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Wide-field subsecond temporal resolution optical monitoring systems for detection and study of cosmic hazards

 a,  a,  a,  b,  b,  b,  b,  c,  d
a Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Zelenchukskiy Region, Karachai-Cherkessian Republic, Russian Federation
b Station Optical Observations "Arkhyz" Research and Production Corporation "Precision Instrument Systems", Nizhny Arkhyz, Zelenchukskii Region, Karachaevo-Cherkesiya, Russian Federation
c Parallax Ltd., ul. Adoratskogo 29v, Kazan, 420132, Russian Federation
d National University of Ireland, University Road, Galway, Ireland

Near-Earth space hazards and their detection (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 27 March 2013)

Fulltext pdf (1.6 MB)
Fulltext is also available at DOI: 10.3367/UFNe.0183.201308i.0888
PACS: 89.60.Gg, 95.55.Cs, 96.30.Ys (all)
DOI: 10.3367/UFNe.0183.201308i.0888
URL: https://ufn.ru/en/articles/2013/8/h/
000327017200007
2-s2.0-84888115637
2013PhyU...56..836B
Citation: Beskin G M, Karpov S V, Plokhotnichenko V L, Bondar S F, Perkov A V, Ivanov E A, Katkova E V, Sasyuk V V, Sherer A "Wide-field subsecond temporal resolution optical monitoring systems for detection and study of cosmic hazards" Phys. Usp. 56 836–842 (2013)
BibTex BibNote ® (generic)BibNote ® (RIS)MedlineRefWorks
%0 Journal Article
%T Wide-field subsecond temporal resolution optical monitoring systems for detection and study of cosmic hazards
%A G. M. Beskin
%A S. V. Karpov
%A V. L. Plokhotnichenko
%A S. F. Bondar
%A A. V. Perkov
%A E. A. Ivanov
%A E. V. Katkova
%A V. V. Sasyuk
%A A. Sherer
%I Physics-Uspekhi
%D 2013
%J Phys. Usp.
%V 56
%N 8
%P 836-842
%U https://ufn.ru/en/articles/2013/8/h/
%U https://doi.org/10.3367/UFNe.0183.201308i.0888

27th, March 2013

Оригинал: Бескин Г М, Карпов С В, Плохотниченко В Л, Бондарь С Ф, Перков А В, Иванов Е А, Каткова Е В, Сасюк В В, Шерер Э «Системы широкоугольного оптического мониторинга субсекундного временнóго разрешения для обнаружения и исследования космических угроз» УФН 183 888–894 (2013); DOI: 10.3367/UFNr.0183.201308i.0888

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