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ICAME 2005

Proceedings of the 28th International Conference on the Applications of the Mössbauer Effect (ICAME 2005) held in Montpellier, France, 4-9 September 2005, Volume II ( Part III-V/V)

  • Conference proceedings
  • © 2007

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Table of contents (114 papers)

  1. Mössbauer investigation of Fe0.5In1.5S3

  2. Mössbauer study of Fe0.05Ni0.95Cl2

  3. Formation of Fe i −B pairs in silicon at high temperatures

  4. Identification of substitutional and interstitial Fe in 6H-SiC

  5. Mössbauer and magnetic study of Mn2+- and Cr3+-substituted spinel magnesioferrites of the composition Mg1−xMnxFe2−2xCr2xO4

  6. Critical behavior of La0.67−y (Sr, Ba, Ca)0.33+y Mn1−x Sn x O3 (x=0.0l, 0.02, y=0, 0.07) perovskites

  7. Magnetization and magnetostriction studies of TbFeCo/YFeCo multilayers

  8. Thickness dependence of the magnetic anisotropy of Fe layers separated by Al

  9. CEMS characterisation of Fe/high-κ oxide interfaces

  10. Hematite thin films: growth and characterization

  11. Mössbauer and optical investigation of Co3−x Fe x O4 thin films grown by sol-gel process

  12. Mössbauer spectroscopical investigation of the exchange biased Fe/MnF2 interface

  13. Intermixing during epitaxial growth and Mössbauer spectroscopy with probe layers

  14. Mössbauer and SEM study of Fe-Al film

  15. Light-induced spin crossover observed for a Fe(II) complex embedded in a Nation membrane

Keywords

About this book

Since January 2004, Mossbauer spectrometers [1] have been making measurements on Mars as a component of the Athena instrument suite because the technique can "yield information about early Martian environmental conditions" and can help in "identifying minerals formed in hot, watery environments that could preserve fossil evidence of Martian life" (from an early Athena web site; cf. [2]). The spectrometers are mounted on the instrument deployment armsoftwo Mars Exploration Rovers, MER-A (Spirit) and MER-B (Opportunity), where they have access to a wide range of rocks and soils. Initial measurements at the Spirit site showed that surface samples contained primarily basaltic minerals with weathering by physical processes [3], while mineralogy inferred from data acquired at the Opportunity site provided evidence for past aqueous processes [4]. More recently, Mossbauer spectroscopy has identified goethite at Columbia Hills [5] and contributed to an understanding of the nature of Martian atmospheric dust and its implications for the history of water on Mars [6]. It is important that MER-team results be verified and expanded upon. Since August 2004, Mars Mossbauer and related data, with supporting documentation, have been made available to the science community via the Planetary Data System (PDS) at the MER Analyst's Notebook download site (http://www. anserverl. eprsl. wustl. edu/) and at the PDS Geosciences Node (http://www. pds-geosciences. wustl. edu/).

Editors and Affiliations

  • Université Montpellier II — CNRS, Montpellier, France

    P.-E. Lippens, J.-C. Jumas

  • Uiversité Henri Poincaré-Nancy I, Villers-lès-Nancy, France

    J.-M. R. Génin

Bibliographic Information

  • Book Title: ICAME 2005

  • Book Subtitle: Proceedings of the 28th International Conference on the Applications of the Mössbauer Effect (ICAME 2005) held in Montpellier, France, 4-9 September 2005, Volume II ( Part III-V/V)

  • Editors: P.-E. Lippens, J.-C. Jumas, J.-M. R. Génin

  • DOI: https://doi.org/10.1007/978-3-540-49853-7

  • Publisher: Springer Berlin, Heidelberg

  • eBook Packages: Physics and Astronomy, Physics and Astronomy (R0)

  • Copyright Information: Springer-Verlag Berlin Heidelberg 2007

  • Hardcover ISBN: 978-3-540-49852-0Published: 06 March 2007

  • Softcover ISBN: 978-3-642-43344-3Published: 06 December 2014

  • eBook ISBN: 978-3-540-49853-7Published: 15 April 2010

  • Edition Number: 1

  • Number of Pages: XII, 683

  • Additional Information: Reprinted from Hyperfine Interactions, Volume 167, Nos.1-3 (2006); Volume 168, Nos. 1-3 (2006) and Volume 169, Nos.1-3 (2006)

  • Topics: Nuclear Physics, Heavy Ions, Hadrons

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