Experimental assessment of the matched filter for laser guide star wavefront sensing

Laser guide star wavefront sensing comes with several limitations. When imaged with a Shack-Hartmann wavefront sensor, the laser guide star is seen as extended sources elongated in the directions given by the lenslet locations and the laser axis. A test bed has been built in the Adaptive Optics Labo...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Applied Optics 2009-02, Vol.48 (6), p.1198-1211
Hauptverfasser: Conan, Rodolphe, Lardière, Olivier, Herriot, Glen, Bradley, Colin, Jackson, Kate
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1211
container_issue 6
container_start_page 1198
container_title Applied Optics
container_volume 48
creator Conan, Rodolphe
Lardière, Olivier
Herriot, Glen
Bradley, Colin
Jackson, Kate
description Laser guide star wavefront sensing comes with several limitations. When imaged with a Shack-Hartmann wavefront sensor, the laser guide star is seen as extended sources elongated in the directions given by the lenslet locations and the laser axis. A test bed has been built in the Adaptive Optics Laboratory of the University of Victoria that reproduces this effect as seen on extremely large telescopes. A new wavefront sensing algorithm, the matched filter, has been implemented and its performance assessed with the test bed. Its ability to mitigate laser guide star aberrations by tracking the sodium layer fluctuations in a closed loop adaptive optics system is shown.
doi_str_mv 10.1364/AO.48.001198
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1325329676</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>754865829</sourcerecordid><originalsourceid>FETCH-LOGICAL-c323t-abf6e31e7987402ff10b520e9e82248dbf8b7c810e7ef6ab51a3af783af12b0a3</originalsourceid><addsrcrecordid>eNp9kLtPwzAQhy0EolDYmJE3GEjxM3bGqioPqVKXIrFZTnJug_IodsLjv8dVCyPL3e-k7066D6ErSiaUp-J-upwIPSGE0kwfoTMqeZYIydjxLsssoUy_jtB5CG-EcCkydYpGjMtUSc3O0Gr-tQVfNdD2tsY2BAhhN-DO4X4DuLF9sYESu6ruwWPXeVzbENN6qErAobcef9oPcL6LSwHaULXrC3TibB3g8tDH6OVhvpo9JYvl4_NsukgKznif2NylwCmoTCtBmHOU5JIRyEAzJnSZO52rQlMCClxqc0ktt07pWCjLieVjdLO_u_Xd-wChN00VCqhr20I3BKOk0Gl8M4vk7b8k5UxylqUqjejdHi18F4IHZ7bRj_XfhhKzM26mSyO02RuP-PXh8pA3UP7Bv4r5D1ZufEc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1325329676</pqid></control><display><type>article</type><title>Experimental assessment of the matched filter for laser guide star wavefront sensing</title><source>Alma/SFX Local Collection</source><source>Optica Publishing Group Journals</source><creator>Conan, Rodolphe ; Lardière, Olivier ; Herriot, Glen ; Bradley, Colin ; Jackson, Kate</creator><creatorcontrib>Conan, Rodolphe ; Lardière, Olivier ; Herriot, Glen ; Bradley, Colin ; Jackson, Kate</creatorcontrib><description>Laser guide star wavefront sensing comes with several limitations. When imaged with a Shack-Hartmann wavefront sensor, the laser guide star is seen as extended sources elongated in the directions given by the lenslet locations and the laser axis. A test bed has been built in the Adaptive Optics Laboratory of the University of Victoria that reproduces this effect as seen on extremely large telescopes. A new wavefront sensing algorithm, the matched filter, has been implemented and its performance assessed with the test bed. Its ability to mitigate laser guide star aberrations by tracking the sodium layer fluctuations in a closed loop adaptive optics system is shown.</description><identifier>ISSN: 1559-128X</identifier><identifier>ISSN: 0003-6935</identifier><identifier>EISSN: 1539-4522</identifier><identifier>DOI: 10.1364/AO.48.001198</identifier><identifier>PMID: 23567582</identifier><language>eng</language><publisher>United States</publisher><ispartof>Applied Optics, 2009-02, Vol.48 (6), p.1198-1211</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c323t-abf6e31e7987402ff10b520e9e82248dbf8b7c810e7ef6ab51a3af783af12b0a3</citedby><cites>FETCH-LOGICAL-c323t-abf6e31e7987402ff10b520e9e82248dbf8b7c810e7ef6ab51a3af783af12b0a3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/23567582$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Conan, Rodolphe</creatorcontrib><creatorcontrib>Lardière, Olivier</creatorcontrib><creatorcontrib>Herriot, Glen</creatorcontrib><creatorcontrib>Bradley, Colin</creatorcontrib><creatorcontrib>Jackson, Kate</creatorcontrib><title>Experimental assessment of the matched filter for laser guide star wavefront sensing</title><title>Applied Optics</title><addtitle>Appl Opt</addtitle><description>Laser guide star wavefront sensing comes with several limitations. When imaged with a Shack-Hartmann wavefront sensor, the laser guide star is seen as extended sources elongated in the directions given by the lenslet locations and the laser axis. A test bed has been built in the Adaptive Optics Laboratory of the University of Victoria that reproduces this effect as seen on extremely large telescopes. A new wavefront sensing algorithm, the matched filter, has been implemented and its performance assessed with the test bed. Its ability to mitigate laser guide star aberrations by tracking the sodium layer fluctuations in a closed loop adaptive optics system is shown.</description><issn>1559-128X</issn><issn>0003-6935</issn><issn>1539-4522</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><recordid>eNp9kLtPwzAQhy0EolDYmJE3GEjxM3bGqioPqVKXIrFZTnJug_IodsLjv8dVCyPL3e-k7066D6ErSiaUp-J-upwIPSGE0kwfoTMqeZYIydjxLsssoUy_jtB5CG-EcCkydYpGjMtUSc3O0Gr-tQVfNdD2tsY2BAhhN-DO4X4DuLF9sYESu6ruwWPXeVzbENN6qErAobcef9oPcL6LSwHaULXrC3TibB3g8tDH6OVhvpo9JYvl4_NsukgKznif2NylwCmoTCtBmHOU5JIRyEAzJnSZO52rQlMCClxqc0ktt07pWCjLieVjdLO_u_Xd-wChN00VCqhr20I3BKOk0Gl8M4vk7b8k5UxylqUqjejdHi18F4IHZ7bRj_XfhhKzM26mSyO02RuP-PXh8pA3UP7Bv4r5D1ZufEc</recordid><startdate>20090220</startdate><enddate>20090220</enddate><creator>Conan, Rodolphe</creator><creator>Lardière, Olivier</creator><creator>Herriot, Glen</creator><creator>Bradley, Colin</creator><creator>Jackson, Kate</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20090220</creationdate><title>Experimental assessment of the matched filter for laser guide star wavefront sensing</title><author>Conan, Rodolphe ; Lardière, Olivier ; Herriot, Glen ; Bradley, Colin ; Jackson, Kate</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c323t-abf6e31e7987402ff10b520e9e82248dbf8b7c810e7ef6ab51a3af783af12b0a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Conan, Rodolphe</creatorcontrib><creatorcontrib>Lardière, Olivier</creatorcontrib><creatorcontrib>Herriot, Glen</creatorcontrib><creatorcontrib>Bradley, Colin</creatorcontrib><creatorcontrib>Jackson, Kate</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><jtitle>Applied Optics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Conan, Rodolphe</au><au>Lardière, Olivier</au><au>Herriot, Glen</au><au>Bradley, Colin</au><au>Jackson, Kate</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Experimental assessment of the matched filter for laser guide star wavefront sensing</atitle><jtitle>Applied Optics</jtitle><addtitle>Appl Opt</addtitle><date>2009-02-20</date><risdate>2009</risdate><volume>48</volume><issue>6</issue><spage>1198</spage><epage>1211</epage><pages>1198-1211</pages><issn>1559-128X</issn><issn>0003-6935</issn><eissn>1539-4522</eissn><abstract>Laser guide star wavefront sensing comes with several limitations. When imaged with a Shack-Hartmann wavefront sensor, the laser guide star is seen as extended sources elongated in the directions given by the lenslet locations and the laser axis. A test bed has been built in the Adaptive Optics Laboratory of the University of Victoria that reproduces this effect as seen on extremely large telescopes. A new wavefront sensing algorithm, the matched filter, has been implemented and its performance assessed with the test bed. Its ability to mitigate laser guide star aberrations by tracking the sodium layer fluctuations in a closed loop adaptive optics system is shown.</abstract><cop>United States</cop><pmid>23567582</pmid><doi>10.1364/AO.48.001198</doi><tpages>14</tpages></addata></record>
fulltext fulltext
identifier ISSN: 1559-128X
ispartof Applied Optics, 2009-02, Vol.48 (6), p.1198-1211
issn 1559-128X
0003-6935
1539-4522
language eng
recordid cdi_proquest_miscellaneous_1325329676
source Alma/SFX Local Collection; Optica Publishing Group Journals
title Experimental assessment of the matched filter for laser guide star wavefront sensing
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T22%3A55%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Experimental%20assessment%20of%20the%20matched%20filter%20for%20laser%20guide%20star%20wavefront%20sensing&rft.jtitle=Applied%20Optics&rft.au=Conan,%20Rodolphe&rft.date=2009-02-20&rft.volume=48&rft.issue=6&rft.spage=1198&rft.epage=1211&rft.pages=1198-1211&rft.issn=1559-128X&rft.eissn=1539-4522&rft_id=info:doi/10.1364/AO.48.001198&rft_dat=%3Cproquest_cross%3E754865829%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1325329676&rft_id=info:pmid/23567582&rfr_iscdi=true