Analysis of sustained long-period activity at Etna Volcano, Italy |
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| Authors: | Gilberto Saccorotti Ivan Lokmer Christopher J Bean Giuseppe Di Grazia Domenico Patan |
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| Institution: | aIstituto Nazionale di Geofisica e Vulcanologia Sez. di Napoli, Osservatorio Vesuviano, Via Diocleziano, 328- 80124 Napoli, Italy;bSchool of Geological Sciences, University College Dublin, Belfield, Dublin 4, Ireland;cIstituto Nazionale di Geofisica e Vulcanologia, Sez. di Catania. Piazza Roma, 2- 95123 Catania, Italy |
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| Abstract: | Following the installation of a broadband network on Mt. Etna, sustained Long-Period (LP) activity was recorded accompanying a period of total quiescence and the subsequent onset of the 2004–2005 effusive episode. From about 56000 events detected by an automatic classification procedure, we analyse a subset of about 3000 signals spanning the December 17th, 2003–September 25th, 2004, time interval. LP spectra are characterised by several, unevenly-spaced narrow peaks spanning the 0.5–10 Hz frequency band. These peaks are common to all the recording sites of the network, and different from those associated with tremor signals. Throughout the analysed time interval, LP spectra and waveforms maintain significant similarity, thus indicating the involvement of a non-destructive source process that we interpret in terms of the resonance of a fluid-filled buried cavity. Polarisation analysis indicates radiation from a non-isotropic source involving large amounts of shear. Concurrently with LP signals, recordings from the summit station also depict Very-Long-Period (VLP) pulses whose rectilinear motion points to a region located beneath the summit craters at depths ranging between 800 and 1100 m beneath the surface. Based on a refined repicking of similar waveforms, we obtain robust locations for a selected subset of the most energetic LP events from probabilistic inversion of travel-times calculated for a 3D heterogenous structure. LP sources cluster in a narrow volume located beneath the summit craters, and extending to a maximum depth of ≈ 800 m beneath the surface. No causal relationships are observed between LP, VLP and tremor activities and the onset of the 2004–2005 lava effusions, thus indicating that magmatic overpressure played a limited role in triggering this eruption. These data represent the very first observation of LP and VLP activity at Etna during non-eruptive periods, and open the way to the quantitative modelling of the geometry and dynamics of the shallow plumbing system. |
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| Keywords: | long-period seismicity Etna volcano volcano monitoring precursor |
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