Refractive lenses for coherent x-ray sources
Incoherent x rays in the wavelength interval from approximately 0.5-2 A have been focused with refractive lenses. A single lens would have a long focal length because the refractive index of any material is close to unity; but with a stack of N lens elements the focal length is reduced by the factor...
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Veröffentlicht in: | Appl.Opt.40:5100,2001 2001, 2001-10, Vol.40 (28), p.5100-5105 |
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creator | Pantell, R H Feinstein, J Beguiristain, H R Piestrup, M A Gary, C K Cremer, J T |
description | Incoherent x rays in the wavelength interval from approximately 0.5-2 A have been focused with refractive lenses. A single lens would have a long focal length because the refractive index of any material is close to unity; but with a stack of N lens elements the focal length is reduced by the factor N, and such a lens is termed a compound refractive lens (CRL). Misalignment of the parabolic lens elements does not alter the focusing properties and results in only a small reduction in transmission. Based on the principle of spontaneous emission amplification in a FEL wiggler, coherent x-ray sources are being developed with wavelengths of 1-1.5 A and source diameters of 50-80 mum; and the CRL can be used to provide a small, intense image. Chromatic aberration increases the image size by an amount comparable with the diffraction-limited size, and so chromatic correction is important. Pulse broadening through the lens that is due to material dispersion is negligible. The performance of a CRL used in conjunction with a coherent source is analyzed by means of the Kirchhoff integral. For typical parameters, intensity gain is 10(5)-10(6), where gain is defined as the intensity ratio in an image plane with and without the lens in place. (There may be some confusion concerning the usage of the word intensity. As employed in this manuscript, intensity, also called irradiance, refers to power per unit area. This is a commonly accepted usage for intensity, although there are places in the literature where the term radiant incidence is reserved for this definition and intensity refers to power per unit solid angle.) The image intensity is maximized when the CRL is placed 100-200 m from the source, and the diameter of the diffraction-limited spot is approximately 0.12 mum. |
doi_str_mv | 10.1364/AO.40.005100 |
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Pulse broadening through the lens that is due to material dispersion is negligible. The performance of a CRL used in conjunction with a coherent source is analyzed by means of the Kirchhoff integral. For typical parameters, intensity gain is 10(5)-10(6), where gain is defined as the intensity ratio in an image plane with and without the lens in place. (There may be some confusion concerning the usage of the word intensity. As employed in this manuscript, intensity, also called irradiance, refers to power per unit area. This is a commonly accepted usage for intensity, although there are places in the literature where the term radiant incidence is reserved for this definition and intensity refers to power per unit solid angle.) The image intensity is maximized when the CRL is placed 100-200 m from the source, and the diameter of the diffraction-limited spot is approximately 0.12 mum.</description><identifier>ISSN: 1559-128X</identifier><identifier>ISSN: 0003-6935</identifier><identifier>EISSN: 1539-4522</identifier><identifier>DOI: 10.1364/AO.40.005100</identifier><identifier>PMID: 18364790</identifier><language>eng</language><publisher>United States</publisher><subject>LENSES ; PARTICLE ACCELERATORS ; REFRACTION ; STANFORD LINEAR ACCELERATOR CENTER ; STANFORD SYNCHROTRON RADIATION LABORATORY ; SYNCHROTRON RADIATION ; X-RAY SOURCES</subject><ispartof>Appl.Opt.40:5100,2001, 2001-10, Vol.40 (28), p.5100-5105</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c314t-4663b22c3a84ef60785e543ea4d4c15c39951399c7bf3cd66dfd6365168e4ae43</citedby><cites>FETCH-LOGICAL-c314t-4663b22c3a84ef60785e543ea4d4c15c39951399c7bf3cd66dfd6365168e4ae43</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,882,27905,27906</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/18364790$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/802460$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Pantell, R H</creatorcontrib><creatorcontrib>Feinstein, J</creatorcontrib><creatorcontrib>Beguiristain, H R</creatorcontrib><creatorcontrib>Piestrup, M A</creatorcontrib><creatorcontrib>Gary, C K</creatorcontrib><creatorcontrib>Cremer, J T</creatorcontrib><creatorcontrib>Stanford Synchrotron Radiation Lab. (US)</creatorcontrib><creatorcontrib>Stanford Linear Accelerator Center, Menlo Park, CA (US)</creatorcontrib><title>Refractive lenses for coherent x-ray sources</title><title>Appl.Opt.40:5100,2001</title><addtitle>Appl Opt</addtitle><description>Incoherent x rays in the wavelength interval from approximately 0.5-2 A have been focused with refractive lenses. A single lens would have a long focal length because the refractive index of any material is close to unity; but with a stack of N lens elements the focal length is reduced by the factor N, and such a lens is termed a compound refractive lens (CRL). Misalignment of the parabolic lens elements does not alter the focusing properties and results in only a small reduction in transmission. Based on the principle of spontaneous emission amplification in a FEL wiggler, coherent x-ray sources are being developed with wavelengths of 1-1.5 A and source diameters of 50-80 mum; and the CRL can be used to provide a small, intense image. Chromatic aberration increases the image size by an amount comparable with the diffraction-limited size, and so chromatic correction is important. Pulse broadening through the lens that is due to material dispersion is negligible. The performance of a CRL used in conjunction with a coherent source is analyzed by means of the Kirchhoff integral. For typical parameters, intensity gain is 10(5)-10(6), where gain is defined as the intensity ratio in an image plane with and without the lens in place. (There may be some confusion concerning the usage of the word intensity. As employed in this manuscript, intensity, also called irradiance, refers to power per unit area. This is a commonly accepted usage for intensity, although there are places in the literature where the term radiant incidence is reserved for this definition and intensity refers to power per unit solid angle.) The image intensity is maximized when the CRL is placed 100-200 m from the source, and the diameter of the diffraction-limited spot is approximately 0.12 mum.</description><subject>LENSES</subject><subject>PARTICLE ACCELERATORS</subject><subject>REFRACTION</subject><subject>STANFORD LINEAR ACCELERATOR CENTER</subject><subject>STANFORD SYNCHROTRON RADIATION LABORATORY</subject><subject>SYNCHROTRON RADIATION</subject><subject>X-RAY SOURCES</subject><issn>1559-128X</issn><issn>0003-6935</issn><issn>1539-4522</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><recordid>eNpFkE1Lw0AQQBdRbK3ePEs8eWnqbnZ2kxxL8QsKBVHwtmwnExpJs3U3kfbfm5KCl5k5vHmHx9it4DMhNTzOVzPgM86V4PyMjYWSeQwqSc6Pt8pjkWRfI3YVwjfnUkGeXrKRyPrPNOdjNn2n0ltsq1-KamoChah0PkK3IU9NG-1jbw9RcJ1HCtfsorR1oJvTnrDP56ePxWu8XL28LebLGKWANgat5TpJUNoMqNQ8zRQpkGShABQKZZ4r0Q9M16XEQuuiLLTUSuiMwBLICbsfvC60lQlYtYQbdE1D2JqMJ6B5zzwMzM67n45Ca7ZVQKpr25DrgkklJGmvTHtyOpDoXQieSrPz1db6gxHcHBOa-coAN0PCHr87ibv1lop_-NRM_gFyxmmZ</recordid><startdate>20011001</startdate><enddate>20011001</enddate><creator>Pantell, R H</creator><creator>Feinstein, J</creator><creator>Beguiristain, H R</creator><creator>Piestrup, M A</creator><creator>Gary, C K</creator><creator>Cremer, J T</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>20011001</creationdate><title>Refractive lenses for coherent x-ray sources</title><author>Pantell, R H ; Feinstein, J ; Beguiristain, H R ; Piestrup, M A ; Gary, C K ; Cremer, J T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c314t-4663b22c3a84ef60785e543ea4d4c15c39951399c7bf3cd66dfd6365168e4ae43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>LENSES</topic><topic>PARTICLE ACCELERATORS</topic><topic>REFRACTION</topic><topic>STANFORD LINEAR ACCELERATOR CENTER</topic><topic>STANFORD SYNCHROTRON RADIATION LABORATORY</topic><topic>SYNCHROTRON RADIATION</topic><topic>X-RAY SOURCES</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pantell, R H</creatorcontrib><creatorcontrib>Feinstein, J</creatorcontrib><creatorcontrib>Beguiristain, H R</creatorcontrib><creatorcontrib>Piestrup, M A</creatorcontrib><creatorcontrib>Gary, C K</creatorcontrib><creatorcontrib>Cremer, J T</creatorcontrib><creatorcontrib>Stanford Synchrotron Radiation Lab. (US)</creatorcontrib><creatorcontrib>Stanford Linear Accelerator Center, Menlo Park, CA (US)</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Appl.Opt.40:5100,2001</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pantell, R H</au><au>Feinstein, J</au><au>Beguiristain, H R</au><au>Piestrup, M A</au><au>Gary, C K</au><au>Cremer, J T</au><aucorp>Stanford Synchrotron Radiation Lab. (US)</aucorp><aucorp>Stanford Linear Accelerator Center, Menlo Park, CA (US)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Refractive lenses for coherent x-ray sources</atitle><jtitle>Appl.Opt.40:5100,2001</jtitle><addtitle>Appl Opt</addtitle><date>2001-10-01</date><risdate>2001</risdate><volume>40</volume><issue>28</issue><spage>5100</spage><epage>5105</epage><pages>5100-5105</pages><issn>1559-128X</issn><issn>0003-6935</issn><eissn>1539-4522</eissn><abstract>Incoherent x rays in the wavelength interval from approximately 0.5-2 A have been focused with refractive lenses. A single lens would have a long focal length because the refractive index of any material is close to unity; but with a stack of N lens elements the focal length is reduced by the factor N, and such a lens is termed a compound refractive lens (CRL). Misalignment of the parabolic lens elements does not alter the focusing properties and results in only a small reduction in transmission. Based on the principle of spontaneous emission amplification in a FEL wiggler, coherent x-ray sources are being developed with wavelengths of 1-1.5 A and source diameters of 50-80 mum; and the CRL can be used to provide a small, intense image. Chromatic aberration increases the image size by an amount comparable with the diffraction-limited size, and so chromatic correction is important. Pulse broadening through the lens that is due to material dispersion is negligible. The performance of a CRL used in conjunction with a coherent source is analyzed by means of the Kirchhoff integral. For typical parameters, intensity gain is 10(5)-10(6), where gain is defined as the intensity ratio in an image plane with and without the lens in place. (There may be some confusion concerning the usage of the word intensity. As employed in this manuscript, intensity, also called irradiance, refers to power per unit area. This is a commonly accepted usage for intensity, although there are places in the literature where the term radiant incidence is reserved for this definition and intensity refers to power per unit solid angle.) The image intensity is maximized when the CRL is placed 100-200 m from the source, and the diameter of the diffraction-limited spot is approximately 0.12 mum.</abstract><cop>United States</cop><pmid>18364790</pmid><doi>10.1364/AO.40.005100</doi><tpages>6</tpages></addata></record> |
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subjects | LENSES PARTICLE ACCELERATORS REFRACTION STANFORD LINEAR ACCELERATOR CENTER STANFORD SYNCHROTRON RADIATION LABORATORY SYNCHROTRON RADIATION X-RAY SOURCES |
title | Refractive lenses for coherent x-ray sources |
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