Plasma Physics Colloquium

Date: October 30, 2009 from 2:00 pm to 3:00 pm EDT
Location: Columbia University
Morningside Campus
S.W. Mudd, Room 214
Contact: For further information regarding this event, please contact APAM Department by sending email to seasinfo.apam@columbia.edu or by calling 212-854-4457.
Info: Click Here to Visit Website.

Deepak Kumar, California Institute of Technology
"Experimental investigations of magnetohydrodynamic plasma jets"

Spheromak formation consists of a series of dynamic steps whereby highly localized plasma near the electrodes evolves towards a Taylor state equilibrium. The dynamical evolution stage has been modeled as a series of equilibrium states in the past. However, the experiments at the Caltech spheromak facility have revealed that unbalanced J x B forces drive non- equilibrium Alfvenic flows during these preliminary stages.

The Caltech spheromak experiment uses co-planar electrodes to produce a collimated plasma jet flowing away from the electrodes. The jet formation stage precedes the spheromak formation and serves as a mechanism for feeding particles, magnetic helicity, energy and toroidal flux into the system. I will present detailed density and flow velocity measurements of hydrogen and deuterium plasma jets. These measurements show that the jets are extremely dense with  B thermal - 1. Furthermore, the flow velocity of the jets is Alfvenic with respect to the the toroidal magnetic field produced by the axial current within the plasma. I will also describe a magnetohydrodynamics (MHD) model which successfully predicts the e ffect of plasma current on the jet's density and  flow velocity.

These laboratory jets are often compared to collimated bipolar astrophysical jets associated with active galaxies, young stellar objects, etc. I will conclude the talk by highlighting the similarities and di fferences between these laboratory jets and some common models for the astrophysical jets.

Host: Michael Mauel


 

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