Library · IAA RAS

Papers

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

Transactions of IAA RAS, issue 41, 79–84 (2017)

Keywords: VLBI, geodesy, tri-band receiver, 13.2 antenna

About the paper Full text

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.

Citation

Text

BibTeX

RIS

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 // Transactions of IAA RAS. — 2017. — Issue 41. — P. 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 = {Transactions of IAA RAS},
  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/en/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  - Transactions of IAA RAS
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/en/library/paper/1709/
ER  -