnetic turbulence δB/B has been measured to grow with the plasma electron density this would also be a density limit.
Fichier principal
Vignette du fichier
microtearing_PoP_Revised.pdf (1.23 Mo) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)
Loading...

Dates et versions

hal-01248802 , version 1 (28-12-2015)

Identifiants

Citer

Marie-Christine Firpo. Microtearing turbulence: magnetic braiding and disruption limit. Physics of Plasmas, 2015, 22, pp.122511 ⟨10.1063/1.4938273⟩. ⟨hal-01248802⟩
195 Consultations
216 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More