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Application of a dielectric breakdown induced by high-power lasers for a laboratory simulation of meteor plasma. Experimental Astronomy

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00098639%3A_____%2F21%3AN0000002" target="_blank" >RIV/00098639:_____/21:N0000002 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.researchgate.net/publication/348947998_Application_of_a_dielectric_breakdown_induced_by_high-power_lasers_for_a_laboratory_simulation_of_meteor_plasma" target="_blank" >https://www.researchgate.net/publication/348947998_Application_of_a_dielectric_breakdown_induced_by_high-power_lasers_for_a_laboratory_simulation_of_meteor_plasma</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s10686-020-09688-3" target="_blank" >10.1007/s10686-020-09688-3</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Application of a dielectric breakdown induced by high-power lasers for a laboratory simulation of meteor plasma. Experimental Astronomy

  • Original language description

    Spectra of meteor plasma, their dynamics and dominant spectral features are usually a subject of mathematical modelling and computations. In our study, on the other hand, we describe and evaluate the advantages and limitations of the experimental techniques employed for meteor spectra simulations. The experiments are performed by ablating meteorite samples using a series of laser sources, i.e. a large terawatt−class gas laser infrastructure PALS, a high-power Ti:Sapphire femtosecond laser, and laboratory Nd:YAG and ArF excimer lasers. We demonstrate that, notwithstanding the importance of theoretical spectra computation, laboratory experiments may remarkably enhance the qualitative and quantitative evaluation of the meteor emission spectra measured, as well as the assignment of important spectral features therein. We also perform completing experiments to compare the laser-target interaction observed with the expected dynamics of evaporation and disintegration of a real meteoroid body.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>ost</sub> - Miscellaneous article in a specialist periodical

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    V - Vyzkumna aktivita podporovana z jinych verejnych zdroju

Others

  • Publication year

    2021

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Experimental Astronomy

  • ISSN

    1572-9508

  • e-ISSN

    1572-9508

  • Volume of the periodical

    2021

  • Issue of the periodical within the volume

    51.2

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    27

  • Pages from-to

    425-451

  • UT code for WoS article

  • EID of the result in the Scopus database