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Earth, Planets and Space
Fig. 3 | Earth, Planets and Space

Fig. 3

From: Gas flow dynamics in the conduit of Strombolian explosions inferred from seismo-acoustic observations at Aso volcano, Japan

Fig. 3

Histograms of observed differences in seismo-acoustic signal arrival times. a Distribution of time differences between the arrival of the VLP seismic signal at UMA and the arrival of the low-frequency infrasound signal at ACM, ΔtsL–iL. b Distribution of time differences between the eruption earthquake at KAF and the high-frequency infrasound signal at ACM, ΔtsH–iH. c Distribution of time differences between low- and high-frequency infrasound signals at ACM, ΔtiL–iH. The total number of events (N) and the mean and mode values are shown in the upper right in each diagram

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