In this paper we have applied a tau - p inversion method based on a non linear approach to a set of first P-arrival times from a 2-D active seismic experiment performed at Mt. Vesuvius in 1994. The initial seismic investigation is devoted to the study of the shallow structure and the tau - p method has been used for modelling velocity variations of a spherically concentric medium which is a better approximation than a flat layer of the Vesuvius geometry. We are able to obtain detailed 1-D velocity models along different specified sections of the recorded seismic line. These sections span different depth ranges and indicate strong lateral and vertical P-velocity variations in the first 1 km of the volcano structure with values ranging from about 1.5 km/s at the surface to 3.5-4.0 km/s at depth. The average 1-D concentric model obtained in this study call be used as a reasonable starting model for iterative high-resolution tomographies of Vesuvius velocity structures.
P-wave arrival time inversion by using the tau-p method: Application to the Mt Vesuvius volcano, southern Italy / R., Dematteis; Zollo, Aldo; J., Virieux. - In: GEOPHYSICAL RESEARCH LETTERS. - ISSN 0094-8276. - STAMPA. - 24:(1997), pp. 515-518. [10.1029/97GL00186]
P-wave arrival time inversion by using the tau-p method: Application to the Mt Vesuvius volcano, southern Italy
ZOLLO, ALDO;
1997
Abstract
In this paper we have applied a tau - p inversion method based on a non linear approach to a set of first P-arrival times from a 2-D active seismic experiment performed at Mt. Vesuvius in 1994. The initial seismic investigation is devoted to the study of the shallow structure and the tau - p method has been used for modelling velocity variations of a spherically concentric medium which is a better approximation than a flat layer of the Vesuvius geometry. We are able to obtain detailed 1-D velocity models along different specified sections of the recorded seismic line. These sections span different depth ranges and indicate strong lateral and vertical P-velocity variations in the first 1 km of the volcano structure with values ranging from about 1.5 km/s at the surface to 3.5-4.0 km/s at depth. The average 1-D concentric model obtained in this study call be used as a reasonable starting model for iterative high-resolution tomographies of Vesuvius velocity structures.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


