EGU26-10109, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-10109
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 06 May, 16:15–18:00 (CEST), Display time Wednesday, 06 May, 14:00–18:00
 
Hall X1, X1.109
Jet flow dynamics of explosive eruptions: laboratory and numerical investigation of shock-tube experiments
Giuseppe La Spina1, Laura Spina2, Jacopo Taddeucci2, Francesco Pennacchia2, Alessio Posati3, Diego Perugini3, and Piergiorgio Scarlato2
Giuseppe La Spina et al.
  • 1Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Etneo, Sezione di Catania, Catania, Italy (giuseppe.laspina@ingv.it)
  • 2Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Roma1, Roma, Italy
  • 3Università degli Studi di Perugia, Dipartimento di Fisica e Geologia, Perugia, Italy

Explosive eruptions represent the most powerful and hazardous manifestations of volcanic activity on Earth. During such events, a high-velocity gas/pyroclast mixture is injected in the atmosphere, producing ash columns that can reach altitudes of tens of kilometres. Depending on atmospheric conditions and eruption intensity, these ash clouds can travel thousands of kilometres, potentially disrupting the air-traffic and the climate worldwide.

Jet flow dynamics of explosive eruptions are affected by several parameters, including pressure gradient, temperature of the magmatic mixture, particle mass and size distribution, and vent geometry. However, most of these parameters cannot be measured directly during an eruption. Conversely, some of the characteristics of the volcanic jets, such as exit velocity, jet dimension, and acoustic signals, can be collected by volcanic monitoring systems.

To correlate jet flow characteristics with magmatic conditions below the vent of the conduit, we investigated jet flow dynamics using a combination of shock-tube experiments and numerical simulations. Data from laboratory experiments were collected using a high-speed camera to capture the evolution of the jet at high temporal resolution, as well as acoustic signals from microphones. Schlieren shadow photography has also been adopted to visualise shock waves and density contrasts within the gas during the experiments. Using this setup we investigated the role of particles on jet flow characteristics. Preliminary results indicate that in the supersonic regime, both the amplitude of acoustic signals and the spectral properties of the signal are influenced by solid loading. Finally, transient numerical simulations of the shock-tube experiments were also performed to correlate the evolution of the jet features with the internal thermodynamic conditions of the gas/pyroclast mixture.

How to cite: La Spina, G., Spina, L., Taddeucci, J., Pennacchia, F., Posati, A., Perugini, D., and Scarlato, P.: Jet flow dynamics of explosive eruptions: laboratory and numerical investigation of shock-tube experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10109, https://doi.org/10.5194/egusphere-egu26-10109, 2026.