Abstract
Space and phase resolved optical emission spectroscopy and numerical simulations are employed to investigate the excitation dynamics of a radio-frequency-driven microatmospheric pressure plasma jet. Different power coupling modes can be identified by characteristic structures obtained from the spectroscopic measurements. Numerical results from a 1-D fluid code with semikinetic treatment of the electrons show very good agreement with the experimental results.
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Schedule a callMore From: IEEE transactions on plasma science. IEEE Nuclear and Plasma Sciences Society
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