Zobrazeno 1 - 10
of 18
pro vyhledávání: '"A. S. Tuchin"'
Publikováno v:
Odessa Astronomical Publications, Vol 20, Iss 2, Pp 81-83 (2017)
A scanning of plates from Sternberg astronomical institute's photograph collection has began to create a library of digital images. A large number of new variable stars has already discovered using the scans. It is shown that it is possible to carry
Externí odkaz:
https://doaj.org/article/01de8ceb9fd3454dabda8610de1fb40e
Autor:
Yuliya A. Timkina, Vladislav S. Tuchin, Aleksandr P. Litvin, Elena V. Ushakova, Andrey L. Rogach
Publikováno v:
Nanomaterials, Vol 13, Iss 4, p 744 (2023)
Lead–halide perovskite nanocrystals are an attractive class of materials since they can be easily fabricated, their optical properties can be tuned all over the visible spectral range, and they possess high emission quantum yields and narrow photol
Externí odkaz:
https://doaj.org/article/1cad9c80bc034888adee6a559495eb41
Autor:
A. V. Svetlakova, M. Sanchez Mendez, E. S. Tuchin, A. N. Khodan, M. Traore, R. Azouani, A. Kanaev, V. V. Tuchin
Publikováno v:
Optics and Spectroscopy. 129:846-850
Autor:
A. I. Gladyshev, O. Yu. Stekolshchikov, V. G. Moshkalev, M. E. Prokhorov, A. V. Mironov, I. V. Kuznetsova, Andrey I. Zakharov, M. S. Tuchin, N. L. Kroussanova, A. O. Zhukov
Publikováno v:
Optoelectronics, Instrumentation and Data Processing. 57:426-436
Autor:
N. L. Krusanova, O. Y. Stekol’shchikov, V. K. Sysoev, M. E. Prohorov, M. S. Tuchin, I. V. Moskatiniev, A. D. Yudin, A. I. Zacharov
Publikováno v:
Solar System Research. 52:636-643
Modern star trackers are based on photodetector arrays such as CCD or CMOS arrays. The accuracy of commercially available devices is ~1–3 arcseconds. However, the development of the space industry calls for higher orientation accuracies, which are
Autor:
M. E. Prokhorov, A. I. Zakharov, M. S. Tuchin, A. V. Mironov, O. Yu. Stekolshchikov, A. O. Zhukov
Publikováno v:
Астрономия-2018. Том 1.
Publikováno v:
Solar System Research. 47:548-553
A method for determining the celestial coordinates of the center of the disk of the Earth from satellite observations with an accuracy of 1–5 arcseconds is suggested. The choice of the most suitable wavelength range is substantiated.
Publikováno v:
Astrophysical Bulletin. 68:481-493
We describe the principles of the computation of minimum specifications of the optical system and array detector of the star attitude sensor to achieve the required attitude accuracy for the given exposure. The computations assume that the attitude e
Publikováno v:
Astronomische Nachrichten. 334:828-831
The purpose of the LYRA mission is a multi-color all-sky survey of objects from 3 m to 16 m from the International Space Station, to result in a high-precision photometric catalog (Zakharov et al. 2013b). The expected error of the catalog will be 0.0
Autor:
M. E. Prokhorov, O. Yu. Stekol’shchikov, A. V. Mironov, A. I. Zakharov, M. S. Tuchin, Anton Biryukov
Publikováno v:
Astronomy Reports. 57:195-211
We describe goals and principles for the realization the Lyra-B space experiment onboard the International Space Station, which is currently being prepared at the Sternberg Astronomical Institute. The main goal of the experiment is to carry out a hig