Calculation of the Thermal Footprint of Resonant Magnetic Perturbations in DIII-D

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The effect of resonant magnetic perturbations on heat transport in DIII-D H-mode plasmas has been calculated by combining the TRIP3D field-line tracing code with the E3D two-fluid transport code. Simulations show that the divertor heat flux distribution becomes non-axisymmetric because heat flux is efficiently guided to the divertor along the three-dimensional invariant manifolds of the magnetic field. Calculations demonstrate that heat flux is spread over a wider area of the divertor target, thereby reducing the peak heat flux delivered during steady-state operation. Filtered optical cameras have observed non-axisymmetric particle fluxes at the strike-point and Langmuir probes have observed non-axisymmetric floating ... continued below

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Joseph, I; Evans, T; Moyer, R; Fenstermacher, M; Groth, M; Kasilov, S et al. September 14, 2007.

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The effect of resonant magnetic perturbations on heat transport in DIII-D H-mode plasmas has been calculated by combining the TRIP3D field-line tracing code with the E3D two-fluid transport code. Simulations show that the divertor heat flux distribution becomes non-axisymmetric because heat flux is efficiently guided to the divertor along the three-dimensional invariant manifolds of the magnetic field. Calculations demonstrate that heat flux is spread over a wider area of the divertor target, thereby reducing the peak heat flux delivered during steady-state operation. Filtered optical cameras have observed non-axisymmetric particle fluxes at the strike-point and Langmuir probes have observed non-axisymmetric floating potentials. On the other hand, the predicted magnitude of stochastic thermal transport is too large to match the pedestal plasma profiles measured by Thomson scattering and charge exchange recombination spectroscopy. The Braginskii thermal conductivity overestimates the expected heat transport in the pedestal because the mean free path is longer than estimates of the parallel thermal correlation length, and collisionless transport models are probably required for accurate description. However, even the collisionless estimates for electron thermal transport are too large by one to two orders of magnitude. Thus, it is likely that another mechanism such as rotational screening of resonant perturbations limits the stochastic region and reduces transport inside of the pedestal.

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PDF-file: 33 pages; size: 9.5 Mbytes

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  • Journal Name: Nuclear Fusion, vol. 48, no. 4, April 1, 2008, pp. 045009; Journal Volume: 48; Journal Issue: 4

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  • Report No.: UCRL-JRNL-234683
  • Grant Number: W-7405-ENG-48
  • Office of Scientific & Technical Information Report Number: 941388
  • Archival Resource Key: ark:/67531/metadc901160

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  • September 14, 2007

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  • Sept. 27, 2016, 1:39 a.m.

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  • Nov. 22, 2016, 9:50 p.m.

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Joseph, I; Evans, T; Moyer, R; Fenstermacher, M; Groth, M; Kasilov, S et al. Calculation of the Thermal Footprint of Resonant Magnetic Perturbations in DIII-D, article, September 14, 2007; Livermore, California. (digital.library.unt.edu/ark:/67531/metadc901160/: accessed November 12, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.