Direct and inverse problems for light scattered by rough surfaces

Calculations are performed to relate the stylus profile of a one-dimensionally rough surface to the angular distribution of the light scattered by such a surface. In the direct problem, the angular distribution of the scattered light calculated from the profile is shown to agree with the measured on...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Applied Optics 1990-09, Vol.29 (25), p.3613-3626
Hauptverfasser: MARX, E, VORBURGER, T. V
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 3626
container_issue 25
container_start_page 3613
container_title Applied Optics
container_volume 29
creator MARX, E
VORBURGER, T. V
description Calculations are performed to relate the stylus profile of a one-dimensionally rough surface to the angular distribution of the light scattered by such a surface. In the direct problem, the angular distribution of the scattered light calculated from the profile is shown to agree with the measured one. In the inverse problem, the rms roughness and the autocorrelation function are found by a least-squares fit to the measured angular distribution. For the smoother surfaces, the rms roughness is mostly determined by the ratio between the power of the specular beam and the total power of the scattered light; the computed values are proportional to those calculated directly from the stylus profiles. The values of the parameters obtained by the least-squares fit are affected by a variety of errors and agree only partially with those obtained from the stylus profile.
doi_str_mv 10.1364/ao.29.003613
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_733371939</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>733371939</sourcerecordid><originalsourceid>FETCH-LOGICAL-c383t-116427c907828b3dfe0cc426b5129eb0351dd40e1874fd51e1a0e9120d9f61793</originalsourceid><addsrcrecordid>eNo90E1Lw0AQgOFFFFurN8-yB8GLqTv7leyx1E8o9KLnsNnMtpGkqbuJ0H9vSmtPA8PDMLyE3AKbgtDyybZTbqaMCQ3ijIxBCZNIxfk5GbNhm2gj1IhcxfjNGPBMm0sy4kzpVGoYk9lzFdB11G5KWm1-MUSk29AWNTaR-jbQulqtOxqd7ToMWNJiR0Pbr9Y09sFbh_GaXHhbR7w5zgn5en35nL8ni-Xbx3y2SJzIRJcAaMlTZ1ia8awQpUfmnOS6UMANFkwoKEvJELJU-lIBgmVogLPSeA2pERPycLg7vPfTY-zypooO69pusO1jngohUjBiLx8P0oU2xoA-34aqsWGXA8v3zfLZMucmPzQb-N3xcF80WJ7wf6QB3B-BHTrUPtiNq-LJKckN45n4AynuciI</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>733371939</pqid></control><display><type>article</type><title>Direct and inverse problems for light scattered by rough surfaces</title><source>Alma/SFX Local Collection</source><source>Optica Publishing Group Journals</source><creator>MARX, E ; VORBURGER, T. V</creator><creatorcontrib>MARX, E ; VORBURGER, T. V</creatorcontrib><description>Calculations are performed to relate the stylus profile of a one-dimensionally rough surface to the angular distribution of the light scattered by such a surface. In the direct problem, the angular distribution of the scattered light calculated from the profile is shown to agree with the measured one. In the inverse problem, the rms roughness and the autocorrelation function are found by a least-squares fit to the measured angular distribution. For the smoother surfaces, the rms roughness is mostly determined by the ratio between the power of the specular beam and the total power of the scattered light; the computed values are proportional to those calculated directly from the stylus profiles. The values of the parameters obtained by the least-squares fit are affected by a variety of errors and agree only partially with those obtained from the stylus profile.</description><identifier>ISSN: 0003-6935</identifier><identifier>ISSN: 1559-128X</identifier><identifier>EISSN: 1539-4522</identifier><identifier>DOI: 10.1364/ao.29.003613</identifier><identifier>PMID: 20567461</identifier><identifier>CODEN: APOPAI</identifier><language>eng</language><publisher>Washington, DC: Optical Society of America</publisher><subject>Exact sciences and technology ; Fundamental areas of phenomenology (including applications) ; Optics ; Physics ; Wave optics ; Wave propagation, transmission and absorption</subject><ispartof>Applied Optics, 1990-09, Vol.29 (25), p.3613-3626</ispartof><rights>1992 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c383t-116427c907828b3dfe0cc426b5129eb0351dd40e1874fd51e1a0e9120d9f61793</citedby><cites>FETCH-LOGICAL-c383t-116427c907828b3dfe0cc426b5129eb0351dd40e1874fd51e1a0e9120d9f61793</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=5429028$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/20567461$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>MARX, E</creatorcontrib><creatorcontrib>VORBURGER, T. V</creatorcontrib><title>Direct and inverse problems for light scattered by rough surfaces</title><title>Applied Optics</title><addtitle>Appl Opt</addtitle><description>Calculations are performed to relate the stylus profile of a one-dimensionally rough surface to the angular distribution of the light scattered by such a surface. In the direct problem, the angular distribution of the scattered light calculated from the profile is shown to agree with the measured one. In the inverse problem, the rms roughness and the autocorrelation function are found by a least-squares fit to the measured angular distribution. For the smoother surfaces, the rms roughness is mostly determined by the ratio between the power of the specular beam and the total power of the scattered light; the computed values are proportional to those calculated directly from the stylus profiles. The values of the parameters obtained by the least-squares fit are affected by a variety of errors and agree only partially with those obtained from the stylus profile.</description><subject>Exact sciences and technology</subject><subject>Fundamental areas of phenomenology (including applications)</subject><subject>Optics</subject><subject>Physics</subject><subject>Wave optics</subject><subject>Wave propagation, transmission and absorption</subject><issn>0003-6935</issn><issn>1559-128X</issn><issn>1539-4522</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1990</creationdate><recordtype>article</recordtype><recordid>eNo90E1Lw0AQgOFFFFurN8-yB8GLqTv7leyx1E8o9KLnsNnMtpGkqbuJ0H9vSmtPA8PDMLyE3AKbgtDyybZTbqaMCQ3ijIxBCZNIxfk5GbNhm2gj1IhcxfjNGPBMm0sy4kzpVGoYk9lzFdB11G5KWm1-MUSk29AWNTaR-jbQulqtOxqd7ToMWNJiR0Pbr9Y09sFbh_GaXHhbR7w5zgn5en35nL8ni-Xbx3y2SJzIRJcAaMlTZ1ia8awQpUfmnOS6UMANFkwoKEvJELJU-lIBgmVogLPSeA2pERPycLg7vPfTY-zypooO69pusO1jngohUjBiLx8P0oU2xoA-34aqsWGXA8v3zfLZMucmPzQb-N3xcF80WJ7wf6QB3B-BHTrUPtiNq-LJKckN45n4AynuciI</recordid><startdate>19900901</startdate><enddate>19900901</enddate><creator>MARX, E</creator><creator>VORBURGER, T. V</creator><general>Optical Society of America</general><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>19900901</creationdate><title>Direct and inverse problems for light scattered by rough surfaces</title><author>MARX, E ; VORBURGER, T. V</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c383t-116427c907828b3dfe0cc426b5129eb0351dd40e1874fd51e1a0e9120d9f61793</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1990</creationdate><topic>Exact sciences and technology</topic><topic>Fundamental areas of phenomenology (including applications)</topic><topic>Optics</topic><topic>Physics</topic><topic>Wave optics</topic><topic>Wave propagation, transmission and absorption</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>MARX, E</creatorcontrib><creatorcontrib>VORBURGER, T. V</creatorcontrib><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Applied Optics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>MARX, E</au><au>VORBURGER, T. V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Direct and inverse problems for light scattered by rough surfaces</atitle><jtitle>Applied Optics</jtitle><addtitle>Appl Opt</addtitle><date>1990-09-01</date><risdate>1990</risdate><volume>29</volume><issue>25</issue><spage>3613</spage><epage>3626</epage><pages>3613-3626</pages><issn>0003-6935</issn><issn>1559-128X</issn><eissn>1539-4522</eissn><coden>APOPAI</coden><abstract>Calculations are performed to relate the stylus profile of a one-dimensionally rough surface to the angular distribution of the light scattered by such a surface. In the direct problem, the angular distribution of the scattered light calculated from the profile is shown to agree with the measured one. In the inverse problem, the rms roughness and the autocorrelation function are found by a least-squares fit to the measured angular distribution. For the smoother surfaces, the rms roughness is mostly determined by the ratio between the power of the specular beam and the total power of the scattered light; the computed values are proportional to those calculated directly from the stylus profiles. The values of the parameters obtained by the least-squares fit are affected by a variety of errors and agree only partially with those obtained from the stylus profile.</abstract><cop>Washington, DC</cop><pub>Optical Society of America</pub><pmid>20567461</pmid><doi>10.1364/ao.29.003613</doi><tpages>14</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0003-6935
ispartof Applied Optics, 1990-09, Vol.29 (25), p.3613-3626
issn 0003-6935
1559-128X
1539-4522
language eng
recordid cdi_proquest_miscellaneous_733371939
source Alma/SFX Local Collection; Optica Publishing Group Journals
subjects Exact sciences and technology
Fundamental areas of phenomenology (including applications)
Optics
Physics
Wave optics
Wave propagation, transmission and absorption
title Direct and inverse problems for light scattered by rough surfaces
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-06T20%3A19%3A46IST&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=Direct%20and%20inverse%20problems%20for%20light%20scattered%20by%20rough%20surfaces&rft.jtitle=Applied%20Optics&rft.au=MARX,%20E&rft.date=1990-09-01&rft.volume=29&rft.issue=25&rft.spage=3613&rft.epage=3626&rft.pages=3613-3626&rft.issn=0003-6935&rft.eissn=1539-4522&rft.coden=APOPAI&rft_id=info:doi/10.1364/ao.29.003613&rft_dat=%3Cproquest_cross%3E733371939%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=733371939&rft_id=info:pmid/20567461&rfr_iscdi=true