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Laboratory investigations of space-relevant, self-organizing MHD plasmas

Bellan, P. M. (2007) Laboratory investigations of space-relevant, self-organizing MHD plasmas. In: Turbulence and Nonlinear Processes in Astrophysical Plasmas: 6th Annual International Astrophysics Conference, Oahu, Hawaii, 16-22 March 2007. AIP Conference Proceedings. No.932. American Institute of Physics , Melville, NY, pp. 359-368. ISBN 978-0-7354-0443-4. https://resolver.caltech.edu/CaltechAUTHORS:BELaipcp07

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Abstract

Pulsed power technology is used to produce transient MHD-regime plasmas having topology and dynamical behavior similar to solar and astrophysical plasmas. These plasmas are not exact scale models, but exhibit many behaviors similar to actual solar and astrophysical plasmas, for example, collimation, kinking, and jet motion. These plasmas can also display an interaction between MHD-dynamics and non-MHD particle orbit behavior.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.2778986PublisherArticle
https://doi.org/10.1063/1.2778986DOIUNSPECIFIED
https://doi.org/10.1063/1.2778986DOIUNSPECIFIED
ORCID:
AuthorORCID
Bellan, P. M.0000-0002-0886-8782
Additional Information:© 2007 American Institute of Physics This paper summarizes work done in collaboration with J. F. Hansen, S. C. Hsu, S. K. P. Tripathi, G. S. Yun, S. You, A. Moser, and E. Stenson. Supported in part by US DOE and NSF.
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)UNSPECIFIED
NSFUNSPECIFIED
Subject Keywords:astrophysical plasma; plasma magnetohydrodynamics; solar corona; coronal loops; spheromaks
Series Name:AIP Conference Proceedings
Issue or Number:932
Record Number:CaltechAUTHORS:BELaipcp07
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:BELaipcp07
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:8659
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:03 Sep 2007
Last Modified:02 Oct 2019 23:53

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