Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session UP11: Poster Session VIII: MST; DIII-D Tokamak; SPARC, C-Mod, and High Field Tokamaks; HBT-EP; Transport and LPI in ICF Plasmas, Hydrodynamic Instability; HEDP Posters; Space and Astrophysical Plasmas (2:00pm-5:00pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.UP11.80
Abstract: UP11.00080 : Comparison of GDB edge simulations of Alcator C-Mod IWL L-mode with experimental measurements**
Presenter:
Ben Zhu
(Lawrence Livermore Natl Lab)
Authors:
Manaure Francisquez
(Dartmouth Coll)
Ben Zhu
(Lawrence Livermore Natl Lab)
Barrett Rogers
(Dartmouth Coll)
Four Alcator C-Mod IWL L-mode shots were simulated with the GDB code [1] -- a global 3D drift-reduced Braginskii based electromagnetic edge turbulence model evolves both plasma and flow profiles self-consistently in both SOL and close flux region. In these simulations, magnetic geometry and particle source profile were based on EFIT and KN1D model respectively [2]; plasma profiles were initially set to be close to experiment measurements but allowed to evolve freely afterwards. We found that well beyond turbulence saturated stage (>2 ms), the global plasma and the spontaneous generated E×B flow [3] profiles obtained from GDB simulations agree well with the MLP data. Turbulence statistics analysis [4] and comparison with MLP and GPI data are underway.
[1] Zhu et.al, CPC, in press (2018) [2] LaBombard, PSFC/RR-01-3, (2001)[3] Zhu et.al, PoP, 24, 055903, (2017)[4] Francisquez et.al, NF, 57, 116049 (2017)
*This work was supported by DOE-SC-0010508 and performed under the auspices of the U.S. DoE by LLNL under Contract DE-AC52-07NA27344 and. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.80
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