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New type optical Cassegrain antenna with lenses telescope system
The loss, which caused by the secondary mirror of Cassegrain antenna, is analyzed with Gaussian theory. Under the diameter of secondary mirror being one-fifth of the primary diameter, the loss goes beyond 15%. Optimum structure of optical antenna, which is made up of Cassegrain antenna and lenses sy...
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Published in: | Optik (Stuttgart) 2010-03, Vol.121 (6), p.521-525 |
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container_title | Optik (Stuttgart) |
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creator | Xiao, Liuping Yang, Huajun Liu, Xiaojing Xu, Quan Xiong, Xinqiang |
description | The loss, which caused by the secondary mirror of Cassegrain antenna, is analyzed with Gaussian theory. Under the diameter of secondary mirror being one-fifth of the primary diameter, the loss goes beyond 15%. Optimum structure of optical antenna, which is made up of Cassegrain antenna and lenses system, is devised to solve the waste effectively. The optimal diameter of the mirror is analyzed with Matlab. The relation, the transmitting distance with the ratio of
P
r min/
P
out1 is attained by Gaussian theory, where
P
r min is the minimum power of receiver signals required by optimum antenna;
P
out1 is the power emitted by the optimum antenna. |
doi_str_mv | 10.1016/j.ijleo.2008.09.002 |
format | article |
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P
r min/
P
out1 is attained by Gaussian theory, where
P
r min is the minimum power of receiver signals required by optimum antenna;
P
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P
r min/
P
out1 is attained by Gaussian theory, where
P
r min is the minimum power of receiver signals required by optimum antenna;
P
out1 is the power emitted by the optimum antenna.</description><subject>Antennas</subject><subject>Astronomy</subject><subject>Cassegrain antenna</subject><subject>Cassegrain antennas</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</subject><subject>Gaussian</subject><subject>Historical astronomy and archaeoastronomy; and other topics in fundamental astronomy and astrophysics; instrumentation, techniques, and astronomical observations</subject><subject>Laser communication</subject><subject>Lenses</subject><subject>Matlab</subject><subject>Optical antenna</subject><subject>Optimization</subject><subject>Secondary mirrors</subject><subject>Transmission</subject><issn>0030-4026</issn><issn>1618-1336</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp9kD1PwzAURS0EEqXwC1iyILEkPMeJ7QxIoIovqYIFZstxXsBVmhQ_Q9V_T0orRqa3nHuv3mHsnEPGgcurReYXHQ5ZDqAzqDKA_IBNuOQ65ULIQzYBEJAWkMtjdkK0AAClQE3YzTOuk7hZYTKsone2S2aWCN-D9X1i-4h9b5O1jx9Jhz0hJRE7JDeMAdpQxOUpO2ptR3i2v1P2dn_3OntM5y8PT7PbeeqElDFVha0loHYCdcVrXWsBWBQC6saVeV47ZXOwumig1VqpkrfS2aKESnNetZUVU3a5612F4fMLKZqlJ4ddZ3scvshwqbiQ1ShgRMUOdWEgCtiaVfBLGzaGg9n6Mgvz68tsfRmozOhrTF3sByyNHtpge-fpL5rnqtSVLkbuesfh-O23x2DIeewdNj6gi6YZ_L87P38IgSI</recordid><startdate>201003</startdate><enddate>201003</enddate><creator>Xiao, Liuping</creator><creator>Yang, Huajun</creator><creator>Liu, Xiaojing</creator><creator>Xu, Quan</creator><creator>Xiong, Xinqiang</creator><general>Elsevier GmbH</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>201003</creationdate><title>New type optical Cassegrain antenna with lenses telescope system</title><author>Xiao, Liuping ; Yang, Huajun ; Liu, Xiaojing ; Xu, Quan ; Xiong, Xinqiang</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c366t-74ab60e8c3e891b8b830e4430bdc522bc7a20a84d0f887751f6ca45098119f9a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Antennas</topic><topic>Astronomy</topic><topic>Cassegrain antenna</topic><topic>Cassegrain antennas</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</topic><topic>Gaussian</topic><topic>Historical astronomy and archaeoastronomy; and other topics in fundamental astronomy and astrophysics; instrumentation, techniques, and astronomical observations</topic><topic>Laser communication</topic><topic>Lenses</topic><topic>Matlab</topic><topic>Optical antenna</topic><topic>Optimization</topic><topic>Secondary mirrors</topic><topic>Transmission</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Xiao, Liuping</creatorcontrib><creatorcontrib>Yang, Huajun</creatorcontrib><creatorcontrib>Liu, Xiaojing</creatorcontrib><creatorcontrib>Xu, Quan</creatorcontrib><creatorcontrib>Xiong, Xinqiang</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Optik (Stuttgart)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Xiao, Liuping</au><au>Yang, Huajun</au><au>Liu, Xiaojing</au><au>Xu, Quan</au><au>Xiong, Xinqiang</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New type optical Cassegrain antenna with lenses telescope system</atitle><jtitle>Optik (Stuttgart)</jtitle><date>2010-03</date><risdate>2010</risdate><volume>121</volume><issue>6</issue><spage>521</spage><epage>525</epage><pages>521-525</pages><issn>0030-4026</issn><eissn>1618-1336</eissn><coden>OTIKAJ</coden><abstract>The loss, which caused by the secondary mirror of Cassegrain antenna, is analyzed with Gaussian theory. Under the diameter of secondary mirror being one-fifth of the primary diameter, the loss goes beyond 15%. Optimum structure of optical antenna, which is made up of Cassegrain antenna and lenses system, is devised to solve the waste effectively. The optimal diameter of the mirror is analyzed with Matlab. The relation, the transmitting distance with the ratio of
P
r min/
P
out1 is attained by Gaussian theory, where
P
r min is the minimum power of receiver signals required by optimum antenna;
P
out1 is the power emitted by the optimum antenna.</abstract><cop>Reutlingen</cop><pub>Elsevier GmbH</pub><doi>10.1016/j.ijleo.2008.09.002</doi><tpages>5</tpages></addata></record> |
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subjects | Antennas Astronomy Cassegrain antenna Cassegrain antennas Earth, ocean, space Exact sciences and technology Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Gaussian Historical astronomy and archaeoastronomy and other topics in fundamental astronomy and astrophysics instrumentation, techniques, and astronomical observations Laser communication Lenses Matlab Optical antenna Optimization Secondary mirrors Transmission |
title | New type optical Cassegrain antenna with lenses telescope system |
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