Interferometric method for image formation: the basic ideas and computer simulation

• Опубліковано в: : Кинематика и физика небесных тел
• Дата: 2005
• Автори: Kornienko, Yu., Pugach, V.
• Формат: Стаття
• Мова: English
• Опубліковано: Головна астрономічна обсерваторія НАН України 2005
• Теми: MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
• Онлайн доступ: https://nasplib.isofts.kiev.ua/handle/123456789/79716
• Назва журналу: Digital Library of Periodicals of National Academy of Sciences of Ukraine
• Цитувати: Interferometric method for image formation: the basic ideas and computer simulation / Yu. Kornienko, V. Pugach // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 534-536. — Бібліогр.: 6 назв. — англ.

As it is known, the key resolution limit of an astronomical instrument is determined by diffraction of a received wave on the instrument aperture. However, by performing observations from the Earth surface in a short-wave part of the wave band, it is seldom possible to achieve this limit because of...