Full-wave simulations of ICRF heating regimes in toroidal plasmas with non-Maxwellian distribution functions

Bertelli, N. ; Valeo, E. J. ; Green, D. L.; Gorelenkova, M. ; Phillips, C. K. ; Podesta, M. ; Lee, J. P.; Wright, J. C.; Jaeger, E.
Issue date: 2017
Rights:
Creative Commons Attribution 4.0 International (CC BY)
Cite as:
Bertelli, N., Valeo, E. J., Green, D. L., Gorelenkova, M., Phillips, C. K., Podesta, M., Lee, J. P., Wright, J. C., & Jaeger, E. (2017). Full-wave simulations of ICRF heating regimes in toroidal plasmas with non-Maxwellian distribution functions [Data set]. Princeton Plasma Physics Laboratory, Princeton University. https://doi.org/10.11578/1356364
@electronic{bertelli_n_2017,
  author      = {Bertelli, N. and
                Valeo, E. J. and
                Green, D. L. and
                Gorelenkova, M. and
                Phillips, C. K. and
                Podesta, M. and
                Lee, J. P. and
                Wright, J. C. and
                Jaeger, E.},
  title       = {{Full-wave simulations of ICRF heating re
                gimes in toroidal plasmas with non-Maxwe
                llian distribution functions}},
  publisher   = {{Princeton Plasma Physics Laboratory, Pri
                nceton University}},
  year        = 2017,
  url         = {https://doi.org/10.11578/1356364}
}
Description:

At the power levels required for significant heating and current drive in magnetically-confined toroidal plasma, modification of the particle distribution function from a Maxwellian shape is likely [T. H. Stix, Nucl. Fusion, 15 737 (1975)], with consequent changes in wave propagation and in the location and amount of absorption. In order to study these effects computationally, both the finite-Larmor-radius and the high-harmonic fast wave (HHFW), versions of the full-wave, hot-plasma toroidal simulation code TORIC [M. Brambilla, Plasma Phys. Control. Fusion 41, 1 (1999) and M. Brambilla, Plasma Phys. Control. Fusion 44, 2423 (2002)], have been extended to allow the prescription of arbitrary velocity distributions of the form f(v||, v_perp, psi , theta). For hydrogen (H) minority heating of a deuterium (D) plasma with anisotropic Maxwellian H distributions, the fractional H absorption varies significantly with changes in parallel temperature but is essentially independent of perpendicular temperature. On the other hand, for HHFW regime with anisotropic Maxwellian fast ion distribution, the fractional beam ion absorption varies mainly with changes in the perpendicular temperature. The evaluation of the wave-field and power absorption, through the full wave solver, with the ion distribution function provided by either aMonte-Carlo particle and Fokker-Planck codes is also examined for Alcator C-Mod and NSTX plasmas. Non-Maxwellian effects generally tends to increase the absorption with respect to the equivalent Maxwellian distribution.

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# Filename Filesize
1 readme.txt 17.8 KB
2 ARK_DATA.zip 350 MB