Data on 824 fireballs observed by the digital cameras of the European Fireball Network in 2017-2018. I. Description of the network, data reduction procedures, and the catalog

0567448 - ASÚ 2023 RIV FR eng J - Journal Article
Borovička, Jiří - Spurný, Pavel - Shrbený, Lukáš - Štork, Rostislav - Kotková, Lenka - Fuchs, Jan - Keclíková, Jaroslava - Zichová, Hana - Mánek, Jan - Váchová, Pavlína - Macourková, Ivana - Svoreň, J. - Mucke, H.
Data on 824 fireballs observed by the digital cameras of the European Fireball Network in 2017-2018. I. Description of the network, data reduction procedures, and the catalog.
Astronomy & Astrophysics. Roč. 667, December (2022), č. článku A157. ISSN 0004-6361. E-ISSN 1432-0746
R&D Projects: GA ČR(CZ) GX19-26232X
Institutional support: RVO:67985815
Keywords : meteorites * meteors * meteoroids
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 6.5, year: 2022
Method of publishing: Open access

A catalog of 824 fireballs (bright meteors), observed by a dedicated network of all-sky digital photographic cameras in central Europe in the years 2017-2018 is presented. The status of the European Fireball Network, established in 1963, is described. The cameras collect digital images of meteors brighter than an absolute magnitude of about −2 and radiometric light curves with a high temporal resolution of those brighter than a magnitude ≈−4. All meteoroids larger than 5 g, corresponding to sizes of about 2 cm, are detected regardless of their entry velocity. High-velocity meteoroids are detected down to masses of about 0.1 g. The largest observed meteoroid in the reported period 2017-2018 had a mass of about 100 kg and a size of about 40 cm. The methods of data analysis are explained and all catalog entries are described in detail. The provided data include the fireball date and time, atmospheric trajectory and velocity, the radiant in various coordinate systems, heliocentric orbital elements, maximum brightness, radiated energy, initial and terminal masses, maximum encountered dynamic pressure, physical classification, and possible shower membership. Basic information on the fireball spectrum is available for some bright fireballs (apparent magnitude <−7). A simple statistical evaluation of the whole sample is provided. The scientific analysis is presented in an accompanying paper.
Permanent Link: https://hdl.handle.net/11104/0338705