Bulletin of the American Physical Society
77th Annual Gaseous Electronics Conference
Monday–Friday, September 30–October 4 2024; San Diego, California
Session GF2: Atmospheric Pressure Plasma Jets and Sources
10:00 AM–12:00 PM,
Friday, October 4, 2024
Room: Great Room 6-8
Chair: Andrew Tasman Powis, Princeton Plasma Physics Laboratory, Princeton, USA
Abstract: GF2.00007 : An Atmospheric Plasma Jet Array Based on the Evanescent-Mode Cavity Resonator Technology*
11:45 AM–12:00 PM
Presenter:
Kushagra Singhal
(University Of Toledo)
Authors:
Kushagra Singhal
(University Of Toledo)
Kazi Sadman S Kabir
(The University of Toledo, Toledo, Ohio)
Abbas Semnani
(University of Toledo)
This study introduces an array of plasma jets based on the SIW EVA cavity resonator technology, addressing the plasma jet volume limitation. The resonator, designed at a frequency of 910 MHz, extends the strong E-field region, resulting in a large volume of plasma. A uniform |E|-field on the order of 105 V/m is observed at the resonance frequency with a 1-W input power. To ensure uniform gas flow, the channel is carefully designed, breaking a large inflow into smaller outflow channels directed through the central post of the EVA resonator. The flow splitter is fabricated using a stereolithography (SLA)-based 3D printing technique. Experimental investigations utilize helium flow rates ranging from 1 to 20 slpm and input power levels ranging from 1 to 20 Watts. These findings provide a comprehensive understanding of the performance and behavior of this resonant microwave plasma jet array, offering practical insights for the design and optimization of plasma jet technology.
**This work was supported by the National Science Foundation (NSF) Grant No. 2102100.
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