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.UP11.43
Abstract: UP11.00043 : Effect of opacity on the density pedestal structure in DIII-D and Alcator C-Mod*
Presenter:
Saskia Mordijck
(William & Mary)
Authors:
Saskia Mordijck
(William & Mary)
Richard Joseph Groebner
(General Atomics - San Diego)
Tom Osborne
(General Atomics - San Diego)
Thomas Neil Carlstrom
(General Atomics - San Diego)
Fenton Glass
(General Atomics - San Diego)
Philip B Snyder
(General Atomics - San Diego)
Jerry W Hughes
(Massachusetts Inst of Tech-MIT)
Aaro E Jarvinen
(Lawrence Livermore Natl Lab)
Antti Salmi
(VTT)
Tuomas Tala
(VTT)
Florian Laggner
(Princeton Univ)
George R McKee
(Univ of Wisconsin, Madison)
Richard A Moyer
(Univ of California - San Diego)
Terry L Rhodes
(University of California, Los Angeles)
Lei Zeng
(Univ of California - Los Angeles)
Analysis of experimental data from DIII-D and C-Mod is used to study the role of opacity on the density pedestal structure. Dα measurements at the midplane on DIII-D indicate that we were able to push the ionization front further out by increasing the separatrix and SOL electron densities. We find that in pressure-record breaking EDA H-modes on C-Mod, adding more gas fueling does not result in an increase of the pedestal density, only an increase in the SOL density. In DIII-D, using gas puff modulations, we observe that when the outer strike point detaches, this strongly reduces the amplitude of the electron density response in the SOL and results in a larger amplitude inside the separatrix. Moreover, we observe the creation of an up-down asymmetry in the electron density with increased gas puff/opacity. Close to the X-point, up to ψN ~ 0.98, the electron density is larger than upstream in DIII-D. SOLPS modeling will be performed to get a better evaluation of the poloidal and radial ionization profiles as well as to better understand the origin of the up-down asymmetry of the electron density in DIII-D.
*This work is supported by the US DOE under DE-SC0007880, DE-FG02-08ER54984, DE-AC05-06OR23100, DE-FC02-04ER54698, and DE-SC0014264.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.43
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. |
© 2024 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