Chemical abundances determined from meteor spetra. I. Rations of the main chemical clements.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030088" target="_blank" >RIV/67985815:_____/03:01030088 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Chemical abundances determined from meteor spetra. I. Rations of the main chemical clements.
Original language description
Relative chemical abundances of 13 meteoroids were determined by averaging the composition of the radiating gas along the fireball path that originated during their penetration into the Earth's atmosphere.The chemical composition of all meteoroids studied in this work differs from that of 1P/Halley dust.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Meteoritics and Planetary Science
ISSN
0026-1114
e-ISSN
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Volume of the periodical
38
Issue of the periodical within the volume
8
Country of publishing house
US - UNITED STATES
Number of pages
12
Pages from-to
1283-1294
UT code for WoS article
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EID of the result in the Scopus database
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