Publications

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Seismology on Venus has long eluded planetary scientists due to extreme temperature and pressure conditions on its surface, which most electronics cannot withstand for mission durations required for ground-based seismic studies. Here, we show that infrasonic (low-frequency) pressure fluctuations, generated as a result of ground motion, produced by an artificial seismic source known as a seismic hammer, and recorded using sensitive microbarometers deployed on a tethered balloon, are able to replicate the frequency content of ground motion. We also show that weak, artificial seismic activity thus produced may be geolocated by using multiple airborne barometers. The success of this technique paves the way for balloon-based aero-seismology, leading to a potentially revolutionary method to perform seismic studies from a remote airborne station on the earth and solar system objects with substantial atmospheres such as Venus and Titan.

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Subterranean energy releases such as explosions and earthquakes may disturb the Earth-atmosphere interface, creating acoustic waves that can travel great distances. These waves provide a record of the ground motion directly above the event. The information they encode may provide critical insight into the depth and size of underground explosions, the sequence of events immediately before volcanic eruptions, and the magnitude of strong motion resulting from earthquakes. However, the effect of event size and burial depth on the resulting acoustic wave has not been explored in detail. Here, the relationship between acoustic amplitude, frequency, and energy is investigated for a series of well-characterized underground chemical explosions in granite. Acoustic amplitude was found to vary linearly with explosive yield divided by emplacement depth. Peak acoustic frequency appears to be a function of explosive yield alone. The ratio of radiated acoustic energy to source energy had a relatively poor fit to yield, depth, and combinations thereof. These relationships suggest that acoustic analysis can be used to determine the size and depth of a buried explosion. The results presented here have particular relevance to the nuclear monitoring community, because depth is difficult to determine with seismic methods.

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Strong ground motion induces acoustic waves in the atmosphere that can be detected at great distances. These waves provide a record of acceleration at the epicenter of the subterranean event. While this information is valuable for nuclear monitoring purposes, a systematic study of the variation in acoustic parameters with explosive yield and depth has not yet been conducted. Here, we provide a survey of low frequency sound waves generated during the Source Physics Phase 1 experiment, in which six chemical explosions were detonated in granite. We found that pressure amplitudes increase with explosion size but decrease with depth as expected. Pressure amplitude variability increased with signal magnitude. Surprisingly, peak frequency appears to increase with depth. A possible directional signal was identified for one of the events as well. The results presented here may aid the nuclear monitoring community in developing means of determining event depth and yield using acoustic methods. This will complement existing algorithms based on seismic radiation.

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