Запис Детальніше

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

Vernadsky National Library of Ukraine

Переглянути архів Інформація
 
 
Поле Співвідношення
 
Title Interferometric method for image formation: the basic ideas and computer simulation
 
Creator Kornienko, Yu.
Pugach, V.
 
Subject MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
 
Description 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 phase distortions arising by the propagation of a wave in the Earth’s atmosphere which is caused by fluctuations of the refraction index. There is a series of ideas how to form an astronomical image decreasing or excluding the influence of phase distortions during the observation. One of such methods is the interferometric imaging method. We describe this technique and present results of simulated observations of various objects and their images reconstructed for various atmospheric distortions. The advantage of a multi-beam interferometer, both by obtaining of instantaneous images and by using time accumulation is well-visible.
 
Date 2015-04-03T20:16:38Z
2015-04-03T20:16:38Z
2005
 
Type Article
 
Identifier 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.
0233-7665
http://dspace.nbuv.gov.ua/handle/123456789/79716
 
Language en
 
Relation Кинематика и физика небесных тел
 
Publisher Головна астрономічна обсерваторія НАН України