Calibration-free quantitative elemental analysis of meteor plasma using reference laser-induced breakdown spectroscopy of meteorite samples
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00501384" target="_blank" >RIV/68378271:_____/18:00501384 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/61388955:_____/17:00484218 RIV/00098639:_____/18:N0000001 RIV/00216208:11310/18:10387063
Výsledek na webu
<a href="http://dx.doi.org/10.1051/0004-6361/201629950" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201629950</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201629950" target="_blank" >10.1051/0004-6361/201629950</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Calibration-free quantitative elemental analysis of meteor plasma using reference laser-induced breakdown spectroscopy of meteorite samples
Popis výsledku v původním jazyce
We aim to analyse real-time Perseid and Leonid meteor spectra using a novel calibration-free (CF) method, which is usually applied in the laboratory for laser-induced breakdown spectroscopic (LIBS) chemical analysis. Reference laser ablation spectra of specimens of chondritic meteorites were measured in situ simultaneously with a highresolution laboratory echelle spectrograph and a spectral camera for meteor observation. Laboratory data were subsequently evaluated via the CF method and compared with real meteor emission spectra. Additionally, spectral features related to airglow plasma were compared with the spectra of laser-induced breakdown and electric discharge in the air. We show that this method can be applied in the evaluation of meteor spectral data observed in real time. CF analysis can be used to determine the chemical composition of meteor plasma, which, in the case of the Perseid and Leonid meteors analysed in this study, corresponds to that of the C-group of chondrites.n
Název v anglickém jazyce
Calibration-free quantitative elemental analysis of meteor plasma using reference laser-induced breakdown spectroscopy of meteorite samples
Popis výsledku anglicky
We aim to analyse real-time Perseid and Leonid meteor spectra using a novel calibration-free (CF) method, which is usually applied in the laboratory for laser-induced breakdown spectroscopic (LIBS) chemical analysis. Reference laser ablation spectra of specimens of chondritic meteorites were measured in situ simultaneously with a highresolution laboratory echelle spectrograph and a spectral camera for meteor observation. Laboratory data were subsequently evaluated via the CF method and compared with real meteor emission spectra. Additionally, spectral features related to airglow plasma were compared with the spectra of laser-induced breakdown and electric discharge in the air. We show that this method can be applied in the evaluation of meteor spectral data observed in real time. CF analysis can be used to determine the chemical composition of meteor plasma, which, in the case of the Perseid and Leonid meteors analysed in this study, corresponds to that of the C-group of chondrites.n
Klasifikace
Druh
J<sub>SC</sub> - Článek v periodiku v databázi SCOPUS
CEP obor
—
OECD FORD obor
10306 - Optics (including laser optics and quantum optics)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2018
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy & Astrophysics
ISSN
1432-0746
e-ISSN
—
Svazek periodika
610
Číslo periodika v rámci svazku
Mar
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
12
Strana od-do
1-12
Kód UT WoS článku
000427142500005
EID výsledku v databázi Scopus
2-s2.0-85043258749