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The S/X/Ka Receiving System for Radio Telescope RT-13 of the “Quasar” VLBI Network

V. Chernov, A. Evstigneev, O. Evstigneeva, D. Ivanov, A. Ipatov, I. Ipatova, E. Khvostov, A. Lavrov, V. Mardyshkin, I. Pozdnyakov, Y. Vekshin, M. Zotov

Труды ИПА РАН, вып. 41, 79–84 (2017)

Ключевые слова: VLBI, geodesy, tri-band receiver, 13.2 antenna

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IAA RAS has already made the radio interferometer which consists of two radio telescopes with dish diameter of 13.2 m. Each radio telescope is equipped with a specially designed receiving system. The main feature of this system is the cryogenic receiving unit that includes cooled triband feed and low-noise amplifiers (LNA). Feed design allows to receive signals in three frequency bands S (2.2–2.6 GHz), X (7.0–9.5 GHz) and Ka (28–34 GHz) for both circular polarizations (LCP and RCP) simultaneously.

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V. Chernov, A. Evstigneev, O. Evstigneeva, D. Ivanov, A. Ipatov, I. Ipatova, E. Khvostov, A. Lavrov, V. Mardyshkin, I. Pozdnyakov, Y. Vekshin, M. Zotov. The S/X/Ka Receiving System for Radio Telescope RT-13 of the “Quasar” VLBI Network // Труды ИПА РАН. — 2017. — Вып. 41. — С. 79–84.

@article{chernov2017,
  abstract = {IAA RAS has already made the radio interferometer which consists of two radio telescopes with dish diameter of 13.2 m. Each radio telescope is equipped with a specially designed receiving system. The main feature of this system is the cryogenic receiving unit that includes cooled triband feed and low-noise amplifiers (LNA). Feed design allows to receive signals in three frequency bands S (2.2–2.6 GHz), X (7.0–9.5 GHz) and Ka (28–34 GHz) for both circular polarizations (LCP and RCP) simultaneously.},
  author = {V. Chernov and A. Evstigneev and O. Evstigneeva and D. Ivanov and A. Ipatov and I. Ipatova and E. Khvostov and A. Lavrov and V. Mardyshkin and I. Pozdnyakov and Y. Vekshin and M. Zotov},
  issue = {41},
  journal = {Труды ИПА РАН},
  keyword = {VLBI, geodesy, tri-band receiver, 13.2 antenna},
  pages = {79--84},
  title = {The S/X/Ka Receiving System for Radio Telescope RT-13 of the “Quasar” VLBI Network},
  url = {http://iaaras.ru/library/paper/1709/},
  year = {2017}
}

TY  - JOUR
TI  - The S/X/Ka Receiving System for Radio Telescope RT-13 of the “Quasar” VLBI Network
AU  - Chernov, V.
AU  - Evstigneev, A.
AU  - Evstigneeva, O.
AU  - Ivanov, D.
AU  - Ipatov, A.
AU  - Ipatova, I.
AU  - Khvostov, E.
AU  - Lavrov, A.
AU  - Mardyshkin, V.
AU  - Pozdnyakov, I.
AU  - Vekshin, Y.
AU  - Zotov, M.
PY  - 2017
T2  - Труды ИПА РАН
IS  - 41
SP  - 79
AB  - IAA RAS has already made the radio interferometer which consists of
two radio telescopes with dish diameter of 13.2 m. Each radio
telescope is equipped with a specially designed receiving system. The
main feature of this system is the cryogenic receiving unit that
includes cooled triband feed and low-noise amplifiers (LNA). Feed
design allows to receive signals in three frequency bands S (2.2–2.6
GHz), X (7.0–9.5 GHz) and Ka (28–34 GHz) for both circular
polarizations (LCP and RCP) simultaneously.
UR  - http://iaaras.ru/library/paper/1709/
ER  -