Bulletin of the American Physical Society
64th Annual Meeting of the APS Division of Plasma Physics
Volume 67, Number 15
Monday–Friday, October 17–21, 2022; Spokane, Washington
Session GO07: Laboratory Plasma Astrophysics
9:30 AM–12:18 PM,
Tuesday, October 18, 2022
Room: 401 ABC
Chair: Sergey Lebedev, Imperial College London
Abstract: GO07.00007 : Modeling of Young Stellar Objects through the study of magnetized rear-driven plasma jets from thin foil targets*
10:42 AM–10:54 AM
Presenter:
Pablo Perez-Martin
(Helmholtz-Zentrum Dresden-Rossendorf)
Authors:
Pablo Perez-Martin
(Helmholtz-Zentrum Dresden-Rossendorf)
Michal Šmíd
(Helmholtz-Zentrum Dresden-Rossendorf)
Victorien Bouffetier
(European XFEL)
Florian-Emanuel Brack
(Helmholtz-Zentrum Dresden-Rossendorf)
Petr Cagas
(Virginia Tech)
Michal Červenák
(Czech Academy of Sciences)
Fabian Donat
(Helmholtz-Zentrum Dresden-Rossendorf)
Pavel Gajdos
(Czech Technical University)
Zhiyu He
(Shanghai Institute of Laser Plasma)
Milan Holec
(Lawrence Livermore Natl Lab)
Grigory Kagan
(Imperial College London)
Lenka Hronová
(Czech Technical University)
Kakolee F Kaniz
(Jagannath University)
Michaela Kozlova
(Helmholtz-Zentrum Dresden-Rossendorf)
Florian Kroll
(Helmholtz-Zentrum Dresden-Rossendorf)
Huiya Liu
(Shanghai Institute of Laser Plasma)
Xiayun Pan
(Helmholtz-Zentrum Dresden-Rossendorf)
Irene Prencipe
(Helmholtz-Zentrum Dresden-Rossendorf)
Gabriel Schaumann
(Technische Universität Darmstädt)
Sushil K Singh
(Czech Academy of Sciences)
Manfred Sobiella
(Helmholtz-Zentrum Dresden-Rossendorf)
Bhuvana Srinivasan
(Virginia Tech)
Jamil Stafford
(Virginia Tech)
Jinren Sun
(Shanghai Institute of Laser Plasma)
Zhiyong Xie
(Shanghai Institute of Laser Plasma)
Jun Xiong
(Shanghai Institute of Laser Plasma)
Panzheng Zhang
(Shanghai Institute of Optics and Fine Mechanics)
Yan Zhang
(Shanghai Institute of Optics and Fine Mechanics)
Francisco Suzuki-Vidal
(Imperial College London / First Light Fusion)
Miroslav Krůs
(Czech Academy of Sciences)
Lei Ren
(Shanghai Institute of Optics and Fine Mechanics)
Ning Kang
(Shanghai Institute of Optics and Fine Mechanics)
Katerina Falk
(Helmholtz-Zentrum Dresden-Rossendorf)
Magnetic fields were generated using a pair of Helmholtz coils that provide 5-10 T in the direction perpendicular to the jet propagation. The diagnostics used were the streaked optical self-emission as a measurement of jet velocity, and 4-frame interferometry as a measurement of the jet density.
With the right scaling factors, this data can help model the accretion of matter into magnetized astrophysical systems, such as the surface of Young Stellar Objects, as well as the role that instabilities play in this process [4].
[1] G. Revet et al., Science Advances 3, 11 (2017)
[2] Kulkarni, A. K. \& Romanova, M. M. , Monthly Notices RAS 386, (2008)
[3] E. Falize, et al., Astrophysics and Space Science 336, 81 (2011)
[4] Burdonov, K. et al., A\&A 657, A112 (2022)
*This work was supported by the Helmholtz Association under Grant No. VH-NG-1338
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