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Dual band S/X crioelectronic block of radio telescope

V. V. Mardyshkin, I. A. Pozdnyakov, E. Y. Khvostov, V. C. Chernov

Transactions of IAA RAS, issue 24, 140–143 (2012)

Keywords: feed systems of radio telescopes, cryoelectronic focal unit, noise parameters, noise temperature

Abstract

In accordance with the recommendations of the IVS Committee VLBI2010, radio telescopes of the new generation VLBI networks are to receive simultaneous signals in several frequency windows within the frequency band of 2-14 GHz. Feed systems of the radio telescopes, meeting these recommendations, typically require cooling to temperatures of hydrogen level [1]. In the article a cryoelectronic unit that provides cooling the dual band feed and a few low-noise amplifiers is presented.

Citation

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V. V. Mardyshkin, I. A. Pozdnyakov,  E. Y. Khvostov,  V. C. Chernov. Dual band S/X crioelectronic block of radio telescope // Transactions of IAA RAS. — 2012. — Issue 24. — P. 140–143.

@article{mardyshkin2012,
  abstract = {In accordance with the recommendations of the IVS Committee VLBI2010, radio telescopes of the new generation VLBI networks are to receive simultaneous signals in several frequency windows within the frequency band of 2-14 GHz. Feed systems of the radio telescopes, meeting these recommendations, typically require cooling to temperatures of hydrogen level [1]. In the article a cryoelectronic unit that provides cooling the dual band feed and a few low-noise amplifiers is presented.},
  author = {V.~V. Mardyshkin and I.~A. Pozdnyakov and E.~Y. Khvostov and V.~C. Chernov},
  issue = {24},
  journal = {Transactions of IAA RAS},
  keyword = {feed systems of radio telescopes, cryoelectronic focal unit, noise parameters, noise temperature},
  pages = {140--143},
  title = {Dual band S/X crioelectronic block of radio telescope},
  url = {http://iaaras.ru/en/library/paper/839/},
  year = {2012}
}

TY  - JOUR
TI  - Dual band S/X crioelectronic block of radio telescope
AU  - Mardyshkin, V. V.
AU  - Pozdnyakov, I. A.
AU  - Khvostov, E. Y.
AU  - Chernov, V. C.
PY  - 2012
T2  - Transactions of IAA RAS
IS  - 24
SP  - 140
AB  - In accordance with the recommendations of the IVS Committee VLBI2010,
radio telescopes of the new generation VLBI networks are to receive
simultaneous signals in several frequency windows within the
frequency band of 2-14 GHz. Feed systems of the radio telescopes,
meeting these recommendations, typically require cooling to
temperatures of hydrogen level [1]. In the article a cryoelectronic
unit that provides cooling the dual band feed and a few low-noise
amplifiers is presented.
UR  - http://iaaras.ru/en/library/paper/839/
ER  -