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Open Astronomy

formerly Baltic Astronomy

Editor-in-Chief: Barbuy, Beatriz


IMPACT FACTOR 2018: 0.350

CiteScore 2018: 0.24

SCImago Journal Rank (SJR) 2018: 0.202
Source Normalized Impact per Paper (SNIP) 2018: 0.144

ICV 2017: 121.03

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Online
ISSN
2543-6376
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Volume 27, Issue 1

Issues

The speckle-interferometric images modelling of artificial Earth satellites in problems of near-Earth astronomy

Vladimir P. Aleshin
  • Corresponding author
  • Joint-stock Company Research-and-Production Corporation “Precision System and Instruments”, Moscow, Russian Federation
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  • Other articles by this author:
  • De Gruyter OnlineGoogle Scholar
/ Eugene A. Grishin
  • Joint-stockCompany Research-and-Production Corporation “Precision System and Instruments”, Moscow, Russian Federation
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  • De Gruyter OnlineGoogle Scholar
/ Oleg A. Ivlev
  • Joint-stockCompany Research-and-Production Corporation “Precision System and Instruments”, Moscow, Russian Federation
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  • De Gruyter OnlineGoogle Scholar
/ Dmitry D. Novgorodtsev
  • Joint-stockCompany Research-and-Production Corporation “Precision System and Instruments”, Moscow, Russian Federation
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  • De Gruyter OnlineGoogle Scholar
/ Victor D. Shargorodsky
  • Joint-stockCompany Research-and-Production Corporation “Precision System and Instruments”, Moscow, Russian Federation
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Published Online: 2018-07-05 | DOI: https://doi.org/10.1515/astro-2018-0020

Abstract

The article represents the results of efficiency estimation for perspective observation facilities of near-Earth astronomy in terms of the AES (artificial Earth’s satellite) optical images obtaining and quality. A mathematical method for modeling optical images based on the induced virtual environment is proposed . A speckle interferometric image registration scheme and bispectral processing are reviewed. Upon modelling, the real speckle interferometric images of stars have been used as scattering functions; the AES orbits and geometry have been set in reliance on the real AES orbits and 3D-shapes. Additionally, photon and readout noises have been modelled. A large set of different variants of the AES orbits and 3D-shapes is reviewed.Anon-linear distortion problem is analyzed. The modelling has been performed under various atmosphere turbulence conditions (2”, 4”). The following characteristics have been estimated: number of frames to accumulate depending on the AES orbit and shape, noise intensity, type and parameters of bispectral processing, energy characteristics.

Keywords : speckle interferometry; artificial Earth’s satellite; bispectral processing

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About the article

Received: 2017-11-16

Accepted: 2017-12-27

Published Online: 2018-07-05


Citation Information: Open Astronomy, Volume 27, Issue 1, Pages 120–125, ISSN (Online) 2543-6376, DOI: https://doi.org/10.1515/astro-2018-0020.

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© 2018 Vladimir P. Aleshin et al.. This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License. BY-NC-ND 4.0

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