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Monte Carlo simulation of high power microwave window breakdown at atmospheric conditions
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10.1063/1.2388877
/content/aip/journal/apl/89/20/10.1063/1.2388877
http://aip.metastore.ingenta.com/content/aip/journal/apl/89/20/10.1063/1.2388877
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

Electron cloud formation in an air environment with 1600 seed electrons at . The bottom of each image coincides with the dielectric surface. Electric field’s rise time is identical to that of the experimental setup.

Image of FIG. 2.
FIG. 2.

Normalized electric field vs delay time multiplied by pressure in both air (gray diamonds) and nitrogen (gray squares) environments under ideal excitation at gigahertz frequencies. The graph also shows volume breakdown curve from Gould and Roberts (black line).

Image of FIG. 3.
FIG. 3.

Normalized electric field vs delay time multiplied by pressure in air. The graph shows data collected on the current test setup (gray boxes), simulated data (black diamonds), and a curve fit of all the experimental data in air (light gray line).

Image of FIG. 4.
FIG. 4.

Flashover delay times for both experimental (open symbols) and simulated (closed symbols) setups vs background pressure.

Image of FIG. 5.
FIG. 5.

Comparison of EEDF’s for air and nitrogen environments generated by the simulation, EEDF’s are averaged over two periods for conditions with zero net electron gain (nitrogen: 20 electrons and oxygen: 1600 electrons).

Image of FIG. 6.
FIG. 6.

Dependence of flashover delay time on frequency of applied field. All calculations performed at with a maximum applied field amplitude.

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/content/aip/journal/apl/89/20/10.1063/1.2388877
2006-11-14
2014-04-20
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Monte Carlo simulation of high power microwave window breakdown at atmospheric conditions
http://aip.metastore.ingenta.com/content/aip/journal/apl/89/20/10.1063/1.2388877
10.1063/1.2388877
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