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 GP11: Poster Session III: Basic Plasma Physics: General; Space and Astrophysical Plasmas; ICF Measurement and Computational Techniques, Direct and Indirect Drive; MIF Science and Technology (9:30am-12:30pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.GP11.77
Abstract: GP11.00077 : Particle orbits and electric fields in astrophysical jets*
Presenter:
Paul M Bellan
(Caltech)
Author:
Paul M Bellan
(Caltech)
elsewhere. It was recently shown [1] that neutral-ion clumps having a
critical q/m in a weakly ionized protostellar accretion disk spiral
inwards and accumulate at small radius to produce a positively charged
cloud. Because the spiral motion depends on q/m, electrons do not
similarly spiral in and, instead, try to neutralize the positive charge
cloud by flowing along poloidal magnetic flux surfaces outside the disk.
This creates a complete poloidal electric current circuit where the inward
spiraling positive clumps are the power source and the jets are the load.
Toroidal magnetic field links the poloidal current so resultant J x B
forces drive bi-directional jets while also providing a Z-pinch
radial equilibrium. A radial EMF must supply the continuously increasing
toroidal flux in the lengthening, constant-current jets. Lorentz
transformation to the lab frame of Harris's Bennett pinch solution [2] supports
this point of view by showing that a Z-pinch moving with axial center of
mass velocity Vz has a lab-frame electric field Er = VzBphi.
[3] E. G. Harris, Nuovo Cimento 23 (1962) 115
*Supported by USDOE Grant DE-FG02-04ER54755
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.GP11.77
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