Conveners
Instabilities and confinement: Instabilities and confinement
- Per Helander
-
Kaixuan Fan (Shanghai Jiao Tong University)05/10/2026, 14:00Main trackOral presentation
We propose a method for predicting the nonlinear saturation level of convective instabilities in neutral and magnetized fluids. The method combines Gardner's restacking algorithm, which computes the available energy and ground states of collisionless plasmas in phase space, and Lagrangian relaxation, where fluid elements find lower-energy equilibria while preserving local invariants. For the...
Go to contribution page -
Paul Costello (Max Planck Institute for Plasma Physics)05/10/2026, 14:40Main trackOral presentation
The microinstabilities that cause the confinement-limiting turbulence in modern fusion devices are driven by the radial gradients of density and temperature in the plasma. In multi‑scale gyrokinetic theory [1], these gradients act as a source of background free energy that feeds instabilities on the fluctuating micro scales, giving rise to turbulence, and ultimately, energy transport down the...
Go to contribution page -
DR Hatch05/10/2026, 15:50Main trackOral presentation
Transport barriers in magnetically confined plasmas pose an intriguing thermodynamic problem: large gradients, and hence substantial free energy, can coexist with strongly reduced turbulent transport. We examine this phenomenon from the perspective of constrained nonequilibrium dynamics. A macroscopic thermodynamic model treats the plasma boundary layer as a heat engine in which incoming power...
Go to contribution page -
Daishi Toriyama (GSES, Kyoto Univ.)05/10/2026, 16:30Main trackOral presentation
Plasma turbulence is a dominant factor limiting energy confinement time in toroidal fusion plasmas, making computationally cheap confinement proxies highly desirable for quickly identifying experimentally attractive scenarios. In this presentation, we investigate whether "Available Energy (AE)” - an upper limit on the thermal energy available to drive Trapped Electron Mode (TEM) turbulence in...
Go to contribution page