skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Steady supersonically rotating plasmas in the Maryland Centrifugal Experiment

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.1896954· OSTI ID:20736564
; ; ; ; ; ; ; ;  [1]
  1. University of Maryland, College Park, Maryland 20742-3511 (United States)

The Maryland Centrifugal Experiment MCX [R. F. Ellis, A. B. Hassam, and S. Messer, Phys. Plasmas 8, 2057 (2000)] studies supersonic rotation and enhanced confinement produced by the application of an electric field perpendicular to an axial confining mirror magnetic field; radial shear in the rotation is predicted to stabilize magnetohydrodynamic (MHD) interchange modes. The MCX mirror field is 2.6 m in length, maximum mirror field 1.9 T, maximum midplane field 0.33 T; an inner coaxial core is driven by a 10 KV capacitor bank, producing the radial electric field which drives azimuthal rotation. MCX produces high density (n>10{sup 20} m{sup -3}) fully ionized plasmas and has two operating modes. In the O (ordinary) mode the plasma rotates supersonically with azimuthal velocities in the range of 100 km/s for discharge times exceeding 8 ms. Ion temperatures are {approx}30 eV and momentum confinement times 100-200 {mu}s. Sonic Mach numbers (u{sub {phi}}/v{sub ti}) in the range 1-2 and Alfven Mach numbers (u{sub {phi}}/v{sub A}){approx}0.3 have been achieved for O mode discharges which remain steady for many milliseconds, much longer than MHD instability time scales; plasma lifetime is limited by the capacitance of the capacitor bank. MCX also has an enhanced mode of operation [higher rotation (HR) mode] with higher rotation velocities (>200 km/s), sonic Mach numbers greater than 3, Alfven Mach numbers >{approx}0.5, and momentum confinement times of several hundred microseconds. HR mode occurs at higher B fields and lower discharge currents but is transient, transitioning to O mode after a few milliseconds. Both O and HR mode show spectroscopic evidence of radial velocity shear sufficient to satisfy the simplest criterion for MHD stability, but both modes also show significant fluctuations on magnetic probes.

OSTI ID:
20736564
Journal Information:
Physics of Plasmas, Vol. 12, Issue 5; Other Information: DOI: 10.1063/1.1896954; (c) 2005 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
Country of Publication:
United States
Language:
English