Solar imaging with a segmented adaptive mirror
A 19-segment adaptive-mirror system is currently being used on the Sacramento Peak 76-cm Tower Telescope to remove wave-front distortions resulting from atmospheric turbulence. The system has proven to be capable of substantially improving the quality of an image, at times achieving 0.33-arcsec reso...
Gespeichert in:
| Veröffentlicht in: | Applied Optics 1992-06, Vol.31 (16), p.3161-3169 |
|---|---|
| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 3169 |
|---|---|
| container_issue | 16 |
| container_start_page | 3161 |
| container_title | Applied Optics |
| container_volume | 31 |
| creator | ACTON, D. S SMITHSON, R. C |
| description | A 19-segment adaptive-mirror system is currently being used on the Sacramento Peak 76-cm Tower Telescope to remove wave-front distortions resulting from atmospheric turbulence. The system has proven to be capable of substantially improving the quality of an image, at times achieving 0.33-arcsec resolution in visible wavelengths under 1-3-arcsec seeing conditions. An improvement in resolution seems to occur across a large field of view that is, at times, 30 arcsec in diameter. |
| doi_str_mv | 10.1364/AO.31.003161 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_748967159</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>748967159</sourcerecordid><originalsourceid>FETCH-LOGICAL-c348t-476cae5806c052500c230a796ad2536b5b672441b21142e0f6b4ecd1180cf9573</originalsourceid><addsrcrecordid>eNp90MtLw0AQBvBFFFurN8-Sg-jFxJl9JsdSfEGhB_W8bDabGsmj7iaK_72R1h5lDgPDjw_mI-QcIUEm-e18lTBMABhKPCBTFCyLuaD0kExhvMYyY2JCTkJ4B0CayuyYTCgoKqjEKUmeu9r4qGrMumrX0VfVv0UmCm7duLZ3RWQKs-mrTxc1lfedPyVHpamDO9vtGXm9v3tZPMbL1cPTYr6MLeNpH3MlrXEiBWlBUAFgKQOjMmkKKpjMRS4V5Rxzisipg1Lm3NkCMQVbZkKxGbne5m589zG40OumCtbVtWldNwSteJpJhSIb5dW_kopUcMXFCG-20PouBO9KvfHj2_5bI-jfJvV8pRnqbZMjv9jlDnnjij3-q24ElztggjV16U1rq7B3nDE6DvsBBEZ3oA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>25854745</pqid></control><display><type>article</type><title>Solar imaging with a segmented adaptive mirror</title><source>Alma/SFX Local Collection</source><source>Optica Publishing Group Journals</source><creator>ACTON, D. S ; SMITHSON, R. C</creator><creatorcontrib>ACTON, D. S ; SMITHSON, R. C</creatorcontrib><description>A 19-segment adaptive-mirror system is currently being used on the Sacramento Peak 76-cm Tower Telescope to remove wave-front distortions resulting from atmospheric turbulence. The system has proven to be capable of substantially improving the quality of an image, at times achieving 0.33-arcsec resolution in visible wavelengths under 1-3-arcsec seeing conditions. An improvement in resolution seems to occur across a large field of view that is, at times, 30 arcsec in diameter.</description><identifier>ISSN: 0003-6935</identifier><identifier>ISSN: 1559-128X</identifier><identifier>EISSN: 1539-4522</identifier><identifier>DOI: 10.1364/AO.31.003161</identifier><identifier>PMID: 20725261</identifier><identifier>CODEN: APOPAI</identifier><language>eng</language><publisher>Washington, DC: Optical Society of America</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology ; Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</subject><ispartof>Applied Optics, 1992-06, Vol.31 (16), p.3161-3169</ispartof><rights>1993 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c348t-476cae5806c052500c230a796ad2536b5b672441b21142e0f6b4ecd1180cf9573</citedby><cites>FETCH-LOGICAL-c348t-476cae5806c052500c230a796ad2536b5b672441b21142e0f6b4ecd1180cf9573</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=4332323$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/20725261$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>ACTON, D. S</creatorcontrib><creatorcontrib>SMITHSON, R. C</creatorcontrib><title>Solar imaging with a segmented adaptive mirror</title><title>Applied Optics</title><addtitle>Appl Opt</addtitle><description>A 19-segment adaptive-mirror system is currently being used on the Sacramento Peak 76-cm Tower Telescope to remove wave-front distortions resulting from atmospheric turbulence. The system has proven to be capable of substantially improving the quality of an image, at times achieving 0.33-arcsec resolution in visible wavelengths under 1-3-arcsec seeing conditions. An improvement in resolution seems to occur across a large field of view that is, at times, 30 arcsec in diameter.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</subject><issn>0003-6935</issn><issn>1559-128X</issn><issn>1539-4522</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1992</creationdate><recordtype>article</recordtype><recordid>eNp90MtLw0AQBvBFFFurN8-Sg-jFxJl9JsdSfEGhB_W8bDabGsmj7iaK_72R1h5lDgPDjw_mI-QcIUEm-e18lTBMABhKPCBTFCyLuaD0kExhvMYyY2JCTkJ4B0CayuyYTCgoKqjEKUmeu9r4qGrMumrX0VfVv0UmCm7duLZ3RWQKs-mrTxc1lfedPyVHpamDO9vtGXm9v3tZPMbL1cPTYr6MLeNpH3MlrXEiBWlBUAFgKQOjMmkKKpjMRS4V5Rxzisipg1Lm3NkCMQVbZkKxGbne5m589zG40OumCtbVtWldNwSteJpJhSIb5dW_kopUcMXFCG-20PouBO9KvfHj2_5bI-jfJvV8pRnqbZMjv9jlDnnjij3-q24ElztggjV16U1rq7B3nDE6DvsBBEZ3oA</recordid><startdate>19920601</startdate><enddate>19920601</enddate><creator>ACTON, D. S</creator><creator>SMITHSON, R. C</creator><general>Optical Society of America</general><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope></search><sort><creationdate>19920601</creationdate><title>Solar imaging with a segmented adaptive mirror</title><author>ACTON, D. S ; SMITHSON, R. C</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c348t-476cae5806c052500c230a796ad2536b5b672441b21142e0f6b4ecd1180cf9573</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1992</creationdate><topic>Astronomy</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>ACTON, D. S</creatorcontrib><creatorcontrib>SMITHSON, R. C</creatorcontrib><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><jtitle>Applied Optics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ACTON, D. S</au><au>SMITHSON, R. C</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Solar imaging with a segmented adaptive mirror</atitle><jtitle>Applied Optics</jtitle><addtitle>Appl Opt</addtitle><date>1992-06-01</date><risdate>1992</risdate><volume>31</volume><issue>16</issue><spage>3161</spage><epage>3169</epage><pages>3161-3169</pages><issn>0003-6935</issn><issn>1559-128X</issn><eissn>1539-4522</eissn><coden>APOPAI</coden><abstract>A 19-segment adaptive-mirror system is currently being used on the Sacramento Peak 76-cm Tower Telescope to remove wave-front distortions resulting from atmospheric turbulence. The system has proven to be capable of substantially improving the quality of an image, at times achieving 0.33-arcsec resolution in visible wavelengths under 1-3-arcsec seeing conditions. An improvement in resolution seems to occur across a large field of view that is, at times, 30 arcsec in diameter.</abstract><cop>Washington, DC</cop><pub>Optical Society of America</pub><pmid>20725261</pmid><doi>10.1364/AO.31.003161</doi><tpages>9</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0003-6935 |
| ispartof | Applied Optics, 1992-06, Vol.31 (16), p.3161-3169 |
| issn | 0003-6935 1559-128X 1539-4522 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_748967159 |
| source | Alma/SFX Local Collection; Optica Publishing Group Journals |
| subjects | Astronomy Earth, ocean, space Exact sciences and technology Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations |
| title | Solar imaging with a segmented adaptive mirror |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-13T13%3A31%3A35IST&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=Solar%20imaging%20with%20a%20segmented%20adaptive%20mirror&rft.jtitle=Applied%20Optics&rft.au=ACTON,%20D.%20S&rft.date=1992-06-01&rft.volume=31&rft.issue=16&rft.spage=3161&rft.epage=3169&rft.pages=3161-3169&rft.issn=0003-6935&rft.eissn=1539-4522&rft.coden=APOPAI&rft_id=info:doi/10.1364/AO.31.003161&rft_dat=%3Cproquest_cross%3E748967159%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=25854745&rft_id=info:pmid/20725261&rfr_iscdi=true |