Radiation characteristics enhancement of dual‐polarized antipodal Vivaldi antenna using double‐slot structure
In this article, a dual‐polarized double‐slot antipodal Vivaldi antenna (DP‐DsAVA) is proposed to solve the problem of conventional four‐element dual‐polarized antipodal Vivaldi antennas in that the side lobe level increases as frequency increases, and a grating lobe is generated at frequencies abov...
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Veröffentlicht in: | Microwave and optical technology letters 2020-03, Vol.62 (3), p.1245-1251 |
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creator | Kim, Woojoong Park, Jinsung Park, Hyeon‐Gyu Yoon, Young J. |
description | In this article, a dual‐polarized double‐slot antipodal Vivaldi antenna (DP‐DsAVA) is proposed to solve the problem of conventional four‐element dual‐polarized antipodal Vivaldi antennas in that the side lobe level increases as frequency increases, and a grating lobe is generated at frequencies above one octave. The DP‐DsAVA comprises two modified double‐slot antipodal Vivaldi antennas (DsAVAs), which are suitable for dual‐polarized implementation through incision and intersection, and each crossed DsAVA implements each polarization separately. Therefore, the proposed antenna does not produce a grating lobe within the operating frequency range, and it has a lower side lobe level compared to that of a conventional antenna. Measurements of the proposed antenna indicate that its impedance bandwidth is 5.4 to 16.4 GHz, and no grating lobe occurs within this bandwidth. At the operating frequency, the gain is 8.4 to 10.6 dBi, and the cross‐polarization level is below −18 dB. |
doi_str_mv | 10.1002/mop.32120 |
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The DP‐DsAVA comprises two modified double‐slot antipodal Vivaldi antennas (DsAVAs), which are suitable for dual‐polarized implementation through incision and intersection, and each crossed DsAVA implements each polarization separately. Therefore, the proposed antenna does not produce a grating lobe within the operating frequency range, and it has a lower side lobe level compared to that of a conventional antenna. Measurements of the proposed antenna indicate that its impedance bandwidth is 5.4 to 16.4 GHz, and no grating lobe occurs within this bandwidth. At the operating frequency, the gain is 8.4 to 10.6 dBi, and the cross‐polarization level is below −18 dB.</description><identifier>ISSN: 0895-2477</identifier><identifier>EISSN: 1098-2760</identifier><identifier>DOI: 10.1002/mop.32120</identifier><language>eng</language><publisher>Hoboken, USA: John Wiley & Sons, Inc</publisher><subject>Antennas ; Bandwidths ; double‐slot antipodal Vivaldi antenna ; double‐slot structure ; dual polarization ; dual polarization Vivaldi antenna ; Frequencies ; Frequency ranges ; grating lobe ; Polarization ; Sidelobes</subject><ispartof>Microwave and optical technology letters, 2020-03, Vol.62 (3), p.1245-1251</ispartof><rights>2019 Wiley Periodicals, Inc.</rights><rights>2020 Wiley Periodicals, Inc.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2970-4563f7909f5c2c041f202b3704b159e45455cf277540140a8c56413e9718820f3</citedby><cites>FETCH-LOGICAL-c2970-4563f7909f5c2c041f202b3704b159e45455cf277540140a8c56413e9718820f3</cites><orcidid>0000-0003-3980-0614</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2Fmop.32120$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2Fmop.32120$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,27901,27902,45550,45551</link.rule.ids></links><search><creatorcontrib>Kim, Woojoong</creatorcontrib><creatorcontrib>Park, Jinsung</creatorcontrib><creatorcontrib>Park, Hyeon‐Gyu</creatorcontrib><creatorcontrib>Yoon, Young J.</creatorcontrib><title>Radiation characteristics enhancement of dual‐polarized antipodal Vivaldi antenna using double‐slot structure</title><title>Microwave and optical technology letters</title><description>In this article, a dual‐polarized double‐slot antipodal Vivaldi antenna (DP‐DsAVA) is proposed to solve the problem of conventional four‐element dual‐polarized antipodal Vivaldi antennas in that the side lobe level increases as frequency increases, and a grating lobe is generated at frequencies above one octave. The DP‐DsAVA comprises two modified double‐slot antipodal Vivaldi antennas (DsAVAs), which are suitable for dual‐polarized implementation through incision and intersection, and each crossed DsAVA implements each polarization separately. Therefore, the proposed antenna does not produce a grating lobe within the operating frequency range, and it has a lower side lobe level compared to that of a conventional antenna. Measurements of the proposed antenna indicate that its impedance bandwidth is 5.4 to 16.4 GHz, and no grating lobe occurs within this bandwidth. At the operating frequency, the gain is 8.4 to 10.6 dBi, and the cross‐polarization level is below −18 dB.</description><subject>Antennas</subject><subject>Bandwidths</subject><subject>double‐slot antipodal Vivaldi antenna</subject><subject>double‐slot structure</subject><subject>dual polarization</subject><subject>dual polarization Vivaldi antenna</subject><subject>Frequencies</subject><subject>Frequency ranges</subject><subject>grating lobe</subject><subject>Polarization</subject><subject>Sidelobes</subject><issn>0895-2477</issn><issn>1098-2760</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp1kMtKAzEUhoMoWKsL3yDgysW0J7dmZinFG1Qqom6HNJOxKdNkmmSUuvIRfEafxNG6FQ78cPj-c-BD6JTAiADQ8dq3I0YJhT00IFDkGZUT2EcDyAuRUS7lITqKcQUATEo6QJsHVVmVrHdYL1VQOplgY7I6YuOWymmzNi5hX-OqU83Xx2frGxXsu6mwcsm2vlINfravqqnsz8Y4p3AXrXvBle8WjekrsfEJxxQ6nbpgjtFBrZpoTv5yiJ6uLh-nN9lsfn07vZhlmhYSMi4mrJYFFLXQVAMnNQW6YBL4gojCcMGF0DWVUnAgHFSuxYQTZgpJ8pxCzYbobHe3DX7TmZjKle-C61-WlHFOJGP9DNH5jtLBxxhMXbbBrlXYlgTKH6Nlb7T8Ndqz4x37Zhuz_R8s7-b3u8Y3TpV6LA</recordid><startdate>202003</startdate><enddate>202003</enddate><creator>Kim, Woojoong</creator><creator>Park, Jinsung</creator><creator>Park, Hyeon‐Gyu</creator><creator>Yoon, Young J.</creator><general>John Wiley & Sons, Inc</general><general>Wiley Subscription Services, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>8FD</scope><scope>F28</scope><scope>FR3</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-3980-0614</orcidid></search><sort><creationdate>202003</creationdate><title>Radiation characteristics enhancement of dual‐polarized antipodal Vivaldi antenna using double‐slot structure</title><author>Kim, Woojoong ; Park, Jinsung ; Park, Hyeon‐Gyu ; Yoon, Young J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2970-4563f7909f5c2c041f202b3704b159e45455cf277540140a8c56413e9718820f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Antennas</topic><topic>Bandwidths</topic><topic>double‐slot antipodal Vivaldi antenna</topic><topic>double‐slot structure</topic><topic>dual polarization</topic><topic>dual polarization Vivaldi antenna</topic><topic>Frequencies</topic><topic>Frequency ranges</topic><topic>grating lobe</topic><topic>Polarization</topic><topic>Sidelobes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kim, Woojoong</creatorcontrib><creatorcontrib>Park, Jinsung</creatorcontrib><creatorcontrib>Park, Hyeon‐Gyu</creatorcontrib><creatorcontrib>Yoon, Young J.</creatorcontrib><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Technology Research Database</collection><collection>ANTE: Abstracts in New Technology & Engineering</collection><collection>Engineering Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Microwave and optical technology letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kim, Woojoong</au><au>Park, Jinsung</au><au>Park, Hyeon‐Gyu</au><au>Yoon, Young J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radiation characteristics enhancement of dual‐polarized antipodal Vivaldi antenna using double‐slot structure</atitle><jtitle>Microwave and optical technology letters</jtitle><date>2020-03</date><risdate>2020</risdate><volume>62</volume><issue>3</issue><spage>1245</spage><epage>1251</epage><pages>1245-1251</pages><issn>0895-2477</issn><eissn>1098-2760</eissn><abstract>In this article, a dual‐polarized double‐slot antipodal Vivaldi antenna (DP‐DsAVA) is proposed to solve the problem of conventional four‐element dual‐polarized antipodal Vivaldi antennas in that the side lobe level increases as frequency increases, and a grating lobe is generated at frequencies above one octave. The DP‐DsAVA comprises two modified double‐slot antipodal Vivaldi antennas (DsAVAs), which are suitable for dual‐polarized implementation through incision and intersection, and each crossed DsAVA implements each polarization separately. Therefore, the proposed antenna does not produce a grating lobe within the operating frequency range, and it has a lower side lobe level compared to that of a conventional antenna. Measurements of the proposed antenna indicate that its impedance bandwidth is 5.4 to 16.4 GHz, and no grating lobe occurs within this bandwidth. At the operating frequency, the gain is 8.4 to 10.6 dBi, and the cross‐polarization level is below −18 dB.</abstract><cop>Hoboken, USA</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1002/mop.32120</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0003-3980-0614</orcidid></addata></record> |
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subjects | Antennas Bandwidths double‐slot antipodal Vivaldi antenna double‐slot structure dual polarization dual polarization Vivaldi antenna Frequencies Frequency ranges grating lobe Polarization Sidelobes |
title | Radiation characteristics enhancement of dual‐polarized antipodal Vivaldi antenna using double‐slot structure |
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