Very-small-aperture 3-D infrasonic array for volcanic jet observation at Stromboli Volcano
SUMMARY This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has become important in the analysis of volcanic jet noise or geological flows on steep mountain slopes. Although a VSA infrasonic array, with an ap...
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| Published in | Geophysical journal international Vol. 229; no. 1; pp. 459 - 471 |
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| Main Authors | , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Oxford University Press
01.04.2022
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| Subjects | |
| Online Access | Get full text |
| ISSN | 0956-540X 1365-246X 1365-246X |
| DOI | 10.1093/gji/ggab487 |
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| Abstract | SUMMARY
This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has become important in the analysis of volcanic jet noise or geological flows on steep mountain slopes. Although a VSA infrasonic array, with an aperture as small as a few tens of metres, has recently been shown to have a sufficient resolution of the backazimuth (BAZ) of incident signals, its BEL resolution is considered to be poor. We performed a four-element 3-D array experiment with a 20-m aperture and 2-m height at the summit of Stromboli Volcano. We analysed the direction of arrival (DOA) with the MUSIC algorithm as a function of frequency and conducted a cluster analysis for the estimated DOA–frequency functions of eruption signals. As a result, individual infrasonic signals were successfully related to eruptive vents. We also calculated the standard deviation (STD) of the DOAs in each cluster. Of the observed BAZ-STDs and BEL-STDs, 80 per cent were <2.0° and <4.6°, respectively. A comparison among the array geometries showed that the installation of a sensor above the ground, even at only 2 m, improved the BEL resolution, indicating that the VSA-3D array provides more detailed information about the wavefield than a planar array. The observed signals had higher BELs (−20° to 0°) than the vent direction (−30° to −25°) at 3–6 Hz, although signals above 20 Hz arrived from the vent direction. Our array verified that such DOA deviations were significant by the STD analysis and some tests with synthetic data. We infer that the DOA deviations do not indicate the source location and are caused by topographical diffraction. |
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| AbstractList | This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has become important in the analysis of volcanic jet noise or geological flows on steep mountain slopes. Although a VSA infrasonic array, with an aperture as small as a few tens of metres, has recently been shown to have a sufficient resolution of the backazimuth (BAZ) of incident signals, its BEL resolution is considered to be poor. We performed a four-element 3-D array experiment with a 20-m aperture and 2-m height at the summit of Stromboli Volcano. We analysed the direction of arrival (DOA) with the MUSIC algorithm as a function of frequency and conducted a cluster analysis for the estimated DOA–frequency functions of eruption signals. As a result, individual infrasonic signals were successfully related to eruptive vents. We also calculated the standard deviation (STD) of the DOAs in each cluster. Of the observed BAZ-STDs and BEL-STDs, 80 per cent were <2.0° and <4.6°, respectively. A comparison among the array geometries showed that the installation of a sensor above the ground, even at only 2 m, improved the BEL resolution, indicating that the VSA-3D array provides more detailed information about the wavefield than a planar array. The observed signals had higher BELs (−20° to 0°) than the vent direction (−30° to −25°) at 3–6 Hz, although signals above 20 Hz arrived from the vent direction. Our array verified that such DOA deviations were significant by the STD analysis and some tests with synthetic data. We infer that the DOA deviations do not indicate the source location and are caused by topographical diffraction. SUMMARY This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has become important in the analysis of volcanic jet noise or geological flows on steep mountain slopes. Although a VSA infrasonic array, with an aperture as small as a few tens of metres, has recently been shown to have a sufficient resolution of the backazimuth (BAZ) of incident signals, its BEL resolution is considered to be poor. We performed a four-element 3-D array experiment with a 20-m aperture and 2-m height at the summit of Stromboli Volcano. We analysed the direction of arrival (DOA) with the MUSIC algorithm as a function of frequency and conducted a cluster analysis for the estimated DOA–frequency functions of eruption signals. As a result, individual infrasonic signals were successfully related to eruptive vents. We also calculated the standard deviation (STD) of the DOAs in each cluster. Of the observed BAZ-STDs and BEL-STDs, 80 per cent were <2.0° and <4.6°, respectively. A comparison among the array geometries showed that the installation of a sensor above the ground, even at only 2 m, improved the BEL resolution, indicating that the VSA-3D array provides more detailed information about the wavefield than a planar array. The observed signals had higher BELs (−20° to 0°) than the vent direction (−30° to −25°) at 3–6 Hz, although signals above 20 Hz arrived from the vent direction. Our array verified that such DOA deviations were significant by the STD analysis and some tests with synthetic data. We infer that the DOA deviations do not indicate the source location and are caused by topographical diffraction. |
| Author | Ripepe, Maurizio Yamakawa, Kazuya Lacanna, Giorgio Sánchez, Claudia Ichihara, Mie |
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| Cites_doi | 10.1109/PROC.1969.7278 10.1029/2008JB006128 10.1002/2015GL065024 10.1002/2017GL074971 10.1002/2014GL061597 10.1111/j.1365-246X.2012.05696.x 10.1785/0220140047 10.1029/2008GL036486 10.1080/01621459.1963.10500845 10.1002/2017GL076506 10.4294/jpe1952.45.397 10.1016/j.jvolgeores.2011.06.006 10.1093/gji/ggaa010 10.1109/TAP.1986.1143830 10.1111/j.1365-246X.2011.04948.x 10.1002/2013JB010303 10.1038/232253a0 10.1029/2018JB015561 10.1016/j.coldregions.2011.09.006 10.1146/annurev-earth-042711-105508 10.2307/2528688 10.1017/S0022112008003704 10.1029/2011JD016760 10.1093/gji/ggw150 10.1007/978-1-4020-9508-5_2 10.1002/2013JB010827 10.1093/comjnl/9.4.373 10.1029/2009EO270001 10.1029/2002GL015452 10.1029/2006JB004613 10.1109/RBME.2010.2083647 10.1029/2005GL023893 10.1016/j.jvolgeores.2014.06.015 10.1144/M39.9 10.1260/026309205775374451 10.1029/2018GL078851 10.1111/j.1365-246X.2011.04951.x 10.1029/2008JB006007 10.1260/147547207783359459 10.1029/2019JD030386 |
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| Keywords | Infrasound Volcano monitoring Time-series analysis Statistical methods Wave propagation Waveform analysis |
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This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has... This study tested a very-small-aperture 3-D (VSA-3D) infrasonic array. A 3-D array is ideal for resolving the back elevation angle (BEL), which has become... |
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| Title | Very-small-aperture 3-D infrasonic array for volcanic jet observation at Stromboli Volcano |
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