Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11625
Authors: Aiuppa, Alessandro* 
de Moor, J. Maarten* 
Arellano, Santiago* 
Coppola, Diego* 
Francofonte, Vincenzo* 
Galle, Bo* 
Giudice, Gaetano* 
Liuzzo, Marco* 
Mendoza, Elvis* 
Saballos, Armando* 
Tamburello, Giancarlo* 
Battaglia, Angelo* 
Bitetto, Marcello* 
Gurrieri, Sergio* 
Laiolo, Marco* 
Mastrolia, Andrea* 
Moretti, Roberto* 
Title: Tracking Formation of a Lava Lake From Ground and Space: Masaya Volcano (Nicaragua), 2014-2017
Issue Date: Feb-2018
Series/Report no.: 2/19 (2018)
DOI: 10.1002/2017GC007227
URI: http://hdl.handle.net/2122/11625
Abstract: A vigorously degassing lava lake appeared inside the Santiago pit crater of Masaya volcano (Nicaragua) in December 2015, after years of degassing with no (or minor) incandescence. Here we present an unprecedented-long (3 years) and continuous volcanic gas record that instrumentally characterizes the (re)activation of the lava lake. Our results show that, before appearance of the lake, the volcanic gas plume composition became unusually CO2 rich, as testified by high CO2/SO2 ratios (mean: 12.2 ± 6.3) and low H2O/CO2 ratios (mean: 2.3 ± 1.3). The volcanic CO2 flux also peaked in November 2015 (mean: 81.3 ± 40.6 kg/s; maximum: 247 kg/s). Using results of magma degassing models and budgets, we interpret this elevated CO2 degassing as sourced by degassing of a volatile-rich fast-overturning (3.6–5.2 m3 s−1) magma, supplying CO2-rich gas bubbles from minimum equivalent depths of 0.36–1.4 km. We propose this elevated gas bubble supply destabilized the shallow (<1 km) Masaya magma reservoir, leading to upward migration of vesicular (buoyant) resident magma, and ultimately to (re)formation of the lava lake. At onset of lava lake activity on 11 December 2015 (constrained by satellite-based MODIS thermal observations), the gas emissions transitioned to more SO2-rich composition, and the SO2 flux increased by a factor ∼40% (11.4 ± 5.2 kg/s) relative to background degassing (8.0 kg/s), confirming faster than normal (4.4 versus ∼3 m3 s−1) shallow magma convection. Based on thermal energy records, we estimate that only ∼0.8 of the 4.4 m3 s−1 of magma actually reached the surface to manifest into a convecting lava lake, suggesting inefficient transport of magma in the near-surface plumbing system.
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