Fine structure of objects with active nuclei and superluminal component separation velocities

Костенко, В. И.; Matveenko, L. I.; Moiseev, I. G.

doi:10.1070/pu1982v025n02abeh004509

Cited by 2 publications

(3 citation statements)

References 2 publications

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“…The accuracy of the surface was enough for the sub-mm band. The antenna had the Cassegrain illumination with a secondary mirror designed that could compensate a change of focal position and the extra pointing of antenna electrical axis (Kostenko & Matveenko 1982). This project had broad international cooperation.…”

Section: Simeiz-haystack H 2 O Experimentsmentioning

confidence: 99%

Early VLBI in the USSR

Matveenko

2007

Astron Nachr

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This article gives story of interferometer with independent elements (Very Long Baseline Interferometer) in Russia. At the end of February 1962 the author discussed with G.Ya. Gus'kov, DSN Station, Evpatorija a new type of radio interferometer and proposed an experiment between two DSN stations. In September 1962 he reported the new method and proposed a VLBI experiment at seminar of Radio Astronomical Laboratory, Pushino, and then at a seminar of Astronomical Institute GAISH which recommended to take out a Patent. In December GAISH sent documents to the Patent Bureau. In summer 1963 the author discussed with B. Lovell in Evpatorija the VLBI method of and we signed memorandum an Ev‐JB experiment at λ = 32 cm. In December 1963 the Patent Bureau permitted publication, and the paper was sent to Radiofizika. Really VLBI in the USSR began with the proposal of M. Cohen and K. Kellermann, February 1968, to do an experiment between 22‐m antenna Pushino and 43‐m Green Bank. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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Section: Simeiz-haystack H 2 O Experimentsmentioning

confidence: 99%

Early VLBI in the USSR

Matveenko

2007

Astron Nachr

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“…The accuracy of the surface was good enough for the sub-mm band. The secondary mirror could compensate a change of the focal position and the fine pointing of the antenna [17]. The apogee of 20,000 km was determined by the high-energy particles and non-uniform gravity field of the Earth, the perigee of 70,000 km by the space radio telescope sensitivity.…”

Section: Observations Cr-hstmentioning

confidence: 99%

“…The thermal plasma was detected from absorption recombination radio lines [17]. The surrounded thermal plasma determines the rotation measure [14].…”

Section: Pos(rts2012)004mentioning

confidence: 99%

Early VLBI in the USSR

Matveenko¹

2012

Proceedings of Resolving the Sky - Radio Interferometry: Past, Present and Future — PoS(RTS2012)

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Fine structure of objects with active nuclei and superluminal component separation velocities

Cited by 2 publications

References 2 publications

Early VLBI in the USSR

Early VLBI in the USSR

Early VLBI in the USSR

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