Abstract

On 13 December 2020, Etna volcano entered a new eruptive phase, giving rise to a number of paroxysmal episodes involving increased Strombolian activity from the summit craters, lava fountains feeding several-km high eruptive columns and ash plumes, as well as lava flows. As of 2 August 2021, 57 such episodes have occurred in 2021, all of them from the New Southeast Crater (NSEC). Each paroxysmal episode lasted a few hours and was sometimes preceded (but more often followed) by lava flow output from the crater rim lasting a few hours. In this paper, we use remote sensing data from the ground and satellite, integrated with ground deformation data recorded by a high precision borehole strainmeter to characterize the 12 March 2021 eruptive episode, which was one of the most powerful (and best recorded) among that occurred since 13 December 2020. We describe the formation and growth of the lava fountains, and the way they feed the eruptive column and the ash plume, using data gathered from the INGV visible and thermal camera monitoring network, compared with satellite images. We show the growth of the lava flow field associated with the explosive phase obtained from a fixed thermal monitoring camera. We estimate the erupted volume of pyroclasts from the heights of the lava fountains measured by the cameras, and the erupted lava flow volume from the satellite-derived radiant heat flux. We compare all erupted volumes (pyroclasts plus lava flows) with the total erupted volume inferred from the volcano deflation recorded by the borehole strainmeter, obtaining a total erupted volume of ~3 × 106 m3 of magma constrained by the strainmeter. This volume comprises ~1.6 × 106 m3 of pyroclasts erupted during the lava fountain and 2.4 × 106 m3 of lava flow, with ~30% of the erupted pyroclasts being remobilized as rootless lava to feed the lava flows. The episode lasted 130 min and resulted in an eruption rate of ~385 m3 s−1 and caused the formation of an ash plume rising from the margins of the lava fountain that rose up to 12.6 km a.s.l. in ~1 h. The maximum elevation of the ash plume was well constrained by an empirical formula that can be used for prompt hazard assessment.

Highlights

  • Explosive eruptions of mafic magmas produce lava fountains whose heights depend on the exsolved volatile content of the magma, its erupted mass flux, and the geometry of the vent, either an elongated eruptive fissure or a near circular conduit [1].Lava fountains were typical at Kilauea volcano during the 1959–1960, 1969–1970, and1983–2008 eruptions [2,3,4,5], being characterized by vertical jets of gas and incandescent pyroclasts rising several hundred meters above the vent

  • We present details on the lava fountains and their connections with ash plume and lava flow field formation, as well as persistence and decline gathered from a network of ground-based monitoring cameras and from high temporal resolution satellite sensors (e.g., SEVIRI, MODIS, and VIIRS)

  • Our results have essential implications in regard to hazard assessments at Etna during paroxysmal explosive phases. They confirm the role of wind speed [15] in determining if a strong, intermediate, or weak ash plume forms, with wind speeds below 10 m s−1 favoring the formation of strong to intermediate, taller vertical plumes, which cause most of the pyroclastic fallout around the vent

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Summary

Introduction

1983–2008 eruptions [2,3,4,5], being characterized by vertical jets of gas and incandescent pyroclasts rising several hundred meters above the vent. This activity is common at Etna volcano, with several such explosive phases occurring in 2000 [6,7,8], 2001, 2002–. 2021, 13, 3052 over time [17] This is in agreement with a general trend of increasing heights and volume of the lava fountains and ash plumes from 2000 until now [6,8,10,11,12,14,15]

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