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Age-clustered eruptive activity at La Palma (Canary Islands) during the last 4000 years: Evidence from paleomagnetic dating

JVGR, Magli et al. 2025 - Figure 2
Figure 2. Images of sampling sites. (a): PAL03 site, overview of the contact (the dashed white line) between the Malforada–Nambroque lava flow and the younger AD 1949 flow. (b): PAL08 site, view of Montaña Quemada lava flow with its massive core. (c): PAL10 site, photograph of a Martín flow outcrop. (d): PAL25 site, particular of the Fuego flow unit. (e): PAL14 site, landscape image of the La Fajana lava flow reaching the coast. (f): overview of the La Caldereta scoria cone with the location of two paleomagnetic sites (PAL26 and PAL27). (g): PAL28 site, panoramic view of the inner walls of the crater of the San Antonio scoria cone showing pyroclasts of the AD 1677 Strombolian eruption resting on the pre-historic San Antonio phreatomagmatic deposits (according to Carracedo et al., 1996).

Magli A., P. Del Carlo, A. Di Roberto, G. Giordano, S. Meletlidis, M. Pompilio, F. Speranza, (2025).
Journal of Volcanology and Geothermal Research, https://doi.org/10.1016/j.jvolgeores.2025.108328

Abstract

The detailed knowledge of timing and dynamics of pre-historic eruptions is pivotal for volcanic hazard assessment. This is most relevant for inhabited lower slopes of active basaltic volcanoes such as La Palma (Canary Islands), where the 2021 Tajogaite eruption caused severe destruction. We paleomagnetically investigated eight La Palma Holocene eruptions which are currently loosely constrained either by few radiometric (K/Ar and 14C) ages, or by stratigraphic/archaeological evidence. The paleomagnetic directions gathered from 28 sites (300 oriented cores) were compared with updated reference models of the paleo-secular variation of the geomagnetic field direction during the Holocene. Overlapping paleomagnetic directions from the Fuego and La Fajana lava flows, along with geologic and geochemical evidence, imply that the two flows were emplaced during the same eruptive event falling within the 2000–1730 BC time window. Single paleomagnetic age windows – consistent with and narrower than available 14C age intervals – were obtained for the Malforada–Nambroque, Montaña Quemada, and Fuego–La Fajana lava flows. Conversely, the Martín, Birigoyo–La Barquita, and La Caldereta flows yielded multiple age solutions. Moreover, our data show that the flanks of the pre-historic San Antonio scoria cone are almost totally covered by pyroclastic products of the nearby AD 1677 Fuencaliente eruption. The updated chronologic framework of the pre-historic volcanic activity at La Palma demonstrates that the past four kyr are characterized by an early period with low-frequency eruptions (three lava flow eruptions between ca. 2000 BC and 300 BC), followed by a ca. 1000 yr-long quiescence period, and by a subsequent clustering of nine events during the last 1100 yr (about one eruption per century).