Jul 2 – 6, 2018
Žofín Palace
Europe/Prague timezone

I4.405 Overview of the Basic Plasma Science Facility: the physics of waves relevant to space, astrophysical and fusion plasmas

Jul 5, 2018, 4:30 PM
30m
Mánes Bar

Mánes Bar

Talk BSAP

Speaker

Troy Carter

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/I4.405.pdf Overview of the Basic Plasma Science Facility: the physics of waves relevant to space, astrophysical and fusion plasmas T.A. Carter, S. Dorfman, W. Gekelman, G. Morales, S. Tripathi, B. Van Compernolle, S. Vincena Dept. of Physics and Astronomy, UCLA The Basic Plasma Science Facility (BaPSF) at UCLA is a US national user facility for studies of fundamental processes in magnetized plasmas. The centerpiece of the facility is the Large Plasma Device (LAPD), a 20m long, magnetized linear plasma device [1]. This LAPD has been utilized to study a number of fundamental processes, including: collisionless shocks [2], dispersion and damping of kinetic and inertial Alfvén waves [3], flux ropes and magnetic recon- nection [4], three-wave interactions and parametric instabilities of Alfvén waves [5], turbulence and transport [6] and interactions of energetic ions and electrons with plasma waves [7]. A brief overview of research using the facility will be given, followed by a more detailed discussion of studies of the nonlinear physics of Alfvén waves [8]. Recent experiments have resulted in the first laboratory observation of the parametric instability of shear Alfvén waves. Shear waves with sufficiently high ω/Ωc,i (> 0.6) and above a threshold wave amplitude are observed to de- cay into co-propagating daughter waves; one a shear Alfvén wave and the other a low-frequency quasimode. The observed process is similar to the modulational decay instability. References [1] W. Gekelman, et al., Review of Scientific Instruments 87, 025105 (2016). [2] A.S. Bondarenko, et al., Nature Physics 13, 573 (2017). [3] C.A. Kletzing, et al., Phys. Rev. Lett. 104, 095001 (2010). [4] W. Gekelman, et al., Phys. Rev. Lett. 116, 235101 (2016). [5] G. Howes, et al., Phys. Rev. Lett. 109, 255001 (2012). [6] D.A. Schaffner, et al., Phys. Rev. Lett. 109, 135002 (2012). [7] B. Van Compernolle, et al., Phys. Rev. Lett. 114, 245002 (2015). [8] S. Dorfman and T.A. Carter, Phys. Rev. Lett. 116, 195002 (2016).

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