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Meteor Databases in Astronomy

Published online by Cambridge University Press:  30 May 2017

Svitlana V. Kolomiyets Open the ORCID record for Svitlana V. Kolomiyets [Opens in a new window]
Svitlana V. Kolomiyets*
Affiliation:
Kharkiv National University of Radio Electronics, 14 Nauki Ave, Kharkiv UA-61166, Ukraine email: [email protected]
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Abstract

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There are specific problems of databases in meteor science such as making meteor databases into the modern research tools. Special institutes and virtual observatories exist for the meteor data storage where the data is online and in open access. However, there are also numerous databases without the open access, such as for example, three radar databases: Kharkiv database with 250,000 meteor orbits in Ukraine, New Zealand database with 500,000 meteor orbits, and Canadian database with more than 3 million meteor orbits. One of the reasons the open access is absent for these databases could be the complexity in the copyright compliance. In the framework of the creation of the modern effective research tool in the meteor science, we discuss here the case of the Kharkiv meteor database.

Keywords

Meteorsdatabasesorbitsastronomyradars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S325: Astroinformatics , October 2016 , pp. 389 - 392
Copyright
Copyright © International Astronomical Union 2017 

References

Baggaley, W. J., Marsh, S. H., Bennett, R. G. T., & Galligan, D. P. 2001, ESA-SP-495, 387Google Scholar
Brown, P., Jones, J., Weryk, R. J., & Campbell-Brown, M. D. 2004, Earth Moon Planet, 95, 1, 617 Google Scholar
Fedynsky, V. V., Kashcheyev, B. L., Voloshchuk, Y. I., et al. 1976, Bull. AS USSR, 10, 89 Google Scholar
Jenniskens, P., Gural, P. S., Dynneson, L., et al. 2011, Icarus, 216, 40 Google Scholar
Jopek, T. J. & Jenniskens, P. M. 2011, NASA/CP-2011-216469, 7Google Scholar
Kanuchova, Z. & Jopek, T. J. 2016, https://www.ta3.sk/IAUC22DB/MDC2007/ Google Scholar
Kashcheyev, B. L., Lebedinets, V. N. & Lagutin, M. F. 1967, Meteor phenomena in the Earth’s atmosphere, Moscow: Science, 260Google Scholar
Kashcheyev, B. L. & Tkachuk, A. A. 1980, Materials global data center B. Results of Radar observations of faint meteors: Cataloque of meteor orbits to +12 m, Moscow, 232Google Scholar
Kolomiyets, S. V. & Voloshchuk, Yu.I. 2013, in “Meteoroids 2013”, Conf. Program & Abst., P.093Google Scholar
Kruchynenko, V. G. 2012, Mathematical and physical analysis of meteor phenomena, Kiev: Scientific Production Enterprise, Naukova Dumka, NAS of Ukraine, 294Google Scholar
Neslusan, L., Porubcan, V. & Svoren, J. 2014, Earth, Moon, and Planets, 111, 105 CrossRefGoogle Scholar
SonotaCo, 2009, WGN, Journal of the IMO, 37, 55 Google Scholar