The Mochi LabJet Experiment for Measurements of Canonical Helicity Injection in a Laboratory Astrophysical Jet

You, Setthivoine; von der Linden, Jens; Lavine, Eric Sander; Carroll, Evan Grant; Card, Alexander; Quinley, Morgan; Azuara-Rosales, Manuel

doi:10.3847/1538-4365/aaba6f

Title: The Mochi LabJet Experiment for Measurements of Canonical Helicity Injection in a Laboratory Astrophysical Jet

Journal Article · 16 May 2018 · The Astrophysical Journal. Supplement Series (Online)

DOI: https://doi.org/10.3847/1538-4365/aaba6f · OSTI ID:1458704

^[1];

^[2];

^[2]; Carroll, Evan Grant ^[2]; Card, Alexander ^[2]; Quinley, Morgan ^[2]; Azuara-Rosales, Manuel ^[2]

Univ. of Washington, Seattle, WA (United States). Aeronautics & Astronautics; Univ. of Tokyo (Japan). Graduate School of Frontier Sciences
Univ. of Washington, Seattle, WA (United States). Aeronautics & Astronautics

The Mochi device is a new pulsed power plasma experiment designed to produce long, collimated, stable, magnetized plasma jets when set up in the LabJet configuration. The LabJet configuration aims to simulate an astrophysical jet in the laboratory by mimicking an accretion disk threaded by a poloidal magnetic field with concentric planar electrodes in front of a solenoidal coil. The unique setup consists of three electrodes, each with azimuthally symmetric gas slits. Two of the electrodes are biased independently with respect to the third electrode to control the radial electric field profile across the poloidal bias magnetic field. This design approximates a shear azimuthal rotation profile in an accretion disk. The azimuthally symmetric gas slits provide a continuously symmetric mass source at the footpoint of the plasma jet, so any azimuthal rotation of the plasma jet is not hindered by a discrete number of gas holes. The initial set of diagnostics consists of current Rogowski coils, voltage probes, magnetic field probe arrays, an interferometer and ion Doppler spectroscopy, supplemented by a fast ion gauge and a retarding grid energy analyzer. The measured parameters of the first plasmas are ~10²² m^-3, ~0.4 T, and 5–25 eV, with velocities of ~20–80 km s^-1. Finally, the combination of a controllable electric field profile, a flared poloidal magnetic field, and azimuthally symmetric mass sources in the experiment successfully produces short-lived (~10 μs, ≳5 Alfvén times) collimated magnetic jets with a ~10:1 aspect ratio and long-lived (~100 μs, ≳40 Alfvén times) flow-stabilized, collimated, magnetic jets with a ~30:1 aspect ratio.

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Research Organization:: Univ. of Washington, Seattle, WA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Fusion Energy Sciences (FES) (SC-24)

Grant/Contract Number:: SC0010340

OSTI ID:: 1458704

Report Number(s):: LLNL-JRNL-740210; 894204

Journal Information:: The Astrophysical Journal. Supplement Series (Online), Journal Name: The Astrophysical Journal. Supplement Series (Online) Journal Issue: 2 Vol. 236; ISSN 1538-4365

Publisher:: American Astronomical Society/IOPCopyright Statement

Country of Publication:: United States

Language:: English

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A Spherical Plasma Dynamo Experiment Spence, E. J.; Reuter, K.; Forest, C. B. arXiv https://doi.org/10.48550/arxiv.0901.3406	text	January 2009
The Madison plasma dynamo experiment: a facility for studying laboratory plasma astrophysics Cooper, C. M.; Wallace, J.; Brookhart, M. arXiv https://doi.org/10.48550/arxiv.1310.8637	text	January 2013
Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection Singh, Chandra B.; Mizuno, Yosuke; Pino, Elisabete M. de Gouveia Dal arXiv https://doi.org/10.48550/arxiv.1603.03276	text	January 2016
The Topology of Canonical Flux Tubes in Flared Jet Geometry Lavine, Eric Sander; You, Setthivoine arXiv https://doi.org/10.48550/arxiv.1701.01756	text	January 2017
Laboratory Astrophysics and Collimated Stellar Outflows: The Production of Radiatively Cooled Hypersonic Plasma Jets Lebedev, S. V.; Chittenden, J. P.; Beg, F. N. arXiv https://doi.org/10.48550/arxiv.astro-ph/0108067	text	January 2001
Origin of Galactic and Extragalactic Magnetic Fields Widrow, Lawrence M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0207240	text	January 2002
Relativistic Poynting Jets from Accretion Disks Lovelace, Richard V. E.; Romanova, Marina M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0401481	text	January 2004
Magnetic Fields in Stellar Jets Hartigan, P.; Frank, A.; Varniere, P. arXiv https://doi.org/10.48550/arxiv.astro-ph/0702174	text	January 2007
Instability of toroidal magnetic field in jets and plerions Begelman, Mitchell C. arXiv https://doi.org/10.48550/arxiv.astro-ph/9708142	text	January 1997
Formation and Primary Heating of The Solar Corona - Theory and Simulation Mahajan, Swadesh M.; Miklaszewski, Ryszard; Nikol'skaya, Kommunela I. arXiv https://doi.org/10.48550/arxiv.physics/0009086	text	January 2000
Why current-carrying magnetic flux tubes gobble up plasma and become thin as a result Bellan, P. M. arXiv https://doi.org/10.48550/arxiv.physics/0301037	text	January 2003
On the jets, kinks, and spheromaks formed by a planar magnetized coaxial gun Hsu, S. C.; Bellan, P. M. arXiv https://doi.org/10.48550/arxiv.physics/0411089	text	January 2004

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Helical Shear-Flow Stabilization of an Astrophysically Relevant Laboratory Plasma Jet Lavine, Eric Sander; You, Setthivoine Physical Review Letters, Vol. 123, Issue 14 https://doi.org/10.1103/physrevlett.123.145002	journal	October 2019
Exploring astrophysics-relevant magnetohydrodynamics with pulsed-power laboratory facilities Lebedev, S. V.; Frank, A.; Ryutov, D. D. Reviews of Modern Physics, Vol. 91, Issue 2 https://doi.org/10.1103/revmodphys.91.025002	journal	April 2019

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