IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
L. Wainman, E. Ilyinskaya, M. Pfeffer, C. Mandon, E. Bali, B. A. Edwards, B. I. Kleine-Marshall, S. R. Gudjonsdottir, A. Cotterill, S. W. Scott, P. Wieser, A. Stefánsson, E. J. Nicholson, J. Sepulveda-Araya, S. J. Hammond, B. E. Kunz, F. Jenner, J. R. Gunnarsson, A. Aiuppa, M. Burton, T. A. Mather
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引用次数: 0

摘要

玄武岩裂隙喷发会向对流层低层排放挥发性和环境反应性气体和微粒物质(PM)(如气相中的二氧化硫、氯化氢和氟化氢;微粒物质中的Se、As和Pb复合物)。裂隙喷发产生的熔岩流空间范围很广,但与主喷口的熔岩流相比,其排放物的成分和通量特征却很不明显。利用无人机采样系统和地面遥控傅立叶变换红外光谱仪,我们研究了法格拉德尔斯菲亚尔 2021-2023 年喷发期间活动熔岩流排放物的顺流成分演变。计算得出的熔岩流挥发性痕量金属通量与冰岛的主喷口脱气和人为通量相比都相当可观。我们展示了主要气体排放中的分馏现象,即随着 S/ 卤素比率的下降而向下流动。这种 S-Cl 分馏反映在痕量元素脱气剖面上,在下流排放中,主要与硫络合的元素(如 Se、Te、As、Pb)的丰度相对于与氯化物(如 Cu、Rb、Cs)、氧化物(如 La、Ce)和氢氧化物(如 Fe、Mg、Al、Ti)络合的元素减少得更快。利用热化学模型,我们通过熔岩流老化和冷却过程中与温度和成分有关的元素种类来解释这种关系。因此,与主喷口或更接近熔岩流的排放物相比,一些氯化物络合元素(如铜)在更下游的排放物中变得相对更多。这种顺流元素通量的变化表明,向环境排放的金属可能会随着熔岩流的年龄和热演化而发生变化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Trace Element Emissions Vary With Lava Flow Age and Thermal Evolution During the Fagradalsfjall 2021–2023 Eruptions, Iceland

Trace Element Emissions Vary With Lava Flow Age and Thermal Evolution During the Fagradalsfjall 2021–2023 Eruptions, Iceland

Basaltic fissure eruptions emit volatile and environmentally reactive gases and particulate matter (PM) into the lower troposphere (e.g., SO2, HCl, and HF in the gas phase; Se, As, Pb as complexes in the PM phase). Lava flows from fissure eruptions can be spatially extensive, but the composition and fluxes of their emissions are poorly characterized compared to those from main vent(s). Using uncrewed aircraft systems-mounted (drone) samplers and ground-based remote Fourier Transform Infrared Spectroscopy, we investigated the down-flow compositional evolution of emissions from active lava flows during the Fagradalsfjall 2021–2023 eruptions. The calculated fluxes of volatile trace metals from lava flows are considerable relative to both main vent degassing and anthropogenic fluxes in Iceland. We demonstrate a fractionation in major gas emissions with decreasing S/halogen ratio down-flow. This S-Cl fractionation is reflected in the trace element degassing profile, where the abundance of predominantly sulfur-complexing elements (e.g., Se, Te, As, Pb) decreases more rapidly in down-flow emissions relative to elements complexing as chlorides (e.g., Cu, Rb, Cs), oxides (e.g., La, Ce) and hydroxides (e.g., Fe, Mg, Al, Ti). Using thermochemical modeling, we explain this relationship through temperature and composition dependent element speciation as the lava flow ages and cools. As a result, some chloride-complexing elements (such as Cu) become relatively more abundant in emissions further down-flow, compared to emissions from the main vent or more proximal lava flows. This variability in down-flow element fluxes suggests that the output of metals to the environment may change depending on lava flow age and thermal evolution.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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