Abstract:The flux of carbon into and out of Earth's surface environment has implications for Earth's climate and habitability. We compiled a global data set for carbon and helium isotopes from volcanic arcs and demonstrated that the carbon isotope composition of mean global volcanic gas is considerably heavier, at -3.8 to -4.6 per mil (‰), than the canonical mid-ocean ridge basalt value of -6.0‰. The largest volcanic emitters outgas carbon with higher δC and are located in mature continental arcs that have accreted car… Show more
“…Allard et al (1991), and Edmonds (2008) pointed out that stronger degassing around the volcanic edifice is not uncommon in volcanic regions. Data on individual volcanoes worldwide are based on the compilation of Mason et al (2017), by Allard (1983), Marty and Giggenbach (1990), Poorter et al (1991), Varekamp et al (1992), Sturchio et al (1993), Sano et al (1994), Sano and Marty (1995), Tedesco et al (1995), Hilton (1996), Sano and Williams (1996), Allard et al (1997), Fischer et al (1998), van Soest et al (1998), Pedroni et al (1999, Lewicki et al (2000), Parello et al (2000), Favara et al (2001), Snyder et al (2001), Shaw et al (2003), Symonds et al (2003) Indeed, the occurrence of high-Mg minerals, such as olivine, clinopyroxene, and orthopyroxene in the dacites (Kiss et al, 2014;Vinkler et al, 2007) suggests that mafic magma also played an important role in the magma evolution.…”
Section: 1029/2018gc008153mentioning
confidence: 99%
“…This high magmatic He content of the gases is not unique and resembles what Trasatti et al (2018) proposed for Colli Albani volcanic complex, another long-dormant volcanic field, where they assumed more than 80% mantle-derived component in the emitted CO 2 gases. Data on individual volcanoes worldwide are based on the compilation of Mason et al (2017) from the data presented by Allard (1983), Marty and Giggenbach (1990), Poorter et al (1991), Varekamp et al (1992), Sturchio et al (1993), Sano et al (1994), Sano and Marty (1995), Tedesco et al (1995), Hilton (1996), Sano and Williams (1996), Allard et al (1997), Fischer et al (1998), van Soest et al (1998, Pedroni et al (1999), Lewicki et al (2000), Parello et al (2000), (Ciotoli et al, 2013) plotting He isotopic ratios (R/R a ) versus 13 C CO2 (VPDB) of Ciomadul gas emissions.…”
Ciomadul is the youngest volcano in the Carpathian‐Pannonian Region, Eastern‐Central Europe, which last erupted 30 ka. This volcano is considered to be inactive, however, combined evidence from petrologic and magnetotelluric data, as well as seismic tomography studies, suggests the existence of a subvolcanic crystal mush with variable melt content. The volcanic area is characterized by high CO2 gas output rate, with a minimum of 8.7 × 103 t/year. We investigated 31 gas emissions at Ciomadul to constrain the origin of the volatiles. The δ13C–CO2 and 3He/4He compositions suggest the outgassing of a significant component of mantle‐derived fluids. The He isotope signature in the outgassing fluids (up to 3.10 Ra) is lower than the values in the peridotite xenoliths of the nearby alkaline basalt volcanic field (R/Ra 5.95 Ra ± 0.01), which are representative of a continental lithospheric mantle and significantly lower than MORB values. Considering the chemical characteristics of the Ciomadul dacite, including trace element and Sr–Nd and O isotope compositions, an upper crustal contamination is less probable, whereas the primary magmas could have been derived from an enriched mantle source. The low He isotopic ratios could indicate a strongly metasomatized mantle lithosphere. This could be due to infiltration of subduction‐related fluids and postmetasomatic ingrowth of radiogenic He. The metasomatic fluids are inferred to have contained subducted carbonate material resulting in a heavier carbon isotope composition (δ13C is in the range of −1.4‰ to −4.6‰) and an increase of CO2/3He ratio. Our study shows the magmatic contribution to the emitted gases.
“…Allard et al (1991), and Edmonds (2008) pointed out that stronger degassing around the volcanic edifice is not uncommon in volcanic regions. Data on individual volcanoes worldwide are based on the compilation of Mason et al (2017), by Allard (1983), Marty and Giggenbach (1990), Poorter et al (1991), Varekamp et al (1992), Sturchio et al (1993), Sano et al (1994), Sano and Marty (1995), Tedesco et al (1995), Hilton (1996), Sano and Williams (1996), Allard et al (1997), Fischer et al (1998), van Soest et al (1998), Pedroni et al (1999, Lewicki et al (2000), Parello et al (2000), Favara et al (2001), Snyder et al (2001), Shaw et al (2003), Symonds et al (2003) Indeed, the occurrence of high-Mg minerals, such as olivine, clinopyroxene, and orthopyroxene in the dacites (Kiss et al, 2014;Vinkler et al, 2007) suggests that mafic magma also played an important role in the magma evolution.…”
Section: 1029/2018gc008153mentioning
confidence: 99%
“…This high magmatic He content of the gases is not unique and resembles what Trasatti et al (2018) proposed for Colli Albani volcanic complex, another long-dormant volcanic field, where they assumed more than 80% mantle-derived component in the emitted CO 2 gases. Data on individual volcanoes worldwide are based on the compilation of Mason et al (2017) from the data presented by Allard (1983), Marty and Giggenbach (1990), Poorter et al (1991), Varekamp et al (1992), Sturchio et al (1993), Sano et al (1994), Sano and Marty (1995), Tedesco et al (1995), Hilton (1996), Sano and Williams (1996), Allard et al (1997), Fischer et al (1998), van Soest et al (1998, Pedroni et al (1999), Lewicki et al (2000), Parello et al (2000), (Ciotoli et al, 2013) plotting He isotopic ratios (R/R a ) versus 13 C CO2 (VPDB) of Ciomadul gas emissions.…”
Ciomadul is the youngest volcano in the Carpathian‐Pannonian Region, Eastern‐Central Europe, which last erupted 30 ka. This volcano is considered to be inactive, however, combined evidence from petrologic and magnetotelluric data, as well as seismic tomography studies, suggests the existence of a subvolcanic crystal mush with variable melt content. The volcanic area is characterized by high CO2 gas output rate, with a minimum of 8.7 × 103 t/year. We investigated 31 gas emissions at Ciomadul to constrain the origin of the volatiles. The δ13C–CO2 and 3He/4He compositions suggest the outgassing of a significant component of mantle‐derived fluids. The He isotope signature in the outgassing fluids (up to 3.10 Ra) is lower than the values in the peridotite xenoliths of the nearby alkaline basalt volcanic field (R/Ra 5.95 Ra ± 0.01), which are representative of a continental lithospheric mantle and significantly lower than MORB values. Considering the chemical characteristics of the Ciomadul dacite, including trace element and Sr–Nd and O isotope compositions, an upper crustal contamination is less probable, whereas the primary magmas could have been derived from an enriched mantle source. The low He isotopic ratios could indicate a strongly metasomatized mantle lithosphere. This could be due to infiltration of subduction‐related fluids and postmetasomatic ingrowth of radiogenic He. The metasomatic fluids are inferred to have contained subducted carbonate material resulting in a heavier carbon isotope composition (δ13C is in the range of −1.4‰ to −4.6‰) and an increase of CO2/3He ratio. Our study shows the magmatic contribution to the emitted gases.
“…Changes in the magma degassing behavior and/or the hydrothermal systems beneath volcanoes generally influence the gas composition and gas fluxes. Measuring the emitted gas composition can provide crucial information on understanding subsurface processes related to activity changes (e.g., Allard et al, 1991;Aiuppa et al, 2007;Bobrowski and Giuffrida, 2012;de Moor et al, 2016a;Liotta et al, 2017) and help to estimate fluxes of the geological carbon cycle (e.g., Burton et al, 2013;Mason et al, 2017) and tectonic processes controlling volcanic degassing (e.g., Aiuppa et al, 2017;de Moor et al 2017). In the field of volcanic monitoring, the observation of gas composition changes has become an important tool for detecting precursory processes for volcanic eruptions.…”
Abstract. Volcanoes are a natural source of several reactive gases (e.g., sulfur and halogen containing species) and nonreactive gases (e.g., carbon dioxide) to the atmosphere. The relative abundance of carbon and sulfur in volcanic gas as well as the total sulfur dioxide emission rate from a volcanic vent are established parameters in current volcanomonitoring strategies, and they oftentimes allow insights into subsurface processes. However, chemical reactions involving halogens are thought to have local to regional impact on the atmospheric chemistry around passively degassing volcanoes. In this study we demonstrate the successful deployment of a multirotor UAV (quadcopter) system with custom-made lightweight payloads for the compositional analysis and gas flux estimation of volcanic plumes. The various applications and their potential are presented and discussed in example studies at three volcanoes encompassing flight heights of 450 to 3300 m and various states of volcanic activity. Field applications were performed at Stromboli volcano (Italy), Turrialba volcano (Costa Rica) and Masaya volcano (Nicaragua). Two in situ gas-measuring systems adapted for autonomous airborne measurements, based on electrochemical and optical detection principles, as well as an airborne sampling unit, are introduced. We show volcanic gas composition results including abundances of CO 2 , SO 2 and halogen species. The new instrumental setups were compared with established instruments during ground-based measurements at Masaya volcano, which resulted in CO 2 / SO 2 ratios of 3.6 ± 0.4. For total SO 2 flux estimations a small differential optical absorption spectroscopy (DOAS) system measured SO 2 column amounts on transversal flights below the plume at Turrialba volcano, giving 1776 ± 1108 T d −1 and 1616 ± 1007 T d −1 of SO 2 during two traverses. At Stromboli volcano, elevated CO 2 / SO 2 ratios were observed at spatial and temporal proximity to explosions by airborne in situ measurements. Reactive bromine to sulfur ratios of 0.19 × 10 −4 to 9.8 × 10 −4 were measured in situ in the plume of Stromboli volcano, downwind of the vent.
“…However, there is work suggesting that arc magmas may be more CO 2 rich than previously hought, and that the arc volcanic CO 2 flux may be correspondingly higher (Blundy et al, ). A large portion of the carbon emitted by these volcanoes may be derived from reworking of crustal carbonate rocks in the upper plate (Mason et al, ). Further, metamorphism in contact aureoles around magmatic intrusions also drives decarbonation reactions (D'Errico et al, ; Lee et al, ).…”
The existence of stabilizing feedbacks within Earth's climate system is generally thought to be necessary for the persistence of liquid water and life. Over the course of Earth's history, Earth's atmospheric composition appears to have adjusted to the gradual increase in solar luminosity, resulting in persistently habitable surface temperatures. With limited exceptions, the Earth system has been observed to recover rapidly from pulsed climatic perturbations. Carbon dioxide (CO2) regulation via negative feedbacks within the coupled global carbon‐silica cycles are classically viewed as the main processes giving rise to climate stability on Earth. Here we review the long‐term global carbon cycle budget, and how the processes modulating Earth's climate system have evolved over time. Specifically, we focus on the relative roles that shifts in carbon sources and sinks have played in driving long‐term changes in atmospheric pCO2. We make the case that marine processes are an important component of the canonical silicate weathering feedback, and have played a much more important role in pCO2 regulation than traditionally imagined. Notably, geochemical evidence indicate that the weathering of marine sediments and off‐axis basalt alteration act as major carbon sinks. However, this sink was potentially dampened during Earth's early history when oceans had higher levels of dissolved silicon (Si), iron (Fe), and magnesium (Mg), and instead likely fostered more extensive carbon recycling within the ocean‐atmosphere system via reverse weathering—that in turn acted to elevate ocean‐atmosphere CO2 levels.
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