The trajectory, structure and origin of the Chelyabinsk impactor

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00521161" target="_blank" >RIV/67985815:_____/19:00521161 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/2053-2563/aae894ch2" target="_blank" >http://dx.doi.org/10.1088/2053-2563/aae894ch2</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/2053-2563/aae894ch2" target="_blank" >10.1088/2053-2563/aae894ch2</a>

Result language
angličtina
Original language name
The trajectory, structure and origin of the Chelyabinsk impactor
Original language description
This chapter presents the elaboration of data collected from the observation of the Chelyabinsk meteor of February 15, 2013. The recovered meteorites are not unusual, but the bolide brightness and the strength of the blast wave indicated that Chelyabinsk witnessed the largest impact of a cosmic body since the Tunguska event in 1908. Fortunately for science, this time the event was well documented. Additional information comes from the distribution and properties of the meteorites and from the effects of the blast wave.
Czech name
—
Czech description
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Project
<a href="/en/project/GA16-00761S" target="_blank" >GA16-00761S: Fragmentation of meteoroids and small asteroids in terrestrial atmosphere</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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