Interferometric method for image formation: the basic ideas and computer simulation
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...
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| Veröffentlicht in: | Кинематика и физика небесных тел |
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| Datum: | 2005 |
| ISSN: | 0233-7665 |
| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | Englisch |
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Головна астрономічна обсерваторія НАН України
2005
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/79716 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | 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. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862712663028531200 |
|---|---|
| author | Kornienko, Yu. Pugach, V. |
| author_facet | Kornienko, Yu. Pugach, V. |
| citation_txt | 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. |
| collection | DSpace DC |
| container_title | Кинематика и физика небесных тел |
| 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.
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| first_indexed | 2025-12-07T17:38:51Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-79716 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| issn | 0233-7665 |
| language | English |
| last_indexed | 2025-12-07T17:38:51Z |
| publishDate | 2005 |
| publisher | Головна астрономічна обсерваторія НАН України |
| record_format | dspace |
| spelling | Kornienko, Yu. Pugach, V. 2015-04-03T20:16:38Z 2015-04-03T20:16:38Z 2005 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 https://nasplib.isofts.kiev.ua/handle/123456789/79716 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. en Головна астрономічна обсерваторія НАН України Кинематика и физика небесных тел MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics Interferometric method for image formation: the basic ideas and computer simulation Article published earlier |
| spellingShingle | Interferometric method for image formation: the basic ideas and computer simulation Kornienko, Yu. Pugach, V. MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics |
| title | Interferometric method for image formation: the basic ideas and computer simulation |
| title_full | Interferometric method for image formation: the basic ideas and computer simulation |
| title_fullStr | Interferometric method for image formation: the basic ideas and computer simulation |
| title_full_unstemmed | Interferometric method for image formation: the basic ideas and computer simulation |
| title_short | Interferometric method for image formation: the basic ideas and computer simulation |
| title_sort | interferometric method for image formation: the basic ideas and computer simulation |
| topic | MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics |
| topic_facet | MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/79716 |
| work_keys_str_mv | AT kornienkoyu interferometricmethodforimageformationthebasicideasandcomputersimulation AT pugachv interferometricmethodforimageformationthebasicideasandcomputersimulation |