Monitoring crustal changes at volcanoes by seismic noise interferometry: Mt. Etna case of study

被引:11
作者
Cannata, Andrea [1 ,2 ]
Cannavo, Flavio [2 ]
Montalto, Placido [2 ]
Ercoli, Maurizio [1 ]
Mancinelli, Paolo [1 ]
Pauselli, Cristina [1 ]
Leto, Giuseppe [3 ]
机构
[1] Univ Perugia, Dipartimento Fis & Geol, Perugia, Italy
[2] INGV, Osservatorio Etneo, Sez Catania, Catania, Italy
[3] INAF, Osservatorio Astrofis Catania, Catania, Italy
关键词
Seismic noise interferometry; Mt; Etna; Meteorological parameters; Volcanic tremor; VELOCITY; COHERENCE; BEHAVIOR;
D O I
10.1016/j.jvolgeores.2017.03.023
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
In this work, we analysed the seismic noise recorded at Mt. Etna by 18 stations during the interval 2007-2015 in the frequency band 0.1-03 Hz, chosen to avoid contamination from volcanic tremor. Variations in time of medium seismic velocity in the range -0.8 to 0.8% were found, mostly affecting the stations located on the volcano summit and flanks. Based on the investigated frequency content, the Delta v/v changes took place from the surface to a depth of -4.5-6.5 km. To identify the source mechanism of the observed medium changes, the variations were quantitatively compared by wavelet transform coherence with volcano-tectonic and meteorological parameters. A significant relationship with meteorological parameters with seasonal periodicity (especially air temperature, and snow loading) was found, probably caused by thermo-elastic strain and increasing-decreasing surface loading cycles. Moreover, a sharp medium velocity decrease, taking place in mid-December 2009 and clearly time-related to the largest volcano-tectonic strain release phenomenon of the investigated period, was also found. Such a velocity decrease was interpreted as resulting from ascent of fluids and gas exsolution taking place at the same time as the volcano-tectonic swarm. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:165 / 174
页数:10
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