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Magnetically Induced Rotating Rayleigh-Taylor Instability
06:42

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Published on: March 3, 2017

Resistive wall mode instability at intermediate plasma rotation.

J W Berkery1, S A Sabbagh, R Betti

  • 1Department of Applied Physics and Applied Mathematics, Columbia University, New York, New York 10027, USA.

Physical Review Letters
|April 7, 2010
PubMed
Summary
This summary is machine-generated.

Resistive wall mode instability in fusion devices requires advanced models beyond simple rotation thresholds. Kinetic effects explain observed RWM behavior at intermediate plasma rotation, impacting future fusion energy research.

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Area of Science:

  • Plasma physics
  • Fusion energy research
  • Magnetohydrodynamics

Background:

  • Resistive wall modes (RWMs) are plasma instabilities that can degrade confinement in fusion devices.
  • Existing models often rely on simplified critical rotation thresholds that may not capture complex plasma behaviors.
  • Understanding RWMs is crucial for achieving stable plasma conditions necessary for fusion energy generation.

Purpose of the Study:

  • To investigate the insufficient predictive power of low critical rotation threshold models for RWM instability.
  • To explore the impact of kinetic effects on the relationship between plasma rotation and RWM stability.
  • To compare experimental RWM observations with theoretical calculations incorporating kinetic physics.

Main Methods:

  • Experimental observations of RWM instability in the National Spherical Torus Experiment (NSTX).
  • Theoretical calculations using the MISK code, incorporating kinetic modifications to ideal stability criteria.
  • Self-similar scaling of experimental plasma rotation profiles and collisionality to analyze mode resonances.

Main Results:

  • Experimental RWM instability observed at intermediate plasma rotation levels, challenging simple models.
  • MISK code calculations with kinetic effects show good agreement with experimental RWM marginal points.
  • Resonances between the RWM and ion precession drift/bounce frequencies were explored through profile scaling.
  • RWMs experimentally become unstable when plasma rotation is between stabilizing precession drift and bounce resonances.

Conclusions:

  • Low critical rotation threshold models are insufficient for explaining RWM behavior at intermediate rotation speeds.
  • Kinetic effects significantly influence RWM stability, leading to a more complex rotation-stability relationship.
  • The MISK code, including kinetic physics, successfully predicts experimental RWM behavior, validating theoretical advancements.