Author: Phair, L.
Paper Title Page
THA3 Waveguide DC breaks with optimized impedance matching networks 162
 
  • M.K. Covo, B. Ninemire, D.S. Todd, D.Z. Xie, J. Cruz Duran, J.Y. Benitez, J.P. Garcia, L. Phair, M.B. Johnson, P. Bloemhard
    LBNL, Berkeley, CA, USA
 
  A custom 18 GHz waveguide DC break with a built-in impedance matching network, consisting of two inductive irises adjacent to a capacitive gap assembled around a quartz disk, was built for VENUS and simulated using the ANSYS High Frequency Structure Simulator, a finite element analysis tool. The DC break effectively doubled the RF power available for plasma production at the secondary frequency of 18 GHz while maintaining a DC isolation of 32 kV. Measurements of the forward and reflected power coefficients, performed with a network analyzer, showed excellent agreement with the simulations [1]. Additionally, an extended study was conducted to tailor the frequencies of 28, 35, and 45 GHz using WR-34, WR-28, and WR-22 waveguides with built-in impedance matching networks, aiming to predict performance for our upcoming 4th generation low-power, multi-frequency operation of the MARS-D ion source.
[1] M. Kireeff Covo et al., “Inductive Iris Impedance Matching Network for a Compact Waveguide DC Break”, IEEE Transactions on Microwave Theory and Techniques, early access 2024. doi:10.1109/TMTT.2024.3409470.
 
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DOI • reference for this paper ※ doi:10.18429/JACoW-ECRIS2024-THA3  
About • Received ※ 13 September 2024 — Revised ※ 09 October 2024 — Accepted ※ 30 January 2025 — Issued ※ 18 May 2025
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