Online Material: Figures of waveform fit, apparent source time functions, and video of impact of shock wave at factory. Impacts with our planet cause seismic shaking by a variety of mechanisms. Catastrophic ground motion, even at antipodal distances, can be generated by the extremely infrequent, hypersonic collisions with large asteroids or comets (Meschede et al. , 2011). Fortunately, the atmosphere effectively shields the smaller (and far more common) meteoroids, greatly reducing their initial kinetic energy at high altitude, causing them to slow down, break up, and even vaporize, producing a meteor (Ceplecha and Revelle, 2005). In most instances, the ground shaking is triggered by the atmospheric shock wave of a meteor, not by the impact of the surviving meteorites (Edwards et al. , 2008). A particularly strong shock wave can be generated by explosive fragmentation of the meteoroid in one or several final airbursts (Ceplecha and Revelle, 2005; Edwards et al. , 2008). Such disruptions are triggered when the pressure (ram pressure) caused by atmospheric drag exceeds the internal strength of a meteoroid. They are accompanied by a sudden increase in the meteor luminosity (a flare), because they imply a sharp increase in the surface area being subject to ablation. On 15 February 2013 at 03:20 UTC, an exceptionally large meteor in the region of Chelyabinsk, Russia, produced a powerful shock wave, which caused unprecedented damage to people and property. According to official news reports, glass windows were shattered in over 7300 buildings (some of these even experienced slight structural damage), and falling debris hurt more than 1600 people. The meteorite fragments that survived the atmospheric entry hit the ground at subsonic terminal velocity (Schiermeier, 2013), and did not cause any seismic shaking detectable at regional distances. However, the meteor produced the strongest atmospheric infrasound signal ever recorded (Stone, 2013) and …
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