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Main spectral features of meteors studied using a terawatt-class high-power laser

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21340%2F19%3A00347614" target="_blank" >RIV/68407700:21340/19:00347614 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/19:00517287 RIV/61388955:_____/19:00517287 RIV/61389021:_____/19:00517287 RIV/00216208:11310/19:10409813

  • Result on the web

    <a href="https://doi.org/10.1051/0004-6361/201935816" target="_blank" >https://doi.org/10.1051/0004-6361/201935816</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201935816" target="_blank" >10.1051/0004-6361/201935816</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Main spectral features of meteors studied using a terawatt-class high-power laser

  • Original language description

    Context. Meteor spectra are commonly interpreted using data from databases and tables. Several studies have demonstrated very sophisticated calculations of elemental compositions of meteoroid bodies based on the computation of synthetic meteor spectra or on the spectral analysis of airglow plasma containing evaporated, atomized, and ionized meteoroid matter. However, considering accuracy, reliability of computations, lack of laboratory experimental data in this field, as well as the complicated physical structure of meteor plasma, such qualitative assignment or quantitative calculations are still extensively discussed in the scientific community. Even on the laboratory level, many studies have shown the high complexity of the acquisition and interpretation of the data that are recorded with techniques of emission spectroscopy that are in fashion and philosophy similar to the spectral analysis of meteor plasma, that is, detection and quantification of the elements that are ablated from complicated multicomponent matrices.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/EF16_019%2F0000778" target="_blank" >EF16_019/0000778: Center for advanced applied science</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    630

  • Issue of the periodical within the volume

    A127

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    20

  • Pages from-to

  • UT code for WoS article

    000516616800001

  • EID of the result in the Scopus database

    2-s2.0-85073202712