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Astrophysics and Space Science Proceedings, 2016, Volume 46, Pages 153–183
DOI: https://doi.org/10.1007/978-3-319-46179-3_8 (Mi assp1) 		 
This article is cited in 11 scientific papers (total in 11 papers)

Constraining the Pre-atmospheric Parameters of Large Meteoroids: Košice, a Case Study

Maria Gritsevichabcde, Vasily Dmitrieve, Vladimir Vinnikovd, Daria Kuznetsovaf, Valery Lupovkae, Jouni Peltoniemiba, Sanna Mönköläg, Jeffrey Browerh, Yuri Pupyrevi

a Department of Physics, University of Helsinki, Helsinki, Finland
b Finnish Geospatial Research Institute, Masala, Finland
c Institute of Physics and Technology, Ural Federal University, Ekaterinburg, Russia
d Department of Computational Physics, Dorodnicyn Computing Centre, Russian Academy of Sciences, Moscow, Russia
e Extraterrestrial Laboratory, State University of Geodesy and Cartography (MIIGAiK), Moscow, Russia
f Observatoire de Midi-Pyrénées, Laboratoire d'Aérologie, Université Paul Sabatier, Toulouse, France
g Department of Mathematical Information Technology, University of Jyvaskyla, Jyvaskyla, Finland
h The Royal Astronomical Society of Canada, Etobicoke, Canada
i Steklov Mathematical Institute, Russian Academy of Science, Moscow, Russia
Citations (11)
DOI: https://doi.org/10.1007/978-3-319-46179-3_8
Funding agency Grant number
Academy of Finland 260027
European Research Council 320773
Russian Foundation for Basic Research 14-08-00204
16-05-00004
16-07-01072
Magnus Ehrnrooth Foundation travel grant
Act 211 of the Government of the Russian Federation 02.A03.21.0006
Russian Science Foundation 14-22-00197
COST Action TD1403 "Big Data Era in Sky and Earth Observation"
This study was supported, in part, by the Academy of Finland project No 260027, by the ERC Advanced Grant No 320773, by the Russian Foundation for Basic Research (project Nos 14-08-00204, 16-05-00004 and 16-07-01072), by the Magnus Ehrnrooth Foundation travel grant, and by the Act 211 of the Government of the Russian Federation (agreement No 02.A03.21.0006). The part of the trajectory reconstruction and the orbit computations were done by Maria Gritsevich, Vasily Dmitriev, Daria Kuznetsova, and Valery Lupovka at MIIGAiK under the support of the Russian Science Foundation, project No 14-22-00197 "Studies of Fundamental Geodetic Parameters and Topography of Planets and Satellites". The authors acknowledge being a part of the network supported by the COST Action TD1403 “Big Data Era in Sky and Earth Observation”.
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Document Type: Article
Language: English
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