Lucky image performance simulation on the basis of optical turbulence data obtained on Mt. Shatdzhatmaz

dc.contributor.author	Safonov, B.S.
dc.date.accessioned	2017-06-03T20:15:52Z
dc.date.available	2017-06-03T20:15:52Z
dc.date.issued	2011
dc.identifier.citation	Lucky image performance simulation on the basis of optical turbulence data obtained on Mt. Shatdzhatmaz / B.S. Safonov // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 102-105. — Бібліогр.: 6 назв. — англ.	uk_UA
dc.identifier.isbn	987-966-439-367-3
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119093
dc.description.abstract	Lucky imaging is a method allowing to achieve difiraction resolution on a moderate ground-based telescopes with the cost of magnitude limitation. To adequately evaluate capabilities of this technique for a given place (Mt. Shatdzhatmaz) we performed a Monte Carlo numerical simulation taking into account properties of optical turbulence measured there. Statistics of lucky imaging isoplanatic angle was evaluated on the basis of these data. Optimal atmospheric conditions for lucky imaging were obtained.	uk_UA
dc.description.sponsorship	I would like to thank Dr. Kornilov V. G. and Dr. Tokovinin A. A. for valuable discussions.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Advances in astronomy and space physics	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Lucky image performance simulation on the basis of optical turbulence data obtained on Mt. Shatdzhatmaz	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA