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 CP11: Poster Session II: Basic Plasma Physics; Boundary, PMI, Proto-MPEX; International Tokamaks; Turbulence and Transport; Other Configurations; Z-pinch, Dense Plasma Focus and MagLIF (2:00pm-5:00pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.CP11.44
Abstract: CP11.00044 : Comparing Gyrokinetic Simulation Results and Linear Gyrofluid Closures to Develop Robust Closures*
Presenter:
Akash Shukla
(Univ of Texas, Austin)
Authors:
Akash Shukla
(Univ of Texas, Austin)
David R Hatch
(Univ of Texas, Austin)
Vasil Bratanov
(Univ of Texas, Austin)
Gyrofluid models are attractive because they provide a conceptually simpler and computationally efficient alternative to gyrokinetic models. They rely on a moment closure, which approximates the highest order fluid moment as a function of the lower order moments. Conventional gyrofluid models use linear closures designed to match the plasma dispersion function and can produce linear physics that closely matches gyrokinetics. However, these closures break down in the presence of turbulence, where the nonlinearity strongly modifies the kinetic physics. In order to develop a better understanding of the effects of nonlinear phenomena, we analyze a reduced gyrokinetic model. Detailed comparisons are made between the phase mixing in (1) the linear kinetic system, (2) the linear system closed with a Hammett-Perkins-like closure, and (3) the nonlinear turbulent system modeled by the DNA code. The closure predicts growth rates of the ITG mode that closely agree with the full linear kinetic system. However, the linear physics agrees with the dynamics in the nonlinear turbulent system only in very small regions of wavenumber-space. These discrepancies are analyzed in detail with the aim of formulating gyrofluid closures that are robust even in the presence of turbulence.
*SciDAC
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CP11.44
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2025 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700