2014
DOI: 10.15407/rpra19.01.081
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Cryogenic Receiving Focal Unit for Telescopes of Radiointerferometric Complex of New Generation

Abstract: Приводятся результаты синтеза, конструирования и испытаний экспериментального образца криогенного приемного фокального блока (КПФБ) для радиотелескопов российского радиоинтерферометрического комплекса нового поколения. Радиотелескопы комплекса спроектированы для приема сигналов космических радиоисточников одновременно в S, X и Ka диапазонах и частично совместимы с радиотелескопами перспективной глобальной геодезической сети VLBI2010. Обсуждаются принятые технические решения ключевых узлов КПФБ и приводятся осн… Show more

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Cited by 5 publications
(1 citation statement)
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“…E.g., development of the next generation navigation, positioning, and telecommunication systems like the Very Long Baseline Interferometry (VLBI) Global Observing System (VGOS, formerly VLBI2010) requires small area ( 12 m) antenna dishes containing highly sensitive detectors operating within a broad frequency band 2-18 GHz and at higher radiation frequencies but blocking the influence of the background radiation through the input window on the lowtemperature detector devices used in these systems. 9,10 Reducing the dish area according to VLBI2010 conditions requires development of extremely sensitive (gaining background limited performance in the microwave spectral region) low-temperature detectors ensuring high qualitative faint signal detection and their handling against the background radiation.…”
Section: Introductionmentioning
confidence: 99%
“…E.g., development of the next generation navigation, positioning, and telecommunication systems like the Very Long Baseline Interferometry (VLBI) Global Observing System (VGOS, formerly VLBI2010) requires small area ( 12 m) antenna dishes containing highly sensitive detectors operating within a broad frequency band 2-18 GHz and at higher radiation frequencies but blocking the influence of the background radiation through the input window on the lowtemperature detector devices used in these systems. 9,10 Reducing the dish area according to VLBI2010 conditions requires development of extremely sensitive (gaining background limited performance in the microwave spectral region) low-temperature detectors ensuring high qualitative faint signal detection and their handling against the background radiation.…”
Section: Introductionmentioning
confidence: 99%