Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption
Identifieur interne : 000305 ( Istex/Corpus ); précédent : 000304; suivant : 000306Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption
Auteurs : H. C. Burger ; P. H. Van CittertSource :
- Physica [ 0031-8914 ] ; 1938.
Abstract
The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines 199 and 201 coincide with the lines 198 and 200 resp.
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DOI: 10.1016/S0031-8914(38)80058-6
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Van Cittert</name><affiliation><mods:affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</mods:affiliation></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:EB88320B8CF5631A02CD2125922A1ADF7AF186D9</idno><date when="1938" year="1938">1938</date><idno type="doi">10.1016/S0031-8914(38)80058-6</idno><idno type="url">https://api.istex.fr/document/EB88320B8CF5631A02CD2125922A1ADF7AF186D9/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">000305</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">000305</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption</title><author><name sortKey="Burger, H C" sort="Burger, H C" uniqKey="Burger H" first="H. C." last="Burger">H. C. Burger</name><affiliation><mods:affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</mods:affiliation></affiliation></author><author><name sortKey="Van Cittert, P H" sort="Van Cittert, P H" uniqKey="Van Cittert P" first="P. H." last="Van Cittert">P. H. Van Cittert</name><affiliation><mods:affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Physica</title><title level="j" type="abbrev">PHYSIC</title><idno type="ISSN">0031-8914</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1938">1938</date><biblScope unit="volume">5</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="177">177</biblScope><biblScope unit="page" to="187">187</biblScope></imprint><idno type="ISSN">0031-8914</idno></series><idno type="istex">EB88320B8CF5631A02CD2125922A1ADF7AF186D9</idno><idno type="DOI">10.1016/S0031-8914(38)80058-6</idno><idno type="PII">S0031-8914(38)80058-6</idno><idno type="ArticleID">38800586</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0031-8914</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines 199 and 201 coincide with the lines 198 and 200 resp.</div></front></TEI><istex><corpusName>elsevier</corpusName><author><json:item><name>H.C. Burger</name><affiliations><json:string>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</json:string></affiliations></json:item><json:item><name>P.H. van Cittert</name><affiliations><json:string>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</json:string></affiliations></json:item></author><articleId><json:string>38800586</json:string></articleId><language><json:string>eng</json:string></language><abstract>The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines 199 and 201 coincide with the lines 198 and 200 resp.</abstract><qualityIndicators><score>4.384</score><pdfVersion>1.3</pdfVersion><pdfPageSize>432 x 648 pts</pdfPageSize><refBibsNative>true</refBibsNative><keywordCount>0</keywordCount><abstractCharCount>394</abstractCharCount><pdfWordCount>3604</pdfWordCount><pdfCharCount>15543</pdfCharCount><pdfPageCount>11</pdfPageCount><abstractWordCount>65</abstractWordCount></qualityIndicators><title>Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption</title><pii><json:string>S0031-8914(38)80058-6</json:string></pii><genre><json:string>research-article</json:string></genre><host><volume>5</volume><pii><json:string>S0031-8914(38)X0049-9</json:string></pii><pages><last>187</last><first>177</first></pages><issn><json:string>0031-8914</json:string></issn><issue>3</issue><genre><json:string>Journal</json:string></genre><language><json:string>unknown</json:string></language><title>Physica</title><publicationDate>1938</publicationDate></host><categories><wos><json:string>PHYSICS</json:string></wos></categories><publicationDate>1938</publicationDate><copyrightDate>1938</copyrightDate><doi><json:string>10.1016/S0031-8914(38)80058-6</json:string></doi><id>EB88320B8CF5631A02CD2125922A1ADF7AF186D9</id><fulltext><json:item><original>true</original><mimetype>application/pdf</mimetype><extension>pdf</extension><uri>https://api.istex.fr/document/EB88320B8CF5631A02CD2125922A1ADF7AF186D9/fulltext/pdf</uri></json:item><json:item><original>true</original><mimetype>text/plain</mimetype><extension>txt</extension><uri>https://api.istex.fr/document/EB88320B8CF5631A02CD2125922A1ADF7AF186D9/fulltext/txt</uri></json:item><json:item><original>false</original><mimetype>application/zip</mimetype><extension>zip</extension><uri>https://api.istex.fr/document/EB88320B8CF5631A02CD2125922A1ADF7AF186D9/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/EB88320B8CF5631A02CD2125922A1ADF7AF186D9/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main" xml:lang="en">Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>ELSEVIER</publisher><availability><p>ELSEVIER</p></availability><date>1938</date></publicationStmt><sourceDesc><biblStruct type="inbook"><analytic><title level="a" type="main" xml:lang="en">Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption</title><author><persName><forename type="first">H.C.</forename><surname>Burger</surname></persName><affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</affiliation></author><author><persName><forename type="first">P.H.</forename><surname>van Cittert</surname></persName><affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</affiliation></author></analytic><monogr><title level="j">Physica</title><title level="j" type="abbrev">PHYSIC</title><idno type="pISSN">0031-8914</idno><idno type="PII">S0031-8914(38)X0049-9</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1938"></date><biblScope unit="volume">5</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="177">177</biblScope><biblScope unit="page" to="187">187</biblScope></imprint></monogr><idno type="istex">EB88320B8CF5631A02CD2125922A1ADF7AF186D9</idno><idno type="DOI">10.1016/S0031-8914(38)80058-6</idno><idno type="PII">S0031-8914(38)80058-6</idno><idno type="ArticleID">38800586</idno></biblStruct></sourceDesc></fileDesc><profileDesc><creation><date>1938</date></creation><langUsage><language ident="en">en</language></langUsage><abstract xml:lang="en"><p>The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines 199 and 201 coincide with the lines 198 and 200 resp.</p></abstract></profileDesc><revisionDesc><change when="1938-01-27">Received</change><change when="1938">Published</change></revisionDesc></teiHeader></istex:fulltextTEI></fulltext><metadata><istex:metadataXml wicri:clean="Elsevier doc found" wicri:toSee="Elsevier, no converted or simple article"><istex:xmlDeclaration>version="1.0" encoding="utf-8"</istex:xmlDeclaration><istex:docType PUBLIC="-//ES//DTD journal article DTD version 5.0.1//EN//XML" URI="art501.dtd" name="istex:docType"></istex:docType><istex:document><article version="5.0" xml:lang="en" docsubtype="fla"><item-info><jid>PHYSIC</jid><aid>38800586</aid><ce:pii>S0031-8914(38)80058-6</ce:pii><ce:doi>10.1016/S0031-8914(38)80058-6</ce:doi><ce:copyright type="unknown" year="1938">Martinus Nijhoff, The Hague;Holland</ce:copyright></item-info><head><ce:title>Intensity measurements in hyperfine structure of the mercury line 6<ce:sup loc="post">3</ce:sup>P<ce:inf loc="post">2</ce:inf>-7<ce:sup loc="post">3</ce:sup>S<ce:inf loc="post">1</ce:inf> (λ=5461 ÅU) in absorption</ce:title><ce:author-group><ce:author><ce:given-name>H.C.</ce:given-name><ce:surname>Burger</ce:surname></ce:author><ce:author><ce:given-name>P.H.</ce:given-name><ce:surname>van Cittert</ce:surname></ce:author><ce:affiliation id="aff1"><ce:textfn>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</ce:textfn></ce:affiliation></ce:author-group><ce:date-received day="27" month="1" year="1938"></ce:date-received><ce:abstract id="ab1" class="author" xml:lang="en"><ce:section-title>Summary</ce:section-title><ce:abstract-sec><ce:simple-para>The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines <ce:italic>199</ce:italic> and <ce:italic>201</ce:italic> coincide with the lines <ce:italic>198</ce:italic> and <ce:italic>200</ce:italic> resp.</ce:simple-para></ce:abstract-sec></ce:abstract></head><tail><ce:bibliography><ce:section-title>References</ce:section-title><ce:bibliography-sec><ce:bib-reference id="bib1"><ce:label>1)</ce:label><sb:reference><sb:contribution langtype="en"><sb:authors><sb:author><ce:given-name>H.</ce:given-name><ce:surname>Schüler</ce:surname></sb:author><sb:author><ce:given-name>J.</ce:given-name><ce:surname>Keyston</ce:surname></sb:author></sb:authors></sb:contribution><sb:host><sb:issue><sb:series><sb:title><sb:maintitle>Z. 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Physik</sb:maintitle></sb:title><sb:volume-nr>18</sb:volume-nr></sb:series><sb:date>1933</sb:date></sb:issue><sb:pages><sb:first-page>103</sb:first-page></sb:pages></sb:host></sb:reference></ce:bib-reference><ce:bib-reference id="bib10"><ce:label>10)</ce:label><sb:reference><sb:contribution langtype="en"><sb:authors><sb:author><ce:given-name>J.</ce:given-name><ce:surname>Mattauch</ce:surname></sb:author></sb:authors></sb:contribution><sb:host><sb:issue><sb:series><sb:title><sb:maintitle>Phys. Z.</sb:maintitle></sb:title><sb:volume-nr>35</sb:volume-nr></sb:series><sb:date>1934</sb:date></sb:issue><sb:pages><sb:first-page>613</sb:first-page></sb:pages></sb:host></sb:reference></ce:bib-reference></ce:bibliography-sec></ce:bibliography></tail></article></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Intensity measurements in hyperfine structure of the mercury line 63P2-73S1 (λ=5461 ÅU) in absorption</title></titleInfo><titleInfo type="alternative" lang="en" contentType="CDATA"><title>Intensity measurements in hyperfine structure of the mercury line 6</title></titleInfo><name type="personal"><namePart type="given">H.C.</namePart><namePart type="family">Burger</namePart><affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">P.H.</namePart><namePart type="family">van Cittert</namePart><affiliation>Natuurkundig Laboratorium der Rijks Universiteit te Utrecht, The Netherlands</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="research-article" displayLabel="Full-length article"></genre><originInfo><publisher>ELSEVIER</publisher><dateIssued encoding="w3cdtf">1938</dateIssued><dateCaptured encoding="w3cdtf">1938-01-27</dateCaptured><copyrightDate encoding="w3cdtf">1938</copyrightDate></originInfo><language><languageTerm type="code" authority="iso639-2b">eng</languageTerm><languageTerm type="code" authority="rfc3066">en</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType></physicalDescription><abstract lang="en">The wave-number differences and the intensities of the hyperfine structure components of the green mercury line (λ = 5461 ÅU) are measured in absorption. They are found in good accordance with Schüler's theory, if the interpretation of the structure of the central components is slightly altered. The centres of gravity of the isotope lines 199 and 201 coincide with the lines 198 and 200 resp.</abstract><relatedItem type="host"><titleInfo><title>Physica</title></titleInfo><titleInfo type="abbreviated"><title>PHYSIC</title></titleInfo><genre type="Journal">journal</genre><originInfo><dateIssued encoding="w3cdtf">193803</dateIssued></originInfo><identifier type="ISSN">0031-8914</identifier><identifier type="PII">S0031-8914(38)X0049-9</identifier><part><detail type="volume"><number>5</number><caption>vol.</caption></detail><detail type="issue"><number>3</number><caption>no.</caption></detail><extent unit="issue pages"><start>125</start><end>204</end></extent><extent unit="pages"><start>177</start><end>187</end></extent></part></relatedItem><identifier type="istex">EB88320B8CF5631A02CD2125922A1ADF7AF186D9</identifier><identifier type="DOI">10.1016/S0031-8914(38)80058-6</identifier><identifier type="PII">S0031-8914(38)80058-6</identifier><identifier type="ArticleID">38800586</identifier><accessCondition type="use and reproduction" contentType="">© 1938Martinus Nijhoff, The Hague;Holland</accessCondition><recordInfo><recordContentSource>ELSEVIER</recordContentSource><recordOrigin>Martinus Nijhoff, The Hague;Holland, ©1938</recordOrigin></recordInfo></mods></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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