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13 Nov 2006

Volume 89, Issue 20, Articles (20xxxx)

Issue Cover Spotlight Figure

Appl. Phys. Lett. 89, 202101 (2006); http://dx.doi.org/10.1063/1.2388049 (3 pages)

J. H. Lee, Zh. M. Wang, N. W. Strom, Yu. I. Mazur, and G. J. Salamo
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Monte Carlo simulation of high power microwave window breakdown at atmospheric conditions

John T. Krile, Andreas A. Neuber, Hermann G. Krompholz, and Thomas L. Gibson

Appl. Phys. Lett. 89, 201501 (2006); http://dx.doi.org/10.1063/1.2388877 (3 pages) | Cited 19 times

Online Publication Date: 14 November 2006

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A Monte Carlo-type electron motion simulation program was developed to calculate the increasing electron density for pulsed high power microwave window flashover in air and nitrogen at atmospheric pressures, i.e., >90 torr. Through comparison of experimental and simulated results several processes such as flashover delay time’s strong dependence on pressure and the lack of significant surface charge buildup have been confirmed. The quantitative agreement of the code results with the experiment is a clear step towards predicting high power microwave flashover under a wide range of atmospheric conditions as well as for different gases and more complex window geometries.
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52.80.Pi High-frequency and RF discharges
52.65.Pp Monte Carlo methods
52.25.Fi Transport properties

Method to determine argon metastable number density and plasma electron temperature from spectral emission originating from four 4p argon levels

Davide Mariotti, Yoshiki Shimizu, Takeshi Sasaki, and Naoto Koshizaki

Appl. Phys. Lett. 89, 201502 (2006); http://dx.doi.org/10.1063/1.2390631 (3 pages) | Cited 15 times

Online Publication Date: 15 November 2006

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A simple model and method is proposed here to determine argon metastable number densities and electron temperature with the assumption of a Maxwell-Boltzmann electron energy distribution. This method is based on the availability of experimental relative emission intensities of only four argon lines that originate from any of the 4p argon levels. The proposed model has a relatively wide range of validity for laboratory plasmas that contain argon gas and can be a valuable tool for the emerging field of atmospheric microplasmas, for which diagnostics is still limited.
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52.25.Os Emission, absorption, and scattering of electromagnetic radiation
52.25.Fi Transport properties
52.50.Dg Plasma sources
52.70.Kz Optical (ultraviolet, visible, infrared) measurements
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