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

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 acc...

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Bibliographische Detailangaben
Datum:2011
1. Verfasser: Safonov, B.S.
Format: Artikel
Sprache:English
Veröffentlicht: Advances in astronomy and space physics 2011
Schriftenreihe:Advances in Astronomy and Space Physics
Online Zugang:http://dspace.nbuv.gov.ua/handle/123456789/119093
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
Beschreibung
Zusammenfassung: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.