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Oxygen line in fireball spectra and implications to satellite observations of fireballs

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00604851" target="_blank" >RIV/67985815:_____/23:00604851 - isvavai.cz</a>

  • Result on the web

    <a href="https://articles.adsabs.harvard.edu/pdf/2023pimo.conf...44V" target="_blank" >https://articles.adsabs.harvard.edu/pdf/2023pimo.conf...44V</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Oxygen line in fireball spectra and implications to satellite observations of fireballs

  • Original language description

    We examined the spectral region at 777 nm, where the oxygen triplet dominates, in spectra of 43 fireballs with magnitudes from -8 to -15 obtained within the European Fireball Network. The radiant intensity was compared with the energy radiated in the broadband spectrum. It was confirmed that meteor velocity strongly affects the intensity of the oxygen triplet. In slow meteors, the excitation of atmospheric elements, including oxygen, is low and the relative brightness of atmospheric lines is lower than it is in the case of fast meteors. On the other hand, the oxygen triplet belongs to the brightest lines in the spectra of fast meteors. This behavior must be taken into account when estimating total fireball magnitude from narrow band observations at 777 nm, as is the case with the Geostationary Lightning Mapper (GLM) on board the GOES satellites. We derived an empirical relation between meteor speed, radiation at 777 nm, and the absolute visual magnitude of the meteor. We have successfully applied this relation to real GLM data and can estimate the magnitude of the fireballs observed from these weather satellites.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GX19-26232X" target="_blank" >GX19-26232X: Compositional and orbital mapping of meteoroid sources in the Solar System</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of the International Meteor Conference

  • ISBN

    978-2-87355-035-6

  • ISSN

  • e-ISSN

  • Number of pages

    3

  • Pages from-to

    38-40

  • Publisher name

    International Meteor Organization

  • Place of publication

    Mechelen

  • Event location

    Poroszlo

  • Event date

    Sep 29, 2022

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article