COLLOQUIUM: Laboratory Study of Magnetic Reconnection: Recent Discoveries on MRX
Magnetic reconnection is a phenomenon of nature in which magnetic field lines change their topology in plasma and convert magnetic energy to particles by acceleration and heating. It is one of the most fundamental processes at work in laboratory and astrophysical plasmas. Magnetic reconnection occurs everywhere: in solar flares; coronal mass ejections; the earth’s magnetosphere; in the star forming galaxies; and in plasma fusion devices. This talk focuses on recent discoveries in the fundamental research of magnetic reconnection on Magnetic Reconnection Experiment (MRX) and its application to space astrophysical plasmas. We compare the experimental results with those from theory and numerical simulations. The collaboration between space and laboratory scientists on reconnection research has recently reached a point where we can compare measurements of the reconnection layer profile in detail with support from numerical simulations. In spite of the huge difference in physical scales, we find remarkable commonalities in the features of the magnetic reconnection region in laboratory and space-astrophysical plasmas.
Recently the physics of the reconnection layer has moved forward through understanding of the local physics of collision-less magnetic reconnection. Two-fluid dynamics have been verified through experimental identification of both the ion and electron diffusion layers. The measured in-plane plasma potential profile, which is established by electrons accelerated around the electron diffusion region, shows a saddle-shaped structure that is wider and deeper towards the outflow direction. This potential structure ballistically accelerates ions near the separatrices toward the outflow direction. Ions are heated as they travel into the high pressure downstream region. The effects of guide field on reconnection have also been studied by systematically varying the applied guide field to values much greater than the reconnecting field. Guide field is observed to significantly decrease the reconnection speed and the quantitative relationship of reconnection rate with guide field will be presented.
The Princeton Plasma Physics Laboratory 2017-2018 Colloquium Committee is comprised of the following people. Please feel free to contact them by e-mail regarding any possible speakers or topics for future colloquia.
- Carol Ann Austin 609-243-2484
Princeton Plasma Physics Laboratory is a U.S. Department of Energy national laboratory managed by Princeton University.
© 2018 Princeton Plasma Physics Laboratory. All rights reserved.