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...
Збережено в:
Дата: | 2011 |
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Автор: | |
Формат: | Стаття |
Мова: | English |
Опубліковано: |
Advances in astronomy and space physics
2011
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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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of UkraineРезюме: | 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. |
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