Zobrazeno 1 - 10
of 15
pro vyhledávání: '"V. V. Mardyshkin"'
Autor:
A. B. Ipatov, V. M. Chmil, V. M. Skresanov, D. V. Ivanov, V. V. Mardyshkin, V. K. Chernov, O. M. Pylypenko, A. A. Kirilenko
Publikováno v:
Radio Physics and Radio Astronomy, Vol 19, Iss 1, Pp 81-96 (2014)
Results of synthesis, design and tests of the experimental sample of cryogenic receiving focal unit (CRFU) for telescopes of Russian radio interferometric complex of new generation are presented. The radio telescopes can receive signals of space radi
Externí odkaz:
https://doaj.org/article/d91e6030cb0244a1beeb1e92fcdfc9cf
Autor:
M. G. Mingaliev, M. A. Kharinov, V. V. Mardyshkin, I. A. Ipatova, A. V. Ipatov, V. K. Konnikova
Publikováno v:
Astronomy Reports. 63:316-342
The results of observations of the blazar J1504+1029 (PKS 1502+106, OR 103), obtained in 2000–2018 on the RATAN-600 radio telescope of the Special Astrophysical Observatory at 2.3, 3.9 (4.7), 7.7 (8.2), 11.2, and 21.7 GHz and on the 32-m Zelenchuk
Autor:
A. V. Mel’nikov, N. Shuygina, E. Skurikhina, A. G. Mikhailov, M. Vasilyev, A. Dyakov, G. Ilin, D. A. Marshalov, V. Olifirov, A. I. Sal’nikov, V. V. Mardyshkin, D. Ivanov, I. Gayazov, I. A. Rakhimov, A. V. Ipatov, S. Kurdubov, Igor Surkis, A. Vytnov
Publikováno v:
Geodesy and Geodynamics, Vol 10, Iss 2, Pp 150-156 (2019)
This paper presents the past, present and future status of the Russian VLBI network “Quasar”. This network has been developed for at least 20 years by the Institute of Applied Astronomy of the Russian Academy of Sciences (IAA RAS). The equipment
Autor:
M. V. Sargsyan, Yu. V. Vekshin, A. I. Lapshin, E. Yu. Khvostov, Vitaliy Chernov, V. V. Mardyshkin, I. E. Arsaev, E. F. Yurchuk
Publikováno v:
Measurement Techniques. 61:284-289
The results of experimental investigations of the noise temperatures of the RT-13 radio telescope receiver system of a two-element radio interferometer with a very long baseline in the 2.2–2.6, 7.0–9.5, and 28–34 GHz frequency range are present
Autor:
M. G. Mingaliev, I. A. Ipatova, M. A. Kharinov, V. K. Konnikova, V. V. Mardyshkin, A. V. Ipatov, A. G. Gorshkov
Publikováno v:
Astronomy Reports. 62:183-199
The article presents the results of observations of the blazar 3C 454.3 (J2253+1608), obtained in 2010–2017 on the RATAN-600 radio telescope of the Special Astrophysical Observatory at 4.6, 8.2, 11.2, and 21.7 GHz and on the 32-m Zelenchuk and Bada
Autor:
I. E. Arsaev, E. Yu. Khvostov, Vitaliy Chernov, Yu. V. Vekshin, E. F. Yurchuk, M. V. Sargsyan, V. V. Mardyshkin, A. I. Lapshin
Publikováno v:
Izmeritel`naya Tekhnika. :51-54
Autor:
V. K. Konnikova, V. V. Mardyshkin, M. A. Kharinov, A. V. Ipatov, M. G. Mingaliev, A. G. Gorshkov
Publikováno v:
Astronomy Reports. 58:716-724
Results of the observations of the blazar J1159+2914 (S1156+295) in 2010–2013 are reported. The observations were carried out on the RATAN-600 radio telescope (Special Astrophysical Observatory, Russian Academy of Sciences) at 4.85, 7.7, 11.1, and
Autor:
V. V. Mardyshkin, M. Yu. Piotrovich, R. Yu. Sergeev, A. G. Mikhailov, A. A. Evstigneev, A. V. Ipatov, M. A. Kharinov, Yu. N. Gnedin, A. Dyakov
Publikováno v:
Astronomy Letters. 40:161-170
The results of radio observations for ten kinetically dominated quasars are presented. The observations have been performed at 3.5 cm with the RTF-32 radio telescopes at the Zelenchukskaya and Badary observatories of the Institute of Applied Astronom
Publikováno v:
Instruments and Experimental Techniques. 54:785-793
Broadband amplification and signal-frequency-conversion units with built-in heterodynes have been developed for radioastronomical receivers in wavelengths ranges of 3.5/13 and 6 cm. The use of such units allows extension of the reception band to 900
Autor:
V. V. Mardyshkin, M. A. Kharinov, A. V. Ipatov, A. M. Finkel’shtein, V. K. Konnikova, M. G. Mingaliev, A. G. Gorshkov
Publikováno v:
Astronomy Reports. 55:97-107
Results of a study of the variability of the BL Lac object S5 0716+714 are reported. The data were obtained in 150 daily observations on the RATAN-600 radio telescope at six frequencies from 0.97 to 21.7 GHz and 13 day-long sessions at a wavelength o