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PHYSICS DEPARTMENT COLLOQUIUM
Gas Breakdown in the Sub-nanosecond Regime
Dr. Hermann G. Krompholz
Department of Electrical and Computer Engineering
Center for Pulsed Power and Power Electronics
Texas Tech University
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The understanding of fast gas breakdown is of relevance for
new developments in pulsed power switching, ultra-wide-band radar, and
electronic countermeasures. Physical mechanisms for breakdown in the
sub-nanosecond regime, which is associated with voltages far higher than
voltages for standard conditions, have been explored only recently. New
phenomena include non-steady state distribution functions, non-local
processes, and runaway electrons. For applications of fast breakdown,
general scaling laws, such as statistical and formative time delays, and
breakdown voltages as a function of gas, pressure, gap geometry etc., are
needed, along with information about the relevant discharge properties. For
gap distances from 1 to 10 mm, voltages from 50 to 300 kV, voltage risetimes
< 200 ps, and pressures up to one atmosphere in air, and in argon as a model
gas with well known cross-sections, the basic breakdown phenomenology is
investigated. Voltage and current measurements with resolutions of 25 to 50
ps reveal the temporal characteristics of the discharge. X-ray diagnostics
with rough spectral resolution using absorption of different metal foils
yields statements about the energy distribution of runaway electrons, which
extends to the equivalent charging voltage even for atmospheric pressure.
Streak camera pictures with 5 ps resolution show a multi-channel development
of the discharge, with an ionization zone limited to a narrow layer in front
of the cathode. Simple analytical calculations valid for the high-energy
portion of the electrons, and detailed three-dimensional Monte-Carlo
simulations allow, together with the experimental results, a detailed
quantitative description of the discharge physics and the scaling laws
relevant for applications.
Thursday, April 17, 2008
3:30 P.M. in Sc 234
Refreshments at 3:00 in Sc 103
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