2025-02-23T00:27:47-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-79716%22&qt=morelikethis&rows=5
2025-02-23T00:27:47-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22irk-123456789-79716%22&qt=morelikethis&rows=5
2025-02-23T00:27:47-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-23T00:27:47-05:00 DEBUG: Deserialized SOLR response
Interferometric method for image formation: the basic ideas and computer simulation

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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Bibliographic Details
Main Authors: Kornienko, Yu., Pugach, V.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
Series:Кинематика и физика небесных тел
Subjects:
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/79716
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