Zobrazeno 1 - 10
of 18
pro vyhledávání: '"A. V. Shatina"'
Publikováno v:
Российский технологический журнал, Vol 8, Iss 1, Pp 97-109 (2020)
This paper derives a formula for calculating the velocity of arbitrary point in the field of view of the satellite camera in the process of orbital imagery of the planet's surface. The formula describes the velocity as a function of the point coordin
Externí odkaz:
https://doaj.org/article/25a611e8e3f64e63886cc6ed02d51986
Publikováno v:
Российский технологический журнал, Vol 6, Iss 4, Pp 65-77 (2018)
In this paper, a formula is obtained for calculating the velocity of an image in the plane of image fixation during a space survey of the planet's surface with the aid of an on-oard optoelectronic device. The ideal task is considered: the Earth is mo
Externí odkaz:
https://doaj.org/article/561cd4e3d59b4791ab2dca80543700e1
Autor:
E. V. Sadovnikova, A. V. Shatina
Publikováno v:
Российский технологический журнал, Vol 6, Iss 4, Pp 89-104 (2018)
The rotational motion of an artificial satellite in the central Newtonian force field is investigated. The satellite is modeled as a symmetric solid with rigid viscoelastic rods rigidly attached along the symmetry axis and with a spherical inertia te
Externí odkaz:
https://doaj.org/article/50020d405a0b43ea9990b0fee5b1dda1
Publikováno v:
Российский технологический журнал, Vol 5, Iss 3, Pp 130-137 (2017)
In the paper the classic problem of N bodies is treated as if the mass of one body (the Sun) is much larger than the mass of the rest mutually gravitating bodies. We take as the unperturbed motion the movement of a planet in an elliptical orbit, with
Externí odkaz:
https://doaj.org/article/db9fa916350b432c9755af51911573e4
Autor:
E. V. Sadovnikova, A. V. Shatina
Publikováno v:
Mechanics of Solids. 54:204-210
The present work is aimed at studying the rotational motion of a satellite in a central force field in an elliptical orbit. A satellite is simulated by a dynamically symmetrical solid body with flexible viscoelastic rods, firmly fastened along the sy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c6ac9cca379d31f3520f6b867c98baeb
https://doi.org/10.3103/s0025654419030208
https://doi.org/10.3103/s0025654419030208
Autor:
A. S. Borets, A. V. Shatina
Publikováno v:
Journal of Physics: Conference Series. 1705:012001
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cdbcca0b5b3ffaa829beb027cd49ce50
https://doi.org/10.1088/1742-6596/1705/1/012001
https://doi.org/10.1088/1742-6596/1705/1/012001
Publikováno v:
Journal of Physics: Conference Series. 1705:012008
In this paper we derive the formulas describing velocity of the planet’s surface orbital survey image in the focal plane, obtained via on-board electro-optical equipment in the nadir-viewing geometry, with consideration for the Earth’s oblateness
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f8cbbca8cf1abc02cd85aa401148e536
https://doi.org/10.1088/1742-6596/1705/1/012008
https://doi.org/10.1088/1742-6596/1705/1/012008
Autor:
E. V. Sherstnyov, A. V. Shatina
Publikováno v:
Cosmic Research. 53:163-170
The motion of a “planet-satellite” system in a gravitational field of mutual attraction forces is investigated. The planet is modeled by a body consisting of a solid core and a viscoelastic shell made of Kelvin-Voigt material. The satellite is mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f8dd45b1c8312e1b5e67ba31ff5f530c
https://doi.org/10.1134/s0010952515020082
https://doi.org/10.1134/s0010952515020082
Publikováno v:
Cosmic Research. 49:345-352
Translational-rotational motion of two viscoelastic planets in a gravitational force field is studied. The planets are modeled by homogeneous isotropic viscoelastic bodies. In their natural undeformed state each of the planets represents a sphere. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8554e31b4324eb00e43b7b2479315774
https://doi.org/10.1134/s0010952511030117
https://doi.org/10.1134/s0010952511030117
Publikováno v:
Cosmic Research. 47:438-443
Translational-rotational motion of three planets modeled by viscoelastic balls in the gravitational field of mutual attraction is studied in this paper. The system of equations of motion for the mechanical system under consideration is deduced from t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66ab03bb1ec02a8ff5a4fde3bc940553
https://doi.org/10.1134/s001095250905013x
https://doi.org/10.1134/s001095250905013x