Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics

We proposed tapered pinch discharge as a measure to conduct laboratory astrophysics experiments. Basic behaviors of the plasma have been characterized using a prototype device. Results show that the plasma flux and velocity depend on initial gas density, discharge current and taper geometry. Those b...

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Main Authors: Adachi K., Nakajima M., Kawamura T., Horioka K.
Format: Article
Language:English
Published: EDP Sciences 2013-11-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20135910003
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author Adachi K.
Nakajima M.
Kawamura T.
Horioka K.
author_facet Adachi K.
Nakajima M.
Kawamura T.
Horioka K.
author_sort Adachi K.
collection DOAJ
description We proposed tapered pinch discharge as a measure to conduct laboratory astrophysics experiments. Basic behaviors of the plasma have been characterized using a prototype device. Results show that the plasma flux and velocity depend on initial gas density, discharge current and taper geometry. Those behaviors can be illustrated with a simple model considering the pinching dynamics of the current sheet based on a 1 dimensional (1-D) equation of motion. Achievable value of the tapered pinch plasma is estimated and compared with required plasma parameters based on scaling parameters for laboratory astrophysics.
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spelling doaj.art-3086430d384a475c8ddbf33ba2e2e1482022-12-21T23:22:34ZengEDP SciencesEPJ Web of Conferences2100-014X2013-11-01591000310.1051/epjconf/20135910003Formation of dense, electromagnetically accelerated plasma for laboratory astrophysicsAdachi K.Nakajima M.Kawamura T.Horioka K.We proposed tapered pinch discharge as a measure to conduct laboratory astrophysics experiments. Basic behaviors of the plasma have been characterized using a prototype device. Results show that the plasma flux and velocity depend on initial gas density, discharge current and taper geometry. Those behaviors can be illustrated with a simple model considering the pinching dynamics of the current sheet based on a 1 dimensional (1-D) equation of motion. Achievable value of the tapered pinch plasma is estimated and compared with required plasma parameters based on scaling parameters for laboratory astrophysics.http://dx.doi.org/10.1051/epjconf/20135910003
spellingShingle Adachi K.
Nakajima M.
Kawamura T.
Horioka K.
Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
EPJ Web of Conferences
title Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
title_full Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
title_fullStr Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
title_full_unstemmed Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
title_short Formation of dense, electromagnetically accelerated plasma for laboratory astrophysics
title_sort formation of dense electromagnetically accelerated plasma for laboratory astrophysics
url http://dx.doi.org/10.1051/epjconf/20135910003
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AT nakajimam formationofdenseelectromagneticallyacceleratedplasmaforlaboratoryastrophysics
AT kawamurat formationofdenseelectromagneticallyacceleratedplasmaforlaboratoryastrophysics
AT horiokak formationofdenseelectromagneticallyacceleratedplasmaforlaboratoryastrophysics