Tackling the FeO orange band puzzle in meteor and airglow spectra through combined astronomical and laboratory studies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00548960" target="_blank" >RIV/67985815:_____/21:00548960 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/staa3487" target="_blank" >https://doi.org/10.1093/mnras/staa3487</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/staa3487" target="_blank" >10.1093/mnras/staa3487</a>
Alternative languages
Result language
angličtina
Original language name
Tackling the FeO orange band puzzle in meteor and airglow spectra through combined astronomical and laboratory studies
Original language description
The iron oxide 'orange arc' bands are unambiguously detected in persistent meteor trains, meteor wakes, and clouds, as well as in the terrestrial airglow. In contrast to the majority of other astronomically important diatomic molecules, theoretical simulation of the FeO rovibronic spectra is not feasible due to the extremely condensed and strongly perturbed multiplet structure of its excited states. In this work, the time-evolution of the laser-induced breakdown spectra (LIBS) of high-purity iron recorded in air at high temperature and impact conditions is used to mimic the FeO pseudo-continuum emission observed during meteor events and the terrestrial night airglow. The relative intensity distributions in the structural continuum of the LIBS spectra are measured at 530-660 nm and a plasma temperature of 1500-6500 K. The anomalous increase of the intensity observed at 620-640 nm and temperature < 2000 K could be attributed to the emission of higher oxides of iron as explained by the conducted thermodynamic and kinetic modelling of iron burning in the atmosphere.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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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
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
1365-2966
Volume of the periodical
500
Issue of the periodical within the volume
4
Country of publishing house
GB - UNITED KINGDOM
Number of pages
11
Pages from-to
4296-4306
UT code for WoS article
000606297700003
EID of the result in the Scopus database
2-s2.0-85099682642