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Stark profiles in plasmas interacting with a strong oscillatory quasi-monochromatic electric field

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    SYSNO ASEP0364217
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleStark profiles in plasmas interacting with a strong oscillatory quasi-monochromatic electric field
    Author(s) Sauvan, P. (ES)
    Dalimier, E. (FR)
    Oks, E. (US)
    Renner, Oldřich (FZU-D) RID, ORCID
    Weber, S. (FR)
    Riconda, C. (FR)
    Source Title20th International Conference on Spectral Line Shapes. - Melville : American Institute of Physics, 2010 / Lewis J. ; Predoi-Cross A. - ISBN 978-0-7354-0845-6
    Pagess. 68-78
    Number of pages11 s.
    ActionInternational Conference on Spectral Line Shapes /20./
    Event date06.06.2010-11.06.2010
    VEvent locationSt. John's
    CountryCA - Canada
    Event typeWRD
    Languageeng - English
    CountryUS - United States
    Keywordsstrong oscillating electric field ; laser produced plasma ; Floquet theory
    Subject RIVBH - Optics, Masers, Lasers
    R&D ProjectsGAP205/10/0814 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10100523 - FZU-D (2005-2011)
    UT WOS000286908200011
    AnnotationAdvanced analysis of spectroscopic signatures of strong oscillating Quasi-monochromatic Electric Fields (QEF) interacting with a preformed laser-produced plasma is presented. The Stark line shape in the presence of a QEF is calculated, the QEF intensity profile throughout the plasma is estimmated. The Stark profiles are calculated using the Floquet-Liouville formalism. The Liouville space and the Floquet theory have been joined together to solve the time-dependent Liouville equation. A second kind of simulations involving PIC kinetic simulations is required for the calculation of the QEF and the exotic features exhibited in the spectroscopic diagnostic. The final spectroscopic analysis of the experimental Al He beta line is performed. The spectroscopic signatures of the QEF show up as prominent satellites, non symmetrical with respect to the unperturbed line and distinguishable from the di-electronic satellites.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2012
Number of the records: 1  

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