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My research focuses on understanding how electrical currents (and hence magnetic fields) are generated in fusion plasmas and in turbulent flows of liquid metals. I am an experimentalist, which means that I build devices and carry out experiments on these devices to answer fundamental questions like:
Where do the magnetic fields found on planets and stars come from?
How can magnetic fields be used to confine hot plasmas and create a burning star on Earth?
One of my experiments, the Madison Dynamo Experiment, uses a 300 gallon liquid sodium facility to study how magnetic fields are generated in turbulent flows of liquid metal (like the conditions found in the core of the Earth). The experiment uses two 100 Hp motors to drive flows in a spherical container that are expected to lead to self-generation of magnetic fields. My fusion research is carried out on the Madison Symmetric Torus where confinement and stability of a toroidal magnetic configuration known as the reversed field pinch is carried out. My research on MST focuses on studies of current transport, electron heat transport and microwave heating of electrons (to drive current) in the RFP geometry. I recently spent a year on sabbatical in Germany working on the ASDEX-U tokamak, studying similar questions on a large tokamak. I also direct research on a smaller, basic plasma physics experiment investigating the MHD stability of a line-tied screw pinch plasma. The experiment was constructed to test the hypothesis that two conducting shells, one rotating with respect to the first, can stabilize current driven kink modes in fusion plasmas. The experiment is also providing data about stability a geometry which is strikingly similar to the geometry of solar eruptions (solar flares or coronal mass ejections).
Some Recent Publications
Acknowledgements
My work has been generously supported by
| UNIVERSITY OF WISCONSIN || PHYSICS DEPARTMENT || PLASMA PHYSICS GROUP || PLASMA RESEARCH || OTHER LINKS |