Synchrotron X-ray imaging of inclusions in amber
Identifieur interne : 001554 ( PascalFrancis/Corpus ); précédent : 001553; suivant : 001555Synchrotron X-ray imaging of inclusions in amber
Auteurs : Carmen Soriano ; Mike Archer ; Dany Azar ; Phil Creaser ; Xavier Delclos ; Henk Godthelp ; Suzanne Hand ; Allan Jones ; André Nel ; Didier Neraudeau ; Jaime Ortega-Blanco ; Ricardo Perez-De La Fuente ; Vincent Perrichot ; Erin Saupe ; M Nica Solorzano Kraemer ; Paul TafforeauSource :
- Comptes rendus. Palévol [ 1631-0683 ] ; 2010.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
Over the past six years, organic inclusions preserved in amber samples from outcrops worldwide have been discovered and imaged in 3D using propagation phase contrast based X-ray synchrotron imaging techniques at the European Synchrotron Radiation Facility (ESRF). A brief description of the techniques and protocols used for detecting and 3D non-destructive imaging of amber inclusions is provided. The latest results from the major amber projects in the ESRF are given, illustrating the increasing utility of the imaging capabilities of X-ray synchrotron phase contrast microtomography.
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Pour connaître la documentation sur le format Inist Standard.
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Format Inist (serveur)
NO : | PASCAL 12-0119362 INIST |
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ET : | Synchrotron X-ray imaging of inclusions in amber |
AU : | SORIANO (Carmen); ARCHER (Mike); AZAR (Dany); CREASER (Phil); DELCLOS (Xavier); GODTHELP (Henk); HAND (Suzanne); JONES (Allan); NEL (André); NERAUDEAU (Didier); ORTEGA-BLANCO (Jaime); PEREZ-DE LA FUENTE (Ricardo); PERRICHOT (Vincent); SAUPE (Erin); SOLORZANO KRAEMER (Mónica); TAFFOREAU (Paul); CLEMENT (Gaël); GEFFARD-KURIYAMA (Didier) |
AF : | European Synchrotron Radiation Facility - X-Ray Imaging Group, 6, rue Jules-Horowitz/38000 Grenoble/France (1 aut., 16 aut.); CNRS UMR 6118, géosciences & observatoire des sciences de l'université de Rennes, université Rennes 1, campus de Beaulieu/35042 Rennes/France (1 aut., 10 aut., 13 aut.); School of Biological, Earth and Environmental Sciences, University of New South Wales/Sydney 2052/Australie (2 aut., 4 aut., 6 aut., 7 aut.); Lebanese University, P.O. Box 26110217/Fanar-Matn/Liban (3 aut.); CNRS UMR 7205, Muséum national d'histoire naturelle/75231 Paris/France (3 aut., 9 aut.); Facultat de Geologia, Universitat de Barcelona/Barcelona 08024/Espagne (5 aut., 11 aut., 12 aut.); Australian Key Centre for Microscopy & Microanalysis, University of Sydney/Sydney 2006/Australie (8 aut.); University of Kansas/Lawrence-Kansas 66045/Etats-Unis (14 aut.); Steinmann Institut für Geologie, Mineralogie und Paläontologie/Bonn 53115/Allemagne (15 aut.); Senckenberg Forschungsinstitut und Naturmuseum/Frankfurt am Main 60325/Allemagne (15 aut.); UMR-CNRS 7207 CR2P, USM 203, département histoire de la Terre, Muséum d'histoire naturelle, 57, rue Cuvier, CP 38/75005 Paris/France (1 aut., 2 aut.) |
DT : | Publication en série; Niveau analytique |
SO : | Comptes rendus. Palévol; ISSN 1631-0683; France; Da. 2010; Vol. 9; No. 6-7; Pp. 361-368; Abs. français; Bibl. 1/2 p. |
LA : | Anglais |
EA : | Over the past six years, organic inclusions preserved in amber samples from outcrops worldwide have been discovered and imaged in 3D using propagation phase contrast based X-ray synchrotron imaging techniques at the European Synchrotron Radiation Facility (ESRF). A brief description of the techniques and protocols used for detecting and 3D non-destructive imaging of amber inclusions is provided. The latest results from the major amber projects in the ESRF are given, illustrating the increasing utility of the imaging capabilities of X-ray synchrotron phase contrast microtomography. |
CC : | 001E01Q03; 227A03 |
FD : | Synchrotron; Rayon X; Inclusion; Ambre; Affleurement; Propagation; Rayonnement synchrotron; Projet |
ED : | synchrotrons; X-rays; inclusions; amber; outcrops; propagation; synchrotron radiation; projects |
SD : | Rayos X; Inclusión; Ambar; Afloramiento; Propagación; Proyecto |
LO : | INIST-116H.354000194001010100 |
ID : | 12-0119362 |
Links to Exploration step
Pascal:12-0119362Le document en format XML
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<term>synchrotron radiation</term>
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<front><div type="abstract" xml:lang="en">Over the past six years, organic inclusions preserved in amber samples from outcrops worldwide have been discovered and imaged in 3D using propagation phase contrast based X-ray synchrotron imaging techniques at the European Synchrotron Radiation Facility (ESRF). A brief description of the techniques and protocols used for detecting and 3D non-destructive imaging of amber inclusions is provided. The latest results from the major amber projects in the ESRF are given, illustrating the increasing utility of the imaging capabilities of X-ray synchrotron phase contrast microtomography.</div>
</front>
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<fA03 i2="1"><s0>C. r., Palévol</s0>
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<fA05><s2>9</s2>
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<fA06><s2>6-7</s2>
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<fA08 i1="01" i2="1" l="ENG"><s1>Synchrotron X-ray imaging of inclusions in amber</s1>
</fA08>
<fA09 i1="01" i2="1" l="ENG"><s1>Imaging & 3D in palaeontology and palaeoanthropology</s1>
</fA09>
<fA11 i1="01" i2="1"><s1>SORIANO (Carmen)</s1>
</fA11>
<fA11 i1="02" i2="1"><s1>ARCHER (Mike)</s1>
</fA11>
<fA11 i1="03" i2="1"><s1>AZAR (Dany)</s1>
</fA11>
<fA11 i1="04" i2="1"><s1>CREASER (Phil)</s1>
</fA11>
<fA11 i1="05" i2="1"><s1>DELCLOS (Xavier)</s1>
</fA11>
<fA11 i1="06" i2="1"><s1>GODTHELP (Henk)</s1>
</fA11>
<fA11 i1="07" i2="1"><s1>HAND (Suzanne)</s1>
</fA11>
<fA11 i1="08" i2="1"><s1>JONES (Allan)</s1>
</fA11>
<fA11 i1="09" i2="1"><s1>NEL (André)</s1>
</fA11>
<fA11 i1="10" i2="1"><s1>NERAUDEAU (Didier)</s1>
</fA11>
<fA11 i1="11" i2="1"><s1>ORTEGA-BLANCO (Jaime)</s1>
</fA11>
<fA11 i1="12" i2="1"><s1>PEREZ-DE LA FUENTE (Ricardo)</s1>
</fA11>
<fA11 i1="13" i2="1"><s1>PERRICHOT (Vincent)</s1>
</fA11>
<fA11 i1="14" i2="1"><s1>SAUPE (Erin)</s1>
</fA11>
<fA11 i1="15" i2="1"><s1>SOLORZANO KRAEMER (Mónica)</s1>
</fA11>
<fA11 i1="16" i2="1"><s1>TAFFOREAU (Paul)</s1>
</fA11>
<fA12 i1="01" i2="1"><s1>CLEMENT (Gaël)</s1>
<s9>ed.</s9>
</fA12>
<fA12 i1="02" i2="1"><s1>GEFFARD-KURIYAMA (Didier)</s1>
<s9>ed.</s9>
</fA12>
<fA14 i1="01"><s1>European Synchrotron Radiation Facility - X-Ray Imaging Group, 6, rue Jules-Horowitz</s1>
<s2>38000 Grenoble</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>16 aut.</sZ>
</fA14>
<fA14 i1="02"><s1>CNRS UMR 6118, géosciences & observatoire des sciences de l'université de Rennes, université Rennes 1, campus de Beaulieu</s1>
<s2>35042 Rennes</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>13 aut.</sZ>
</fA14>
<fA14 i1="03"><s1>School of Biological, Earth and Environmental Sciences, University of New South Wales</s1>
<s2>Sydney 2052</s2>
<s3>AUS</s3>
<sZ>2 aut.</sZ>
<sZ>4 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
</fA14>
<fA14 i1="04"><s1>Lebanese University, P.O. Box 26110217</s1>
<s2>Fanar-Matn</s2>
<s3>LBN</s3>
<sZ>3 aut.</sZ>
</fA14>
<fA14 i1="05"><s1>CNRS UMR 7205, Muséum national d'histoire naturelle</s1>
<s2>75231 Paris</s2>
<s3>FRA</s3>
<sZ>3 aut.</sZ>
<sZ>9 aut.</sZ>
</fA14>
<fA14 i1="06"><s1>Facultat de Geologia, Universitat de Barcelona</s1>
<s2>Barcelona 08024</s2>
<s3>ESP</s3>
<sZ>5 aut.</sZ>
<sZ>11 aut.</sZ>
<sZ>12 aut.</sZ>
</fA14>
<fA14 i1="07"><s1>Australian Key Centre for Microscopy & Microanalysis, University of Sydney</s1>
<s2>Sydney 2006</s2>
<s3>AUS</s3>
<sZ>8 aut.</sZ>
</fA14>
<fA14 i1="08"><s1>University of Kansas</s1>
<s2>Lawrence-Kansas 66045</s2>
<s3>USA</s3>
<sZ>14 aut.</sZ>
</fA14>
<fA14 i1="09"><s1>Steinmann Institut für Geologie, Mineralogie und Paläontologie</s1>
<s2>Bonn 53115</s2>
<s3>DEU</s3>
<sZ>15 aut.</sZ>
</fA14>
<fA14 i1="10"><s1>Senckenberg Forschungsinstitut und Naturmuseum</s1>
<s2>Frankfurt am Main 60325</s2>
<s3>DEU</s3>
<sZ>15 aut.</sZ>
</fA14>
<fA15 i1="01"><s1>UMR-CNRS 7207 CR2P, USM 203, département histoire de la Terre, Muséum d'histoire naturelle, 57, rue Cuvier, CP 38</s1>
<s2>75005 Paris</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
</fA15>
<fA20><s1>361-368</s1>
</fA20>
<fA21><s1>2010</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA24 i1="01"><s0>fre</s0>
</fA24>
<fA43 i1="01"><s1>INIST</s1>
<s2>116H</s2>
<s5>354000194001010100</s5>
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<fA44><s0>0000</s0>
<s1>© 2012 INIST-CNRS. All rights reserved.</s1>
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<fA45><s0>1/2 p.</s0>
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<fA47 i1="01" i2="1"><s0>12-0119362</s0>
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<fA60><s1>P</s1>
</fA60>
<fA61><s0>A</s0>
</fA61>
<fA64 i1="01" i2="1"><s0>Comptes rendus. Palévol</s0>
</fA64>
<fA66 i1="01"><s0>FRA</s0>
</fA66>
<fC01 i1="01" l="ENG"><s0>Over the past six years, organic inclusions preserved in amber samples from outcrops worldwide have been discovered and imaged in 3D using propagation phase contrast based X-ray synchrotron imaging techniques at the European Synchrotron Radiation Facility (ESRF). A brief description of the techniques and protocols used for detecting and 3D non-destructive imaging of amber inclusions is provided. The latest results from the major amber projects in the ESRF are given, illustrating the increasing utility of the imaging capabilities of X-ray synchrotron phase contrast microtomography.</s0>
</fC01>
<fC02 i1="01" i2="2"><s0>001E01Q03</s0>
</fC02>
<fC02 i1="02" i2="2"><s0>227A03</s0>
</fC02>
<fC03 i1="01" i2="2" l="FRE"><s0>Synchrotron</s0>
<s5>01</s5>
</fC03>
<fC03 i1="01" i2="2" l="ENG"><s0>synchrotrons</s0>
<s5>01</s5>
</fC03>
<fC03 i1="02" i2="2" l="FRE"><s0>Rayon X</s0>
<s5>02</s5>
</fC03>
<fC03 i1="02" i2="2" l="ENG"><s0>X-rays</s0>
<s5>02</s5>
</fC03>
<fC03 i1="02" i2="2" l="SPA"><s0>Rayos X</s0>
<s5>02</s5>
</fC03>
<fC03 i1="03" i2="2" l="FRE"><s0>Inclusion</s0>
<s5>03</s5>
</fC03>
<fC03 i1="03" i2="2" l="ENG"><s0>inclusions</s0>
<s5>03</s5>
</fC03>
<fC03 i1="03" i2="2" l="SPA"><s0>Inclusión</s0>
<s5>03</s5>
</fC03>
<fC03 i1="04" i2="2" l="FRE"><s0>Ambre</s0>
<s5>04</s5>
</fC03>
<fC03 i1="04" i2="2" l="ENG"><s0>amber</s0>
<s5>04</s5>
</fC03>
<fC03 i1="04" i2="2" l="SPA"><s0>Ambar</s0>
<s5>04</s5>
</fC03>
<fC03 i1="05" i2="2" l="FRE"><s0>Affleurement</s0>
<s5>05</s5>
</fC03>
<fC03 i1="05" i2="2" l="ENG"><s0>outcrops</s0>
<s5>05</s5>
</fC03>
<fC03 i1="05" i2="2" l="SPA"><s0>Afloramiento</s0>
<s5>05</s5>
</fC03>
<fC03 i1="06" i2="2" l="FRE"><s0>Propagation</s0>
<s5>06</s5>
</fC03>
<fC03 i1="06" i2="2" l="ENG"><s0>propagation</s0>
<s5>06</s5>
</fC03>
<fC03 i1="06" i2="2" l="SPA"><s0>Propagación</s0>
<s5>06</s5>
</fC03>
<fC03 i1="07" i2="2" l="FRE"><s0>Rayonnement synchrotron</s0>
<s5>07</s5>
</fC03>
<fC03 i1="07" i2="2" l="ENG"><s0>synchrotron radiation</s0>
<s5>07</s5>
</fC03>
<fC03 i1="08" i2="2" l="FRE"><s0>Projet</s0>
<s5>08</s5>
</fC03>
<fC03 i1="08" i2="2" l="ENG"><s0>projects</s0>
<s5>08</s5>
</fC03>
<fC03 i1="08" i2="2" l="SPA"><s0>Proyecto</s0>
<s5>08</s5>
</fC03>
<fN21><s1>093</s1>
</fN21>
<fN44 i1="01"><s1>PSI</s1>
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<fN82><s1>PSI</s1>
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<server><NO>PASCAL 12-0119362 INIST</NO>
<ET>Synchrotron X-ray imaging of inclusions in amber</ET>
<AU>SORIANO (Carmen); ARCHER (Mike); AZAR (Dany); CREASER (Phil); DELCLOS (Xavier); GODTHELP (Henk); HAND (Suzanne); JONES (Allan); NEL (André); NERAUDEAU (Didier); ORTEGA-BLANCO (Jaime); PEREZ-DE LA FUENTE (Ricardo); PERRICHOT (Vincent); SAUPE (Erin); SOLORZANO KRAEMER (Mónica); TAFFOREAU (Paul); CLEMENT (Gaël); GEFFARD-KURIYAMA (Didier)</AU>
<AF>European Synchrotron Radiation Facility - X-Ray Imaging Group, 6, rue Jules-Horowitz/38000 Grenoble/France (1 aut., 16 aut.); CNRS UMR 6118, géosciences & observatoire des sciences de l'université de Rennes, université Rennes 1, campus de Beaulieu/35042 Rennes/France (1 aut., 10 aut., 13 aut.); School of Biological, Earth and Environmental Sciences, University of New South Wales/Sydney 2052/Australie (2 aut., 4 aut., 6 aut., 7 aut.); Lebanese University, P.O. Box 26110217/Fanar-Matn/Liban (3 aut.); CNRS UMR 7205, Muséum national d'histoire naturelle/75231 Paris/France (3 aut., 9 aut.); Facultat de Geologia, Universitat de Barcelona/Barcelona 08024/Espagne (5 aut., 11 aut., 12 aut.); Australian Key Centre for Microscopy & Microanalysis, University of Sydney/Sydney 2006/Australie (8 aut.); University of Kansas/Lawrence-Kansas 66045/Etats-Unis (14 aut.); Steinmann Institut für Geologie, Mineralogie und Paläontologie/Bonn 53115/Allemagne (15 aut.); Senckenberg Forschungsinstitut und Naturmuseum/Frankfurt am Main 60325/Allemagne (15 aut.); UMR-CNRS 7207 CR2P, USM 203, département histoire de la Terre, Muséum d'histoire naturelle, 57, rue Cuvier, CP 38/75005 Paris/France (1 aut., 2 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>Comptes rendus. Palévol; ISSN 1631-0683; France; Da. 2010; Vol. 9; No. 6-7; Pp. 361-368; Abs. français; Bibl. 1/2 p.</SO>
<LA>Anglais</LA>
<EA>Over the past six years, organic inclusions preserved in amber samples from outcrops worldwide have been discovered and imaged in 3D using propagation phase contrast based X-ray synchrotron imaging techniques at the European Synchrotron Radiation Facility (ESRF). A brief description of the techniques and protocols used for detecting and 3D non-destructive imaging of amber inclusions is provided. The latest results from the major amber projects in the ESRF are given, illustrating the increasing utility of the imaging capabilities of X-ray synchrotron phase contrast microtomography.</EA>
<CC>001E01Q03; 227A03</CC>
<FD>Synchrotron; Rayon X; Inclusion; Ambre; Affleurement; Propagation; Rayonnement synchrotron; Projet</FD>
<ED>synchrotrons; X-rays; inclusions; amber; outcrops; propagation; synchrotron radiation; projects</ED>
<SD>Rayos X; Inclusión; Ambar; Afloramiento; Propagación; Proyecto</SD>
<LO>INIST-116H.354000194001010100</LO>
<ID>12-0119362</ID>
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