Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Yu. I. Velikodskii"'
Autor:
A. N. Opanasenko, V. G. Kaidash, Yu. I. Velikodskii, Viktor Korokhin, Yu. G. Shkuratov, N. V. Opanasenko
Publikováno v:
Kinematics and Physics of Celestial Bodies. 27:38-41
Polarimetric observations of the moon have been carried out at λeff = 0.48 and 0.63 μm using the 50 cm telescope of the Maidanak (Middle Asia) observatory. Imaging has been performed using a Canon-350D camera with a CMOS array and rotating polaroid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a734e924303da08e8516a561e6bee952
https://doi.org/10.3103/s0884591311010077
https://doi.org/10.3103/s0884591311010077
Autor:
S. Yu. Gerasimenko, V. G. Kaidash, Yu. I. Velikodskii, Viktor Korokhin, Yu. G. Shkuratov, N. V. Opanasenko
Publikováno v:
Solar System Research. 43:89-99
During two lunations, telescopic imaging of the near side of the Moon was performed at the Maidanak mountain observatory (Uzbekistan) with the use of digital cameras based on CMOS detectors. In different ranges of phase angles, the slope of the phase
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::35b4164f21ca10e09240572a866d492d
https://doi.org/10.1134/s0038094609020014
https://doi.org/10.1134/s0038094609020014
Publikováno v:
Kinematics and Physics of Celestial Bodies. 24:201-208
Peculiarities in the use of CCD matrices for photopolarimetric observations are considered. Algorithms for processing the CCD photopolarimetric and polarimetric observations of Jupiter and other bright extended objects are described with an emphasis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a63929a91ff81426ae61e34f4b22307
https://doi.org/10.3103/s088459130804003x
https://doi.org/10.3103/s088459130804003x
Autor:
Sergey Kuzin, G. P. Marchenko, Yu. I. Velikodskii, Viktor Korokhin, A. A. Pertsov, S. A. Beletskii, O. I. Bugaenko, A. P. Ignat'ev, Igor A. Zhitnik, I. L. Belkina, L. A. Akimov
Publikováno v:
Astronomy Reports. 49:579-586
A spectral analysis of a series of integrated MgXII 8.42 A X-ray intensities recorded by the CORONAS-F SPIRIT spectroheliometer is presented. Statistically significant peaks for periods in the intervals 12–30 min and 40–200 min were found in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0febf97df6192d191d906f6447041231
https://doi.org/10.1134/1.1985955
https://doi.org/10.1134/1.1985955
Autor:
A. A. Berezhnoi, S. V. Karashevich, A. V. Ivanov, A. V. Sergeev, K. N. Naumov, A. Kurenya, I. A. Vereshchagina, Ya. V. Naiden, M. M. Chernikov, V. Kozlov, D. L. Gorshanov, N. V. Emelyanov, Yu. I. Velikodskii, E. N. Sokov, E. V. Khrutskaya, T. R. Irsmambetova, N. Parakhin, A. V. Devyatkin, Maksim V. Andreev, S. A. Selyaev, I. S. Izmailov, V. N. Raskhozhev, A. S. Bekhteva, M. Yu. Khovrichev, S. N. Vashkov'yak
Publikováno v:
Astronomicheskii Vestnik / Solar System Research
Astronomicheskii Vestnik / Solar System Research, 2011, 45, pp.264-277. ⟨10.1134/S0038094611010035⟩
Astronomicheskii Vestnik / Solar System Research, 2011, 45, pp.264-277. ⟨10.1134/S0038094611010035⟩
International audience; In 2009, in five Russian observatories photometric observations of Jupiter's Galilean satellites during their mutual occultations and eclipses were carried out. Based on these observations, an original method was used to ascer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0c033c6cb5f8396fca8cad4234a6c83
https://hal.science/hal-03742293
https://hal.science/hal-03742293
