EGU23-3556
https://doi.org/10.5194/egusphere-egu23-3556
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

An investigation of high frequency seismic tremor on Mt Etna

Maurice Weber1, Christopher Bean1, Ivan Lokmer2, Patrick Smith1, Luciano Zuccarello3,4, Silvio De Angelis3,4, and Vittorio Minio5
Maurice Weber et al.
  • 1Dublin Institute for Advanced Studies, Dublin, Ireland (mweber@cp.dias.ie)
  • 2University College Dublin, Dublin, Ireland
  • 3Instituto Nazionale di Geofisica e Vulcanologia, Sezione di Pisa, Pisa, Italy
  • 4University of Liverpool, Liverpool, UK
  • 5University of Catania, Catania, Italy

High frequency seismic data (> 10 Hz) on volcanoes have traditionally been less studied as precursory seismicity to volcanic eruptions is dominated by lower frequency signals. However, inspection of newly acquired data during a field campaign between July and September 2022 from individual high sampling rate seismic stations on Mt. Etna reveals the presence of high frequency (10-90Hz) signals, which are poorly understood. In an attempt to determine their location, mechanisms and wavefield properties, we deployed 104 nodal seismic sensors, mainly in 6 tuned circular array configurations consisting of several rings with increasing radius and number of nodes per ring around a central station. The nodes record at a sampling rate of 250Hz (125Hz Nyquist) and the frequency content of the recorded seismicity shows signals up to about 100 Hz. In addition to the high frequency nodes, we also deployed a profile consisting of 11 elements (infrasound, short period) as well as four broad band sensors.

A variety of signals were recorded, with coherent signals on different stations across the full spectral range. Thus far initial multi-array beamforming has been applied to the data, demonstrating a range of locations which varies depending on the frequency range looked at. Whilst sources near the summit region are most common (especially at frequencies below 5 Hz), there are also other locations from which tremor emanates, opening questions about their origin.  Comparisons with infrasound, gas and weather data are ongoing, in an effort to shed light on the sources of these unusual signals.

How to cite: Weber, M., Bean, C., Lokmer, I., Smith, P., Zuccarello, L., De Angelis, S., and Minio, V.: An investigation of high frequency seismic tremor on Mt Etna, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-3556, https://doi.org/10.5194/egusphere-egu23-3556, 2023.

Supplementary materials

Supplementary material file