GALILEAN TELESCOPE ARRAYS IN INFRARED REGION USING SUBSTRATE-MODE HOLOGRAMS
| dc.citation.epage | 116 | en_US |
| dc.citation.issue | 3 | en_US |
| dc.citation.spage | 113 | en_US |
| dc.citation.volume | 24 | en_US |
| dc.citation.woscount | 0 | |
| dc.contributor.author | SU, DC | en_US |
| dc.contributor.author | TSAI, YK | en_US |
| dc.contributor.author | HAUNG, YT | en_US |
| dc.contributor.department | 光電工程學系 | zh_TW |
| dc.contributor.department | Department of Photonics | 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.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.identifier.doi | 10.1088/0150-536X/24/3/003 | en_US |
| dc.identifier.issn | 0150-536X | en_US |
| dc.identifier.journal | JOURNAL OF OPTICS-NOUVELLE REVUE D OPTIQUE | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1088/0150-536X/24/3/003 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/3035 | |
| dc.identifier.wosnumber | WOS:A1993MB92800003 | |
| 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 |