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Recording and evaluation of high resolution optical meteor spectra and comparative laboratory measurements using laser ablation of solid meteorite specimens

  1. 1.
    SYSNO ASEP0484104
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleRecording and evaluation of high resolution optical meteor spectra and comparative laboratory measurements using laser ablation of solid meteorite specimens
    Author(s) Ferus, Martin (UFCH-W) ORCID, RID
    Koukal, J. (CZ)
    Lenža, Libor (UFCH-W) ORCID, RID, SAI
    Srba, J. (CZ)
    Kubelík, Petr (UFCH-W) RID, ORCID
    Laitl, V. (CZ)
    Zanozina, Ekaterina M. (UFCH-W) RID, ORCID
    Váňa, P. (CZ)
    Kaiserová, T. (CZ)
    Knížek, Antonín (UFCH-W) ORCID, RID, SAI
    Civiš, Svatopluk (UFCH-W) RID, ORCID, SAI
    Article number8024864
    Source TitleInternational Conference on Transparent Optical Networks. - Girona : IEEE Computer Society, 2017 - ISBN 978-1-5386-0859-3
    Number of pages4 s.
    Publication formOnline - E
    ActionICTON 2017. International Conference on Transparent Optical Networks /19./
    Event date02.07.2017 - 06.07.2017
    VEvent locationGirona
    CountryES - Spain
    Event typeWRD
    Languageeng - English
    CountryES - Spain
    Keywordsatomic spectra ; laser induced breakdown spectroscopy LIBS ; meteor spectra
    Subject RIVCF - Physical ; Theoretical Chemistry
    OECD categoryPhysical chemistry
    Institutional supportUFCH-W - RVO:61388955
    UT WOS000427031500139
    EID SCOPUS85031043281
    DOI10.1109/ICTON.2017.8024864
    AnnotationImportant features in meteor spectra are usually interpreted by synthetic convolution of lines extracted from databases. For such an assignment, in our study, we employed experimental technique of meteorite specimen laser ablation spectroscopy. The spectra are recorded by high resolution laboratory Echelle spectrograph and simultaneously using novel high resolution Meteor Spectral Camera for meteor observation. The data are subsequently evaluated via calibration-free method alongside with analysis of real meteor emission spectra. Additionally, spectral features related to airglow plasma are compared with the spectra of the Laser Induced Breakdown in the air. In this manner, we show that instead of theoretical spectra simulation, laboratory experiments can be applied in evaluation of the observational data.
    WorkplaceJ. Heyrovsky Institute of Physical Chemistry
    ContactMichaela Knapová, michaela.knapova@jh-inst.cas.cz, Tel.: 266 053 196
    Year of Publishing2018
    Electronic addresshttp://ieeexplore.ieee.org/document/8024864/?section=abstract
Number of the records: 1  

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