Abstract
This chapter considers the Chelyabinsk superbolide as a meteorological phenomenon, which caused a significant heating of air along the trajectory of the falling asteroid and the ejection of thousands of tons of dust into the atmosphere.
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References
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Gorkavyi, N.N. and Taidakova, T.A., “Interaction of the Chelyabinsk bolide with the atmosphere”, Chelyabinsk State University Bulletin, 2014, No. 1 (330), Physics, Issue 19, pp. 26–29.
Popova, O.P., et al. “Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery and Characterization”, Science, 2013, Vol. 342, No. 6162, pp. 1069–73.
Kring, D., et al., “Chelyabinsk: Portrait of an asteroid airburst”, Physics Today, 2014, Vol. 67, No. 9, pp. 32–37.
Gorkavyi, N.N., et al., “Color variations of the aerosol trace of the Chelyabinsk bolide” in The Chelyabinsk meteorite – one year on Earth. Astronomy, physics, geochemistry, mineralogy, petrography: proceedings of the all-Russian scientific conference, ed. Antipin, N.А., Chelyabinsk, 2014, pp. 118–123.
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Gorkavyi, N.N., Taidakova, T.A. (2019). Meteorology of the superbolide or super-experiment in the atmosphere. In: Gorkavyi, N., Dudorov, A., Taskaev, S. (eds) Chelyabinsk Superbolide. Springer Praxis Books(). Springer, Cham. https://doi.org/10.1007/978-3-030-22986-3_10
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DOI: https://doi.org/10.1007/978-3-030-22986-3_10
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