A Reduced Resistive Wall Mode Kinetic Stability Model for Disruption Forecasting

Berkery, J. W. ; Sabbagh, S. A.; Bell, R. E. ; Gerhardt, S. P. ; LeBlanc, B. P.
Issue date: 2017
Creative Commons Attribution 4.0 International (CC BY)
Cite as:
Berkery, J. W., Sabbagh, S. A., Bell, R. E., Gerhardt, S. P., & LeBlanc, B. P. (2017). A Reduced Resistive Wall Mode Kinetic Stability Model for Disruption Forecasting [Data set]. Princeton Plasma Physics Laboratory, Princeton University. https://doi.org/10.11578/1367870
  author      = {Berkery, J. W. and
                Sabbagh, S. A. and
                Bell, R. E. and
                Gerhardt, S. P. and
                LeBlanc, B. P.},
  title       = {{A Reduced Resistive Wall Mode Kinetic St
                ability Model for Disruption Forecasting
  publisher   = {{Princeton Plasma Physics Laboratory, Pri
                nceton University}},
  year        = 2017,
  url         = {https://doi.org/10.11578/1367870}

Kinetic modification of ideal stability theory from stabilizing resonances of mode-particle interaction has had success in explaining resistive wall mode (RWM) stability limits in tokamaks. With the goal of real-time stability forecasting, a reduced kinetic stability model has been implemented in the new Disruption Event Characterization and Forecasting (DECAF) code, which has been written to analyze disruptions in tokamaks. The reduced model incorporates parameterized models for ideal limits on beta, a ratio of plasma pressure to magnetic pressure, which are shown to be in good agreement with DCON code calculations. Increased beta between these ideal limits causes a shift in the unstable region of delta W_K space, where delta W_K is the change in potential energy due to kinetic effects that is solved for by the reduced model, such that it is possible for plasmas to be unstable at intermediate beta but stable at higher beta. Gaussian functions for delta W_K are defined as functions of E cross B frequency and collisionality, with parameters reflecting the experience of the National Spherical Torus Experiment (NSTX). The reduced model was tested on a database of discharges from NSTX and experimentally stable and unstable discharges were separated noticeably on a stability map in E cross B frequency, collisionality space. The reduced model only failed to predict an unstable RWM in 15.6% of cases with an experimentally unstable RWM and performed well on predicting stability for experimentally stable discharges as well.

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# Filename Filesize
1 readme.txt 2.78 KB
2 ARK_DATA.zip 57.7 KB