GALILEAN TELESCOPE ARRAYS IN INFRARED REGION USING SUBSTRATE-MODE HOLOGRAMS

完整後設資料紀錄

DC 欄位	值	語言
dc.contributor.author	SU, DC	en_US
dc.contributor.author	TSAI, YK	en_US
dc.contributor.author	HAUNG, YT	en_US
dc.date.accessioned	2014-12-08T15:04:32Z	-
dc.date.available	2014-12-08T15:04:32Z	-
dc.date.issued	1993-05-01	en_US
dc.identifier.issn	0150-536X	en_US
dc.identifier.uri	http://dx.doi.org/10.1088/0150-536X/24/3/003	en_US
dc.identifier.uri	http://hdl.handle.net/11536/3035	-
dc.description.abstract	Galilean telescope arrays using substrate-mode holograms are presented. They are manufactured the visible region, and designed for operation in the infrared region. And they are formed in a monolithic block and compact, so they are easily introduced into an optical system. In addition, they do not introduce a local inversion as that in the Kepler telescope arrays.	en_US
dc.language.iso	en_US	en_US
dc.subject	GALILEAN TELESCOPE ARRAY	en_US
dc.subject	SUBSTRATE-MODE HOLOGRAM	en_US
dc.title	GALILEAN TELESCOPE ARRAYS IN INFRARED REGION USING SUBSTRATE-MODE HOLOGRAMS	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1088/0150-536X/24/3/003	en_US
dc.identifier.journal	JOURNAL OF OPTICS-NOUVELLE REVUE D OPTIQUE	en_US
dc.citation.volume	24	en_US
dc.citation.issue	3	en_US
dc.citation.spage	113	en_US
dc.citation.epage	116	en_US
dc.contributor.department	光電工程學系	zh_TW
dc.contributor.department	Department of Photonics	en_US
dc.identifier.wosnumber	WOS:A1993MB92800003	-
dc.citation.woscount	0	-
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