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32nd European Microwave Conference, 2002 2002
DOI: 10.1109/euma.2002.339415
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A 2-18GHz ESM Receiver Front-End

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Cited by 8 publications
(8 citation statements)
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“…(1) and (2). The combined NF could be improved by approximately 0.85 dB over the NF in a single path.…”
Section: Noise Figurementioning
confidence: 70%
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“…(1) and (2). The combined NF could be improved by approximately 0.85 dB over the NF in a single path.…”
Section: Noise Figurementioning
confidence: 70%
“…Practical solutions must not only meet the electrical specifications but also be compact and immune to microphonic effects and thermal fluctuations. A wideband receiver module was designed to meet these requirements and to provide matching phase and amplitude [2]. A wideband receiver that is located next to an antenna requires low noise figures (NFs) because very low input signals are received by the antenna.…”
Section: Introductionmentioning
confidence: 99%
“…In addition, each component is connected using a microstrip line or a short RF cable for fabrication and testing. Additional tuning is also required to reduce mutual mismatching [2][3][4]. As previously discussed, the broadband switching matrix module connected to the rear end of the antenna in the electronic support equipment system is a key element determining the overall system performance.…”
Section: Introductionmentioning
confidence: 99%
“…As currently existing wideband receivers made of single modules can only receive signals in bands up to 2-18 GHz, they are insufficient for high-frequency signals in millimeter-wave bands. In addition, as the local oscillator (LO) necessary for frequency conversion is not implemented in their receiver modules [7], but provided separately with converted frequencies from ES system devices, the phase noise characteristics of the entire receivers are dependent on the performance of other devices, and the size of the entire system increases owing to the separate LO module.…”
Section: Introductionmentioning
confidence: 99%
“…First, the ultra-wideband input frequency range of 18-40 GHz were divided into two bands using 18-26 GHz (Band A) and 26-40 GHz (Band B) band pass filters and these were applied to the frequency mixer input. The designed frequency spectra were such that there was no secondary harmonic component in each band, thereby preventing spurious signals from appearing in the intermediate frequencies (IF,(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)(14)(15)(16)(17)(18).…”
Section: Introductionmentioning
confidence: 99%