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...

Повний опис

Збережено в:
Бібліографічні деталі
Дата:2011
Автор: Safonov, B.S.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ: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
Цитувати: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
Опис
Резюме: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.