Radiants, orbits, spectra, and deceleration of selected 2011 Draconids
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00399664" target="_blank" >RIV/67985815:_____/13:00399664 - 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
Radiants, orbits, spectra, and deceleration of selected 2011 Draconids
Original language description
We present radiants and orbits of eight Draconid meteors observed from Northern Italy on October 8, 2011. The radiants agree with theoretical predictions, with a hint that some meteors may belong to the pre-1900 meteoroid trails. The spectra confirm thatDraconids have a normal chondritic composition of main elements (Mg, Fe, Na). There are, nevertheless, enormous differences in the temporal evolution of Na line emissions. The differences are correlated with the deceleration rate and can be ascribed todifferent meteoroid structures.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2013
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, Volume 1
ISBN
978-2-87355-024-4
ISSN
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e-ISSN
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Number of pages
5
Pages from-to
65-69
Publisher name
International Meteor Organization
Place of publication
Howe
Event location
La Palma, Canary Islands,
Event date
Sep 20, 2012
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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