Meteoritics & Planetary Science 38, 989--1003 (2003)

The Moravka meteorite fall:

2. Interpretation of infrasonic and seismic data

P. G. Brown¹, P. Kalenda², D. O. ReVelle³, and J. Borovicka⁴

¹Department of Physics and Astronomy, University of Western Ontario, London, Ontario N6A 3K7, Canada
²CoalExp, Kosmonautu 2, 70030 Ostrava 3, The Czech Republic
³Los Alamos National Laboratory, P.O. Box 1663, MS J557, Los Alamos, New Mexico 87545, USA
⁴Astronomical Institute of the Academy of Sciences, 25165 Ondrejov, The Czech Republic

Abstract. The sound production from the Morávka fireball has been examined in detail making use of infrasound and seismic data. A detailed analysis of the production and propagation of sonic waves during the atmospheric entry of the Morávka meteoroid demonstrates that the acoustic energy was produced both by the hypersonic flight of the meteoroid (producing a cylindrical blast wave) and by individual fragmentation events of the meteoroid which acted as small explosions (producing quasi-spherical shock waves). The deviation of the ray normals for the fragmentation events was found to be as much as 30° beyond that expected from a purely cylindrical line source blast. The main fragmentation of the bolide was confined to heights above 30 km, with a possible maximum in acoustic energy production near 38 km. Seismic stations recorded both the direct arrival of the airwaves (the strongest signal) as well as air coupled P-waves and Rayleigh waves (earlier signals). In addition, deep underground stations detected the seismic signature of the fireball. The seismic data alone permit reconstruction of the fireball trajectory to a precision of order a few degrees. The velocity of the meteoroid is much less well determined by these seismic data. The more distant infrasonic station detected three distinct signals from the fireball, identified as a thermospheric return, a stratospheric return and an unusual mode propagating through the stratosphere horizontally and then leaking to the receiver.

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