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Physical and chemical characteristics of active sulfur flows observed at Lastarria volcano (northern Chile) in January 2019
Indexado
WoS WOS:001025110100001
Scopus SCOPUS_ID:85164565202
DOI 10.3389/FEART.2023.1197363
Año 2023
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Molten sulfur is found in various subaerial volcanoes. However, limited records of the pools and flows of molten sulfur have been reported: therefore, questions remain regarding the physicochemical processes behind this phenomenon. A suite of new sulfur flows, some of which active, was identified at the Lastarria volcano (northern Chile) and studied using satellite imagery, in situ probing, and temperature and video recording. This finding provides a unique opportunity to better understand the emplacement mechanisms and mineral and chemical compositions of molten sulfur, in addition to gaining insight into its origin. Molten sulfur presented temperatures of 124–158°C, with the most prolonged sulfur flow reaching 12 m from the source. Photogrammetric tools permitted the identification of levees and channel structures, with an estimated average flow speed of 0.069 m/s. Field measurements yielded a total volume of 1.45 ± 0.29 m3 of sulfur (equivalent to ∼2.07 tons) mobilized during the January 2019 event for at least 408 min. Solidified sulfur was composed of native sulfur with minor galena and arsenic- and iodine-bearing minerals. Trace element analysis indicated substantial enrichment of Bi, Sb, Sn, Cd, as well as a very high concentration of As (>40.000 ppm). The January 2019 molten sulfur manifestations in Lastarria appear to be more enriched in As compared to the worldwide known volcanoes with molten sulfur records, such as the Shiretoko-Iozan and Poás volcanoes. Furthermore, their rheological properties suggest that the “time of activity” in events such as this could be underestimated as flows in Lastarria have moved significantly slower than previously thought. The origin of molten sulfur is ascribed to the favorable S-rich chemistry of fumarolic gases and changes in host rock permeability (fracture opening). Molten sulfur in Lastarria correlates with a peak in activity characterized by high emissions of SO2 and other acid species, such as HF and HCl, in addition to ground deformation. Consequently, molten sulfur was framed within a period of volcanic unrest in Lastarria, triggered by changes in the magmatic-hydrothermal system. The appearance of molten sulfur is related to physicochemical perturbations inside the volcanic system and is perhaps a precursor of eruptive activity, as observed in the Poás and Turrialba volcanoes.

Revista



Revista ISSN
Frontiers In Earth Science 2296-6463

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Disciplinas de Investigación



WOS
Geosciences, Multidisciplinary
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Inostroza, Manuel Hombre Instituto Milenio de Investigación en Riesgo Volcánico - Chile
2 Fernandez, Bárbara Mujer Universidad Católica del Norte - Chile
3 AGUILERA-VALENZUELA, FELIPE IGNACIO Hombre Instituto Milenio de Investigación en Riesgo Volcánico - Chile
Universidad Católica del Norte - Chile
4 Layana, Susana Mujer Instituto Milenio de Investigación en Riesgo Volcánico - Chile
5 Walter, Thomas R. Hombre Deutsches GeoForschungsZentrum (GFZ) - Alemania
GFZ German Res Ctr Geosci - Alemania
6 Zimmer, Martin Hombre Deutsches GeoForschungsZentrum (GFZ) - Alemania
GFZ German Res Ctr Geosci - Alemania
7 Rodríguez-Díaz, Augusto Hombre Universidad Nacional Autónoma de México - México
Univ Nacl Autonoma Mexico - México
8 Oelze, Marcus Hombre Deutsches GeoForschungsZentrum (GFZ) - Alemania
Federal Institute for Materials Research and Testing Berlin - Alemania
GFZ German Res Ctr Geosci - Alemania
Bundesanstalt Mat Forsch & Prufung BAM - Alemania
Bundesanstalt für Materialforschung und -Prüfung - Alemania

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Financiamiento



Fuente
FONDECYT
Fondo Nacional de Desarrollo Científico y Tecnológico
Fondo de Innovación para la Competitividad
FIC-R BIP
ANID-PCHA/Doctorado Nacional
Instituto de Geofisica
Mitigación de los Riesgos Asociados a Procesos Volcánicos en la Región de Antofagasta
ANID-PCHA/Doctorado Nacional/201621160172
ANID-PCHA/Doctorado Nacional/21160276
Instituto de Geofisica, UNAM

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
MI was funded by ANID-PCHA/Doctorado Nacional/201621160172. SL was funded by ANID-PCHA/Doctorado Nacional/21160276. This study was partially funded by FIC-R BIP 30488832-0 project “Mitigación de los Riesgos Asociados a Procesos Volcánicos en la Región de Antofagasta”, National Research Funding Competition FONDECYT Regular 2021 Code 1211220, and by the internal project of the Instituto de Geofísica, UNAM N103 “Analogías de sistemas hidrotermales fósiles (minería) y activos (geotermia).”
MI was funded by ANID-PCHA/Doctorado Nacional/201621160172. SL was funded by ANID-PCHA/Doctorado Nacional/21160276. This study was partially funded by FIC-R BIP 30488832-0 project "Mitigacion de los Riesgos Asociados a Procesos Volcanicos en la Region de Antofagasta", National Research Funding Competition FONDECYT Regular 2021 Code 1211220, and by the internal project of the Instituto de Geofisica, UNAM N103 "Analogias de sistemas hidrotermales fosiles (mineria) y activos (geotermia)."

Muestra la fuente de financiamiento declarada en la publicación.