Design and experimental test of an optical vortex coronagraph
Using an optical vortex coronagraph (OVC) is one of the most promising techniques for di- rectly imaging exoplanets because of its small inner working angle and high throughput. This paper presents the design and laboratory demonstration performance of an OVC based on liquid crystal polymers (LCPs)...
Gespeichert in:
Veröffentlicht in: | Research in astronomy and astrophysics 2017-05, Vol.17 (6), p.101-106 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 106 |
---|---|
container_issue | 6 |
container_start_page | 101 |
container_title | Research in astronomy and astrophysics |
container_volume | 17 |
creator | Liu, Cheng-Chao Ren, De-Qing Zhu, Yong-Tian Dou, Jiang-Pei |
description | Using an optical vortex coronagraph (OVC) is one of the most promising techniques for di- rectly imaging exoplanets because of its small inner working angle and high throughput. This paper presents the design and laboratory demonstration performance of an OVC based on liquid crystal polymers (LCPs) at 633 nm and 1520 nm. The OVC can deliver good performance in laboratory tests and achieve a contrast of 10-6 at an angular distance of 3A/D, which can be implemented for imaging young giant exoplanets in combination with extreme adaptive optics. |
doi_str_mv | 10.1088/1674-4527/17/6/60 |
format | Article |
fullrecord | <record><control><sourceid>proquest_iop_j</sourceid><recordid>TN_cdi_proquest_journals_2357599430</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cqvip_id>672362792</cqvip_id><sourcerecordid>2357599430</sourcerecordid><originalsourceid>FETCH-LOGICAL-c410t-290cd466932265f4b52f34de95618b9c2559bb6282bf3520c2894d6c629d0d1d3</originalsourceid><addsrcrecordid>eNp9kE9PwzAMxSMEEmPwAbhVwLUscRqnOXBA4680iQucozZJu06j6dIOjW9Pq07jgjhZsn9-fn6EXDJ6y2iazhjKJE4EyBmTM5whPSIT4ErGCFQdk8lhfkrO2nZFKQqBMCF3D66tyjrKahu5XeNC9enqLltHnWu7yBf9IPJNV5m-9eVD53aR8cHXWRmyZnlOTops3bqLfZ2Sj6fH9_lLvHh7fp3fL2KTMNrFoKixCaLiACiKJBdQ8MQ6JZCluTIghMpzhBTyggugBlKVWDQIylLLLJ-S61G3CX6z7Z3pld-Guj-pgQsplEo47Sk2Uib4tg2u0E3_Tha-NaN6SEkPKeghBc2kRo3Dzs24U_nmVzRk2UhQpLqxRY_Ff2D_yV7trSx9XW6qujx4QQkcQSrgP6JofiY</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2357599430</pqid></control><display><type>article</type><title>Design and experimental test of an optical vortex coronagraph</title><source>IOP Publishing Journals</source><source>Alma/SFX Local Collection</source><creator>Liu, Cheng-Chao ; Ren, De-Qing ; Zhu, Yong-Tian ; Dou, Jiang-Pei</creator><creatorcontrib>Liu, Cheng-Chao ; Ren, De-Qing ; Zhu, Yong-Tian ; Dou, Jiang-Pei</creatorcontrib><description>Using an optical vortex coronagraph (OVC) is one of the most promising techniques for di- rectly imaging exoplanets because of its small inner working angle and high throughput. This paper presents the design and laboratory demonstration performance of an OVC based on liquid crystal polymers (LCPs) at 633 nm and 1520 nm. The OVC can deliver good performance in laboratory tests and achieve a contrast of 10-6 at an angular distance of 3A/D, which can be implemented for imaging young giant exoplanets in combination with extreme adaptive optics.</description><identifier>ISSN: 1674-4527</identifier><identifier>EISSN: 2397-6209</identifier><identifier>DOI: 10.1088/1674-4527/17/6/60</identifier><language>eng</language><publisher>Beijing: National Astronomical Observatories, CAS and IOP Publishing Ltd</publisher><subject>Adaptive optics ; Coronagraphs ; Extrasolar planets ; instrumentation: coronagraph ; Laboratories ; Laboratory tests ; Liquid crystal polymers ; Liquid crystals ; methods: laboratory ; Optics ; Polymers ; techniques: optical vortex ; Vortices</subject><ispartof>Research in astronomy and astrophysics, 2017-05, Vol.17 (6), p.101-106</ispartof><rights>2017 National Astronomical Observatories, CAS and IOP Publishing Ltd.</rights><rights>Copyright IOP Publishing May 2017</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c410t-290cd466932265f4b52f34de95618b9c2559bb6282bf3520c2894d6c629d0d1d3</citedby><cites>FETCH-LOGICAL-c410t-290cd466932265f4b52f34de95618b9c2559bb6282bf3520c2894d6c629d0d1d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Uhttp://image.cqvip.com/vip1000/qk/94947C/94947C.jpg</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1674-4527/17/6/60/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27901,27902,53821</link.rule.ids></links><search><creatorcontrib>Liu, Cheng-Chao</creatorcontrib><creatorcontrib>Ren, De-Qing</creatorcontrib><creatorcontrib>Zhu, Yong-Tian</creatorcontrib><creatorcontrib>Dou, Jiang-Pei</creatorcontrib><title>Design and experimental test of an optical vortex coronagraph</title><title>Research in astronomy and astrophysics</title><addtitle>Chinese Journal of Astronomy and Astrophysics</addtitle><description>Using an optical vortex coronagraph (OVC) is one of the most promising techniques for di- rectly imaging exoplanets because of its small inner working angle and high throughput. This paper presents the design and laboratory demonstration performance of an OVC based on liquid crystal polymers (LCPs) at 633 nm and 1520 nm. The OVC can deliver good performance in laboratory tests and achieve a contrast of 10-6 at an angular distance of 3A/D, which can be implemented for imaging young giant exoplanets in combination with extreme adaptive optics.</description><subject>Adaptive optics</subject><subject>Coronagraphs</subject><subject>Extrasolar planets</subject><subject>instrumentation: coronagraph</subject><subject>Laboratories</subject><subject>Laboratory tests</subject><subject>Liquid crystal polymers</subject><subject>Liquid crystals</subject><subject>methods: laboratory</subject><subject>Optics</subject><subject>Polymers</subject><subject>techniques: optical vortex</subject><subject>Vortices</subject><issn>1674-4527</issn><issn>2397-6209</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kE9PwzAMxSMEEmPwAbhVwLUscRqnOXBA4680iQucozZJu06j6dIOjW9Pq07jgjhZsn9-fn6EXDJ6y2iazhjKJE4EyBmTM5whPSIT4ErGCFQdk8lhfkrO2nZFKQqBMCF3D66tyjrKahu5XeNC9enqLltHnWu7yBf9IPJNV5m-9eVD53aR8cHXWRmyZnlOTops3bqLfZ2Sj6fH9_lLvHh7fp3fL2KTMNrFoKixCaLiACiKJBdQ8MQ6JZCluTIghMpzhBTyggugBlKVWDQIylLLLJ-S61G3CX6z7Z3pld-Guj-pgQsplEo47Sk2Uib4tg2u0E3_Tha-NaN6SEkPKeghBc2kRo3Dzs24U_nmVzRk2UhQpLqxRY_Ff2D_yV7trSx9XW6qujx4QQkcQSrgP6JofiY</recordid><startdate>20170501</startdate><enddate>20170501</enddate><creator>Liu, Cheng-Chao</creator><creator>Ren, De-Qing</creator><creator>Zhu, Yong-Tian</creator><creator>Dou, Jiang-Pei</creator><general>National Astronomical Observatories, CAS and IOP Publishing Ltd</general><general>IOP Publishing</general><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>W94</scope><scope>~WA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20170501</creationdate><title>Design and experimental test of an optical vortex coronagraph</title><author>Liu, Cheng-Chao ; Ren, De-Qing ; Zhu, Yong-Tian ; Dou, Jiang-Pei</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c410t-290cd466932265f4b52f34de95618b9c2559bb6282bf3520c2894d6c629d0d1d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Adaptive optics</topic><topic>Coronagraphs</topic><topic>Extrasolar planets</topic><topic>instrumentation: coronagraph</topic><topic>Laboratories</topic><topic>Laboratory tests</topic><topic>Liquid crystal polymers</topic><topic>Liquid crystals</topic><topic>methods: laboratory</topic><topic>Optics</topic><topic>Polymers</topic><topic>techniques: optical vortex</topic><topic>Vortices</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Liu, Cheng-Chao</creatorcontrib><creatorcontrib>Ren, De-Qing</creatorcontrib><creatorcontrib>Zhu, Yong-Tian</creatorcontrib><creatorcontrib>Dou, Jiang-Pei</creatorcontrib><collection>中文科技期刊数据库</collection><collection>中文科技期刊数据库-CALIS站点</collection><collection>中文科技期刊数据库-7.0平台</collection><collection>中文科技期刊数据库-自然科学</collection><collection>中文科技期刊数据库- 镜像站点</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Research in astronomy and astrophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Liu, Cheng-Chao</au><au>Ren, De-Qing</au><au>Zhu, Yong-Tian</au><au>Dou, Jiang-Pei</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Design and experimental test of an optical vortex coronagraph</atitle><jtitle>Research in astronomy and astrophysics</jtitle><addtitle>Chinese Journal of Astronomy and Astrophysics</addtitle><date>2017-05-01</date><risdate>2017</risdate><volume>17</volume><issue>6</issue><spage>101</spage><epage>106</epage><pages>101-106</pages><issn>1674-4527</issn><eissn>2397-6209</eissn><abstract>Using an optical vortex coronagraph (OVC) is one of the most promising techniques for di- rectly imaging exoplanets because of its small inner working angle and high throughput. This paper presents the design and laboratory demonstration performance of an OVC based on liquid crystal polymers (LCPs) at 633 nm and 1520 nm. The OVC can deliver good performance in laboratory tests and achieve a contrast of 10-6 at an angular distance of 3A/D, which can be implemented for imaging young giant exoplanets in combination with extreme adaptive optics.</abstract><cop>Beijing</cop><pub>National Astronomical Observatories, CAS and IOP Publishing Ltd</pub><doi>10.1088/1674-4527/17/6/60</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1674-4527 |
ispartof | Research in astronomy and astrophysics, 2017-05, Vol.17 (6), p.101-106 |
issn | 1674-4527 2397-6209 |
language | eng |
recordid | cdi_proquest_journals_2357599430 |
source | IOP Publishing Journals; Alma/SFX Local Collection |
subjects | Adaptive optics Coronagraphs Extrasolar planets instrumentation: coronagraph Laboratories Laboratory tests Liquid crystal polymers Liquid crystals methods: laboratory Optics Polymers techniques: optical vortex Vortices |
title | Design and experimental test of an optical vortex coronagraph |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-09T05%3A35%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_iop_j&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Design%20and%20experimental%20test%20of%20an%20optical%20vortex%20coronagraph&rft.jtitle=Research%20in%20astronomy%20and%20astrophysics&rft.au=Liu,%20Cheng-Chao&rft.date=2017-05-01&rft.volume=17&rft.issue=6&rft.spage=101&rft.epage=106&rft.pages=101-106&rft.issn=1674-4527&rft.eissn=2397-6209&rft_id=info:doi/10.1088/1674-4527/17/6/60&rft_dat=%3Cproquest_iop_j%3E2357599430%3C/proquest_iop_j%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2357599430&rft_id=info:pmid/&rft_cqvip_id=672362792&rfr_iscdi=true |