2013 International Kharkov Symposium on Physics and Engineering of Microwaves, Millimeter and Submillimeter Waves 2013
DOI: 10.1109/msmw.2013.6622166
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Experience in developing Ka-band waveguide filter with HTS E-plane insert

Abstract: To improve the performance of receivers of both satellite microwave links and radio telescopes, developing the bandpass filter (BPF) with low insertion loss is the actual task. The filter is installed at LNA input and jointly cooled to cryogenic temperatures. Every 0.1 dB insertion loss in BPF increases the receiving system noise temperature for 7-7.5 K at 300 K, which should be considered as notable addition, if we consider that noise temperature of the modern transistor amplifiers in the Ka range is about 60… Show more

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Cited by 4 publications
(1 citation statement)
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“…These rectangular apertures have comb-like periodic ridges on upper and lower edges. The configuration of the septum insert creates necessary periodic boundary conditions required for slow wave propagation within the resonators [7][8][9][10], which results in a physically smaller waveguide but with improved stopband and rejection characteristics.…”
Section: E-plane Waveguide Filter Structurementioning
confidence: 99%
“…These rectangular apertures have comb-like periodic ridges on upper and lower edges. The configuration of the septum insert creates necessary periodic boundary conditions required for slow wave propagation within the resonators [7][8][9][10], which results in a physically smaller waveguide but with improved stopband and rejection characteristics.…”
Section: E-plane Waveguide Filter Structurementioning
confidence: 99%