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Laboratory simulations of astrophysical jets and solar coronal loops: new results View all abstracts by submitter

Paul Bellan   Submitted: 2010-01-28 16:28

An experimental program underway at Caltech has produced plasmas where the shape is neither fixed by the vacuum chamber nor fixed by an external coil set, but instead is determined by self-organization. The plasma dynamics is highly reproducible and so can be studied in considerable detail even though the morphology of the plasma is both complex and time-dependent. A surprising result has been the observation that self-collimating MHD-driven plasma jets are ubiquitous and play a fundamental role in the self-organization. The jets can be considered lab-scale simulations of astrophysical jets and in addition are intimately related to solar coronal loops. The jets are driven by the combination of the axial component of the JxB force and the axial pressure gradient resulting from the non-uniform pinch force associated with the flared axial current density. Behavior is consistent with a model showing that collimation results from axial non-uniformity of the jet velocity. In particular, flow stagnation in the jet frame compresses frozen-in azimuthal magnetic flux, squeezes together toroidal magnetic field lines, thereby amplifying the embedded toroidal magnetic field, enhancing the pinch force, and hence causing collimation of the jet.

Authors: P. M. Bellan, D. Kumar, E. V. Stenson, S. K. P. Tripathi, G. S. Yun, and A. L. Moser
Projects: None

Publication Status: AIP Conf. Proc. (submitted), paper presented at Como Italy Symposium 2009
Last Modified: 2010-01-29 09:59
Go to main E-Print page  Evolution of Solar Magnetic Field and Associated Multiwavelength Phenomena:  Flare Events on 2003 November 20  The spatial damping of magnetohydrodynamic waves in a flowing partially ionised prominence plasma  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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