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Twin digital short period seismic Array Experiment at Stromboli Volcano

Author(s)
Del Pezzo, E.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
La Rocca, M.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
Petrosino, S.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
Grozea, B.  
Università di Salerno  
Maritato, L.  
Università di Salerno  
Saccorotti, G.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Pisa, Pisa, Italia  
Simini, M.  
Università di Salerno  
Ibanez, J.  
Instituto Andaluz de Geofisica  
Alguacil, G.  
Instituto Andaluz de Geofisica  
Carmona, E.  
Instituto Andaluz de Geofisica  
Abril, M.  
Instituto Andaluz de Geofisica  
Almendros, J.  
Instituto Andaluz de Geofisica  
Ortiz, R.  
Museo Naccional de Ciencias Naturales de Madrid  
Garcia, A.  
Museo Naccional de Ciencias Naturales de Madrid  
Pingue, F.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
Esposito, T.  
Osservatorio Vesuviano  
Sponsors
INGV - Osservatorio Vesuviano
Language
English
Status
Unpublished
Peer review journal
No
Date Issued
1998
Alternative Location
http://www.ov.ingv.it/doc/ofr98001.pdf
Series/Report No.
ofr98001
URI
https://www.earth-prints.org/handle/2122/3552
Subjects
04. Solid Earth::04.06. Seismology::04.06.10. Instruments and techniques  
Subjects

Stromboli

Twin array experiment...

Abstract
Two small arrays composed by short period (1 Hz) digital seismic
stations, with an aperture of approximately 400 meters, were set up at
Stromboli volcano (one at semaforo Labronzo, the other at Ginostra-
Timpone del Fuoco) with the purpose of the spatial location of the high
frequency source of the explosion quakes.
About 75 explosion-quakes were recorded at both arrays, and
constitute the available data base.
We have planned to apply the zero-lag cross-correlation technique to
the whole data set in order to obtain back-azimuth and apparent
slowness of the coherent seismic phases. A preliminary analysis for
both arrays show that the predominant back-azimuth for the first phase
is oriented in the direction of , but not strictly coincident to, the crater
area. Moreover some back-scattered arrivals are quite evident in the
seismogram.
Type
report
File(s)
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ofr98001.pdf

Description
report
Size

413.49 KB

Format

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Checksum (MD5)

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