Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Shakun, A. S."'
We investigated two variable stars AH Tau and ZZ Cas. They are eclipsing binaries of W UMa and $\beta$ Lyr types. The period changes with time. The reason for steady changes of the period could be the mass transfer (the flow of matter) between compon
Externí odkaz:
http://arxiv.org/abs/1810.09256
The mean square displacement (MSD) of an argon molecule as a function of time is studied. Its deviations from the standard asymptotic law for intermediate times are analyzed in details. It is shown that these deviations are mainly connected with the
Externí odkaz:
http://arxiv.org/abs/1612.03933
Publikováno v:
In Journal of Molecular Liquids 1 November 2019 293
Publikováno v:
In Journal of Molecular Liquids June 2017 235:155-162
Autor:
Shakun, A. S.1 (AUTHOR), Vorobyova, V. I.1 (AUTHOR), Chygyrynets, O. E.1 (AUTHOR), Skiba, M. I.2 (AUTHOR)
Publikováno v:
Journal of Chemistry. 6/23/2020, p1-10. 10p.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Shakun, L. S.
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 148-152 (2017)
Odessa Astronomical Publications; Том 9 (1996); 148-152
Odessa Astronomical Publications; Том 9 (1996); 148-152
New program models the scattering of the sun light in Earth atmosphere. The program is not in the strict relation with the model of light scattering and atmosphere structure. This fact permits to use the program for different atmosphere models. The w
Publikováno v:
Odessa Astronomical Publications, Vol 17, Iss 0, Pp 78-81 (2017)
Odessa Astronomical Publications; Том 17 (2004); 78-81
Odessa Astronomical Publications; Том 17 (2004); 78-81
Use of a twilight sounding method of the Earth's atmosphere with the aim to reveal aerosols inflow to the upper and medial atmosphere needs a method of separation twilight sky brightness to the brightness of primary and secondary twilight. Method of