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.UP11.154
Abstract: UP11.00154 : Ion energization in the asymmetric reconnection diffusion region*
Presenter:
Shan Wang
(Univ of Maryland-College Park, NASA/GSFC)
Authors:
Shan Wang
(Univ of Maryland-College Park, NASA/GSFC)
Li-Jen Chen
(Univ of Maryland-College Park, NASA/GSFC)
Naoki Bessho
(Univ of Maryland-College Park, NASA/GSFC)
Michael Hesse
(University of Bergen)
Jongsoo Yoo
(Princeton Plasma Phys Lab)
Masaaki Yamada
(Princeton Plasma Phys Lab)
Yi-Hsin Liu
(Dartmouth College)
Daniel Gershman
(NASA/GSFC)
Barbara Giles
(NASA/GSFC)
Thomas Moore
(NASA/GSFC)
We investigate ion energization in the ion diffusion region (IDR) during asymmetric reconnection using particle-in-cell simulations and Magnetosphere Multiscale (MMS) mission observations. In particular, how the ion outflow is built up, the heating characteristics, and the relative importance between the reconnection (Er) and in-plane (Ein) electric fields are studied. The simulation result shows that Er and Ein overall have comparable contribution in energizing ions near the time of the peak reconnection rate, while Ein becomes more important later. Er is most important for accelerating ions entering the central electron diffusion region (EDR). Ein becomes important beyond the central EDR and dominates the net build-up of the ion outflow. Heating of demagnetized ions is mainly due to distributions with counter-streaming populations normal to the current layer. Downstream of the peak outflow, cyclotron turning around the reconnected and Hall magnetic fields leads to further gyrotropization and thermalization. Ion distribution features of acceleration by Er and Ein are observed by MMS.
*The research is supported in part by NSF grants AGS-1543598, AGS-1202537, AGS-1552142, DOE grant DESC0016278 and the NASA MMS mission.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.154
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