Zobrazeno 1 - 1
of 1
pro vyhledávání: '"M. M. Chernikov"'
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