Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite
Identifieur interne : 000284 ( Istex/Corpus ); précédent : 000283; suivant : 000285Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite
Auteurs : M. Nú Ez-Valdez ; Z. Wu ; Y. G. Yu ; R. M. WentzcovitchSource :
- Geophysical Research Letters [ 0094-8276 ] ; 2013-01-28.
Abstract
We present first‐principles results for elastic moduli (bulk, K, and shear, G) and acoustic velocities (compressional, VP, shear, VS, and bulk VΦ) of olivine (α) and wadsleyite (β) (Fex,Mg1 − x)2SiO4, at high pressure (P) and temperature (T) with varying iron content (0 ≤ x ≤ 0.125). Pressure and temperature derivatives of these properties are analyzed. We show that adding 12.5% of Fe in forsterite softens VP and VS by ∼3–6%, the same effect as raising temperature by ∼1000 K in dry olivine at 13.5 GPa—the same is true in wadsleyite. This study suggests that Fe is effective in producing seismic velocity heterogeneity at upper mantle and transition zone conditions and should be another key ingredient, in addition to temperature and water content variations, in interpreting seismic heterogeneities in the transition zone. The effect of Fe on density, elastic, and velocity contrasts across the α → β transition is also addressed at relevant conditions. We show that simultaneous changes of composition, temperature, and pressure do not affect significantly the relative density contrasts. We also find that compressional and shear impedance contrasts result primarily from velocity discontinuities rather than density discontinuity.
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DOI: 10.1002/grl.50131
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<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite</title><author><name sortKey="Nu Ez Aldez, M" sort="Nu Ez Aldez, M" uniqKey="Nu Ez Aldez M" first="M." last="Nú Ez-Valdez">M. Nú Ez-Valdez</name><affiliation><mods:affiliation>School of Physics and Astronomy, University of Minnesota, Minnesota, Minneapolis, USA</mods:affiliation></affiliation></author><author><name sortKey="Wu, Z" sort="Wu, Z" uniqKey="Wu Z" first="Z." last="Wu">Z. Wu</name><affiliation><mods:affiliation>School of Earth and Space Sciences, University of Science and Technology of China, Anhui, Hefei, China</mods:affiliation></affiliation></author><author><name sortKey="Yu, Y G" sort="Yu, Y G" uniqKey="Yu Y" first="Y. G." last="Yu">Y. G. Yu</name><affiliation><mods:affiliation>Department of Chemical Engineering and Materials Science, University of Minnesota, Minnesota, Minneapolis, USA</mods:affiliation></affiliation></author><author><name sortKey="Wentzcovitch, R M" sort="Wentzcovitch, R M" uniqKey="Wentzcovitch R" first="R. M." last="Wentzcovitch">R. M. 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Nú Ez-Valdez</name><affiliation><mods:affiliation>School of Physics and Astronomy, University of Minnesota, Minnesota, Minneapolis, USA</mods:affiliation></affiliation></author><author><name sortKey="Wu, Z" sort="Wu, Z" uniqKey="Wu Z" first="Z." last="Wu">Z. Wu</name><affiliation><mods:affiliation>School of Earth and Space Sciences, University of Science and Technology of China, Anhui, Hefei, China</mods:affiliation></affiliation></author><author><name sortKey="Yu, Y G" sort="Yu, Y G" uniqKey="Yu Y" first="Y. G." last="Yu">Y. G. Yu</name><affiliation><mods:affiliation>Department of Chemical Engineering and Materials Science, University of Minnesota, Minnesota, Minneapolis, USA</mods:affiliation></affiliation></author><author><name sortKey="Wentzcovitch, R M" sort="Wentzcovitch, R M" uniqKey="Wentzcovitch R" first="R. M." last="Wentzcovitch">R. M. Wentzcovitch</name><affiliation><mods:affiliation>Department of Chemical Engineering and Materials Science, Minnesota Supercomputing Institute (MSI), University of Minnesota, Minnesota, Minneapolis, USA</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Geophysical Research Letters</title><title level="j" type="abbrev">Geophys. Res. Lett.</title><idno type="ISSN">0094-8276</idno><idno type="eISSN">1944-8007</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><date type="published" when="2013-01-28">2013-01-28</date><biblScope unit="volume">40</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="290">290</biblScope><biblScope unit="page" to="294">294</biblScope></imprint><idno type="ISSN">0094-8276</idno></series><idno type="istex">E668F77777E876D78DFD3A0EA2EB9797EB4E24AC</idno><idno type="DOI">10.1002/grl.50131</idno><idno type="ArticleID">GRL50131</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0094-8276</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract">We present first‐principles results for elastic moduli (bulk, K, and shear, G) and acoustic velocities (compressional, VP, shear, VS, and bulk VΦ) of olivine (α) and wadsleyite (β) (Fex,Mg1 − x)2SiO4, at high pressure (P) and temperature (T) with varying iron content (0 ≤ x ≤ 0.125). Pressure and temperature derivatives of these properties are analyzed. We show that adding 12.5% of Fe in forsterite softens VP and VS by ∼3–6%, the same effect as raising temperature by ∼1000 K in dry olivine at 13.5 GPa—the same is true in wadsleyite. This study suggests that Fe is effective in producing seismic velocity heterogeneity at upper mantle and transition zone conditions and should be another key ingredient, in addition to temperature and water content variations, in interpreting seismic heterogeneities in the transition zone. The effect of Fe on density, elastic, and velocity contrasts across the α → β transition is also addressed at relevant conditions. We show that simultaneous changes of composition, temperature, and pressure do not affect significantly the relative density contrasts. We also find that compressional and shear impedance contrasts result primarily from velocity discontinuities rather than density discontinuity.</div></front></TEI><istex><corpusName>wiley</corpusName><author><json:item><name>M. Núñez‐Valdez</name><affiliations><json:string>School of Physics and Astronomy, University of Minnesota, Minnesota, Minneapolis, USA</json:string></affiliations></json:item><json:item><name>Z. Wu</name><affiliations><json:string>School of Earth and Space Sciences, University of Science and Technology of China, Anhui, Hefei, China</json:string></affiliations></json:item><json:item><name>Y. G. Yu</name><affiliations><json:string>Department of Chemical Engineering and Materials Science, University of Minnesota, Minnesota, Minneapolis, USA</json:string></affiliations></json:item><json:item><name>R. M. 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American Geophysical Union. All Rights Reserved.©2013. American Geophysical Union. All Rights Reserved.</p></availability><date>2013-01-15</date></publicationStmt><sourceDesc><biblStruct type="inbook"><analytic><title level="a" type="main" xml:lang="en">Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite</title><author xml:id="author-1"><persName><forename type="first">M.</forename><surname>Núñez‐Valdez</surname></persName><note type="correspondence"><p>Correspondence: Corresponding author: M. Núñez‐Valdez, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA. ()</p></note><affiliation>School of Physics and Astronomy, University of Minnesota, Minnesota, Minneapolis, USA</affiliation></author><author xml:id="author-2"><persName><forename type="first">Z.</forename><surname>Wu</surname></persName><affiliation>School of Earth and Space Sciences, University of Science and Technology of China, Anhui, Hefei, China</affiliation></author><author xml:id="author-3"><persName><forename type="first">Y. G.</forename><surname>Yu</surname></persName><affiliation>Department of Chemical Engineering and Materials Science, University of Minnesota, Minnesota, Minneapolis, USA</affiliation></author><author xml:id="author-4"><persName><forename type="first">R. M.</forename><surname>Wentzcovitch</surname></persName><affiliation>Department of Chemical Engineering and Materials Science, Minnesota Supercomputing Institute (MSI), University of Minnesota, Minnesota, Minneapolis, USA</affiliation></author></analytic><monogr><title level="j">Geophysical Research Letters</title><title level="j" type="abbrev">Geophys. Res. Lett.</title><idno type="pISSN">0094-8276</idno><idno type="eISSN">1944-8007</idno><idno type="DOI">10.1002/(ISSN)1944-8007</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><date type="published" when="2013-01-28"></date><biblScope unit="volume">40</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="290">290</biblScope><biblScope unit="page" to="294">294</biblScope></imprint></monogr><idno type="istex">E668F77777E876D78DFD3A0EA2EB9797EB4E24AC</idno><idno type="DOI">10.1002/grl.50131</idno><idno type="ArticleID">GRL50131</idno></biblStruct></sourceDesc></fileDesc><profileDesc><creation><date>2013-01-15</date></creation><langUsage><language ident="en">en</language></langUsage><abstract><p>We present first‐principles results for elastic moduli (bulk, K, and shear, G) and acoustic velocities (compressional, VP, shear, VS, and bulk VΦ) of olivine (α) and wadsleyite (β) (Fex,Mg1 − x)2SiO4, at high pressure (P) and temperature (T) with varying iron content (0 ≤ x ≤ 0.125). Pressure and temperature derivatives of these properties are analyzed. We show that adding 12.5% of Fe in forsterite softens VP and VS by ∼3–6%, the same effect as raising temperature by ∼1000 K in dry olivine at 13.5 GPa—the same is true in wadsleyite. This study suggests that Fe is effective in producing seismic velocity heterogeneity at upper mantle and transition zone conditions and should be another key ingredient, in addition to temperature and water content variations, in interpreting seismic heterogeneities in the transition zone. The effect of Fe on density, elastic, and velocity contrasts across the α → β transition is also addressed at relevant conditions. We show that simultaneous changes of composition, temperature, and pressure do not affect significantly the relative density contrasts. We also find that compressional and shear impedance contrasts result primarily from velocity discontinuities rather than density discontinuity.</p></abstract><abstract style="short"><p>First‐principles high temperature elasticity of Fe‐bearing olivine and wadsleyite Sound velocities at conditions of the 410 km discontinuity Contrast of elastic moduli and velocities across the alpha to beta transition</p></abstract><textClass><keywords scheme="keyword"><list><head>keywords</head><item><term>high‐temperature</term></item><item><term>thermoelasticity</term></item><item><term>olivine</term></item><item><term>wadsleyite</term></item><item><term>first‐principles</term></item><item><term>410 km discontinuity</term></item></list></keywords></textClass><textClass><keywords scheme="Journal Subject"><list><head>index-terms</head><item><term>MINERAL PHYSICS</term></item><item><term>High‐pressure behavior</term></item><item><term>Elasticity and anelasticity</term></item><item><term>Defects</term></item></list></keywords></textClass><textClass><keywords scheme="Journal Subject"><list><head>article-category</head><item><term>Regular Article</term></item></list></keywords></textClass></profileDesc><revisionDesc><change when="2012-07-03">Received</change><change when="2013-01-02">Registration</change><change when="2013-01-15">Created</change><change when="2013-01-28">Published</change></revisionDesc></teiHeader></istex:fulltextTEI><json:item><original>false</original><mimetype>text/plain</mimetype><extension>txt</extension><uri>https://api.istex.fr/document/E668F77777E876D78DFD3A0EA2EB9797EB4E24AC/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component type="serialArticle" version="2.0" xml:lang="en" xml:id="grl50131"><header><publicationMeta level="product"><doi>10.1002/(ISSN)1944-8007</doi><issn type="print">0094-8276</issn><issn type="electronic">1944-8007</issn><idGroup><id type="product" value="GRL"></id></idGroup><titleGroup><title type="main" sort="GEOPHYSICAL RESEARCH LETTERS">Geophysical Research Letters</title><title type="short">Geophys. 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All Rights Reserved.</copyright><eventGroup><event type="manuscriptReceived" date="2012-07-03"></event><event type="manuscriptRevised" date="2012-12-28"></event><event type="manuscriptAccepted" date="2013-01-02"></event><event type="xmlCreated" agent="SPi Global" date="2013-01-15"></event><event type="publishedOnlineAccepted" date="2013-01-05"></event><event type="publishedOnlineEarlyUnpaginated" date="2013-01-31"></event><event type="firstOnline" date="2013-01-31"></event><event type="publishedOnlineFinalForm" date="2013-03-03"></event><event type="xmlConverted" agent="Converter:WILEY_ML3G_TO_WILEY_ML3GV2 version:3.8.8" date="2014-01-26"></event><event type="xmlConverted" agent="Converter:WML3G_To_WML3G version:4.6.4 mode:FullText" date="2015-10-01"></event></eventGroup><numberingGroup><numbering type="pageFirst">290</numbering><numbering type="pageLast">294</numbering></numberingGroup><correspondenceTo>Corresponding author: M. Núñez‐Valdez, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA. (<email>valdez@physics.umn.edu</email>)</correspondenceTo><subjectInfo><subject href="http://psi.agu.org/taxonomy5/3900">MINERAL PHYSICS</subject><subjectInfo><subject href="http://psi.agu.org/taxonomy5/3924">High‐pressure behavior</subject><subject href="http://psi.agu.org/taxonomy5/3909">Elasticity and anelasticity</subject><subject href="http://psi.agu.org/taxonomy5/3904">Defects</subject></subjectInfo></subjectInfo><selfCitationGroup><citation type="self" xml:id="grl50131-cit-0000"><author><familyName>Núñez‐Valdez</familyName>, <givenNames>M.</givenNames></author>, <author><givenNames>Z.</givenNames><familyName>Wu</familyName></author>, <author><givenNames>Y. G.</givenNames><familyName>Yu</familyName></author>, and <author><givenNames>R. M.</givenNames><familyName>Wentzcovitch</familyName></author> (<pubYear year="2013">2013</pubYear>), <articleTitle>Thermal elasticity of (Fe<i><sub>x</sub></i>,Mg<sub>1−<i>x</i></sub>)<sub>2</sub>SiO<sub>4</sub> olivine and wadsleyite</articleTitle>, <journalTitle>Geophys. Res. Lett.</journalTitle>, <vol>40</vol>, <pageFirst>290</pageFirst>–<pageLast>294</pageLast>, doi:<accessionId ref="info:doi/10.1002/grl.50131">10.1002/grl.50131</accessionId>.</citation></selfCitationGroup><linkGroup><link type="toTypesetVersion" href="file:GRL.GRL50131.pdf"></link></linkGroup></publicationMeta><contentMeta><titleGroup><title type="main">Thermal elasticity of (Fe<i><sub>x</sub></i>,Mg<sub>1−<i>x</i></sub>)<sub>2</sub>SiO<sub>4</sub> olivine and wadsleyite</title><title type="short">THERMAL ELASTICITY OF (Fe<i><sub>x</sub></i>,Mg<sub>1−<i>x</i></sub>)<sub>2</sub>SiO<sub>4</sub> OLIVINE AND WADSLEYITE</title><title type="shortAuthors">NÚÑEZ‐VALDEZ ET AL.</title></titleGroup><creators><creator creatorRole="author" xml:id="grl50131-cr-0001" affiliationRef="#grl50131-aff-0001" corresponding="yes"><personName><givenNames>M.</givenNames><familyName>Núñez‐Valdez</familyName></personName></creator><creator creatorRole="author" xml:id="grl50131-cr-0002" affiliationRef="#grl50131-aff-0002"><personName><givenNames>Z.</givenNames><familyName>Wu</familyName></personName></creator><creator creatorRole="author" xml:id="grl50131-cr-0003" affiliationRef="#grl50131-aff-0003"><personName><givenNames>Y. G.</givenNames><familyName>Yu</familyName></personName></creator><creator creatorRole="author" xml:id="grl50131-cr-0004" affiliationRef="#grl50131-aff-0004"><personName><givenNames>R. M.</givenNames><familyName>Wentzcovitch</familyName></personName></creator></creators><affiliationGroup><affiliation countryCode="US" type="organization" xml:id="grl50131-aff-0001"><orgDiv>School of Physics and Astronomy</orgDiv><orgName>University of Minnesota</orgName><address><city>Minneapolis</city><countryPart>Minnesota</countryPart><country>USA</country></address></affiliation><affiliation countryCode="CN" type="organization" xml:id="grl50131-aff-0002"><orgDiv>School of Earth and Space Sciences</orgDiv><orgName>University of Science and Technology of China</orgName><address><city>Hefei</city><countryPart>Anhui</countryPart><country>China</country></address></affiliation><affiliation countryCode="US" type="organization" xml:id="grl50131-aff-0003"><orgDiv>Department of Chemical Engineering and Materials Science</orgDiv><orgName>University of Minnesota</orgName><address><city>Minneapolis</city><countryPart>Minnesota</countryPart><country>USA</country></address></affiliation><affiliation countryCode="US" type="organization" xml:id="grl50131-aff-0004"><orgDiv>Department of Chemical Engineering and Materials Science, Minnesota Supercomputing Institute (MSI)</orgDiv><orgName>University of Minnesota</orgName><address><city>Minneapolis</city><countryPart>Minnesota</countryPart><country>USA</country></address></affiliation></affiliationGroup><keywordGroup type="author"><keyword xml:id="grl50131-kwd-0001">high‐temperature</keyword><keyword xml:id="grl50131-kwd-0002">thermoelasticity</keyword><keyword xml:id="grl50131-kwd-0003">olivine</keyword><keyword xml:id="grl50131-kwd-0004">wadsleyite</keyword><keyword xml:id="grl50131-kwd-0005">first‐principles</keyword><keyword xml:id="grl50131-kwd-0006">410 km discontinuity</keyword></keywordGroup><abstractGroup><abstract type="main"><title type="main">Abstract</title><p label="1">We present first‐principles results for elastic moduli (bulk, <i>K</i>, and shear, <i>G</i>) and acoustic velocities (compressional, <i>V</i><sub><i>P</i></sub>, shear, <i>V</i><sub><i>S</i></sub>, and bulk <i>V</i><sub><i>Φ</i></sub>) of olivine (<i>α</i>) and wadsleyite (<i>β</i>) (Fe<sub><i>x</i></sub>,Mg<sub>1 − <i>x</i></sub>)<sub>2</sub>SiO<sub>4</sub>, at high pressure (<i>P</i>) and temperature (<i>T</i>) with varying iron content (0 ≤ <i>x</i> ≤ 0.125). Pressure and temperature derivatives of these properties are analyzed. We show that adding 12.5% of Fe in forsterite softens <i>V</i><sub><i>P</i></sub> and <i>V</i><sub><i>S</i></sub> by ∼3–6%, the same effect as raising temperature by ∼1000 K in dry olivine at 13.5 GPa—the same is true in wadsleyite. This study suggests that Fe is effective in producing seismic velocity heterogeneity at upper mantle and transition zone conditions and should be another key ingredient, in addition to temperature and water content variations, in interpreting seismic heterogeneities in the transition zone. The effect of Fe on density, elastic, and velocity contrasts across the <i>α</i> → <i>β</i> transition is also addressed at relevant conditions. We show that simultaneous changes of composition, temperature, and pressure do not affect significantly the relative density contrasts. We also find that compressional and shear impedance contrasts result primarily from velocity discontinuities rather than density discontinuity.</p></abstract><abstract type="short"><title type="main">Key Points</title><p><list style="bulleted"><listItem xml:id="grl50131-li-0001">First‐principles high temperature elasticity of Fe‐bearing olivine and wadsleyite</listItem><listItem xml:id="grl50131-li-0002">Sound velocities at conditions of the 410 km discontinuity</listItem><listItem xml:id="grl50131-li-0003">Contrast of elastic moduli and velocities across the alpha to beta transition</listItem></list></p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>THERMAL ELASTICITY OF (Fex,Mg1−x)2SiO4 OLIVINE AND WADSLEYITE</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite</title></titleInfo><name type="personal"><namePart type="given">M.</namePart><namePart type="family">Núñez‐Valdez</namePart><affiliation>School of Physics and Astronomy, University of Minnesota, Minnesota, Minneapolis, USA</affiliation><description>Correspondence: Corresponding author: M. Núñez‐Valdez, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, USA. ()</description><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Z.</namePart><namePart type="family">Wu</namePart><affiliation>School of Earth and Space Sciences, University of Science and Technology of China, Anhui, Hefei, China</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Y. G.</namePart><namePart type="family">Yu</namePart><affiliation>Department of Chemical Engineering and Materials Science, University of Minnesota, Minnesota, Minneapolis, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">R. M.</namePart><namePart type="family">Wentzcovitch</namePart><affiliation>Department of Chemical Engineering and Materials Science, Minnesota Supercomputing Institute (MSI), University of Minnesota, Minnesota, Minneapolis, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article"></genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><dateIssued encoding="w3cdtf">2013-01-28</dateIssued><dateCreated encoding="w3cdtf">2013-01-15</dateCreated><dateCaptured encoding="w3cdtf">2012-07-03</dateCaptured><dateValid encoding="w3cdtf">2013-01-02</dateValid><edition>Núñez‐Valdez, M., Z.Wu, Y. G. Yu, and R. M. Wentzcovitch (2013), Thermal elasticity of (Fex,Mg1−x)2SiO4 olivine and wadsleyite, Geophys. Res. Lett., 40, 290–294, doi:10.1002/grl.50131.</edition><copyrightDate encoding="w3cdtf">2013</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType></physicalDescription><abstract>We present first‐principles results for elastic moduli (bulk, K, and shear, G) and acoustic velocities (compressional, VP, shear, VS, and bulk VΦ) of olivine (α) and wadsleyite (β) (Fex,Mg1 − x)2SiO4, at high pressure (P) and temperature (T) with varying iron content (0 ≤ x ≤ 0.125). Pressure and temperature derivatives of these properties are analyzed. We show that adding 12.5% of Fe in forsterite softens VP and VS by ∼3–6%, the same effect as raising temperature by ∼1000 K in dry olivine at 13.5 GPa—the same is true in wadsleyite. This study suggests that Fe is effective in producing seismic velocity heterogeneity at upper mantle and transition zone conditions and should be another key ingredient, in addition to temperature and water content variations, in interpreting seismic heterogeneities in the transition zone. The effect of Fe on density, elastic, and velocity contrasts across the α → β transition is also addressed at relevant conditions. We show that simultaneous changes of composition, temperature, and pressure do not affect significantly the relative density contrasts. We also find that compressional and shear impedance contrasts result primarily from velocity discontinuities rather than density discontinuity.</abstract><abstract type="short">First‐principles high temperature elasticity of Fe‐bearing olivine and wadsleyite Sound velocities at conditions of the 410 km discontinuity Contrast of elastic moduli and velocities across the alpha to beta transition</abstract><subject><genre>keywords</genre><topic>high‐temperature</topic><topic>thermoelasticity</topic><topic>olivine</topic><topic>wadsleyite</topic><topic>first‐principles</topic><topic>410 km discontinuity</topic></subject><relatedItem type="host"><titleInfo><title>Geophysical Research Letters</title></titleInfo><titleInfo type="abbreviated"><title>Geophys. Res. Lett.</title></titleInfo><genre type="journal">journal</genre><subject><genre>index-terms</genre><topic authorityURI="http://psi.agu.org/taxonomy5/3900">MINERAL PHYSICS</topic><topic authorityURI="http://psi.agu.org/taxonomy5/3924">High‐pressure behavior</topic><topic authorityURI="http://psi.agu.org/taxonomy5/3909">Elasticity and anelasticity</topic><topic authorityURI="http://psi.agu.org/taxonomy5/3904">Defects</topic></subject><subject><genre>article-category</genre><topic>Regular Article</topic></subject><identifier type="ISSN">0094-8276</identifier><identifier type="eISSN">1944-8007</identifier><identifier type="DOI">10.1002/(ISSN)1944-8007</identifier><identifier type="PublisherID">GRL</identifier><part><date>2013</date><detail type="volume"><caption>vol.</caption><number>40</number></detail><detail type="issue"><caption>no.</caption><number>2</number></detail><extent unit="pages"><start>290</start><end>294</end><total>5</total></extent></part></relatedItem><identifier type="istex">E668F77777E876D78DFD3A0EA2EB9797EB4E24AC</identifier><identifier type="DOI">10.1002/grl.50131</identifier><identifier type="ArticleID">GRL50131</identifier><accessCondition type="use and reproduction" contentType="copyright">©2013. American Geophysical Union. All Rights Reserved.©2013. American Geophysical Union. All Rights Reserved.</accessCondition><recordInfo><recordContentSource>WILEY</recordContentSource></recordInfo></mods></metadata><enrichments><json:item><type>multicat</type><uri>https://api.istex.fr/document/E668F77777E876D78DFD3A0EA2EB9797EB4E24AC/enrichments/multicat</uri></json:item></enrichments><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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