z-logo
open-access-imgOpen Access
Strange Attractors in Drift Wave Turbulence
Author(s) -
J. L. V. Lewandowski
Publication year - 2003
Publication title -
osti oai (u.s. department of energy office of scientific and technical information)
Language(s) - English
Resource type - Reports
DOI - 10.2172/814755
Subject(s) - dissipative system , attractor , physics , tokamak , turbulence , plasma , collision , chaotic , classical mechanics , zonal flow (plasma) , collision frequency , mechanics , statistical physics , quantum electrodynamics , quantum mechanics , mathematics , mathematical analysis , computer science , computer security , artificial intelligence
There are growing experimental, numerical and theoretical evidences that the anomalous transport observed in tokamaks and stellarators is caused by slow, drift-type modes (such as trapped electron modes and ion-temperature gradient-driven modes). Although typical collision frequencies in hot, magnetized fusion plasmas can be quite low in absolute values, collisional effects are nevertheless important since they act as dissipative sinks. As it is well known, dissipative systems with many (strictly speaking more than two) degrees of freedom are often chaotic and may evolve towards a so-called attractor

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom