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Recent Advances in Volcanic Gas Science

Original Research ARTICLE Provisionally accepted The full-text will be published soon. Notify me

Front. Earth Sci. | doi: 10.3389/feart.2019.00154

Reaction rates control high-temperature chemistry of volcanic gases in air

  • 1UMR7328 Laboratoire de physique et chimie de l'environnement et de l'Espace (LPC2E), France
  • 2UPR3021 Institut de combustion, aérothermique,réactivité et environnement (ICARE), France
  • 3University of Cambridge, United Kingdom

When volcanic gases enter the atmosphere, they encounter a drastically different chemical and physical environment, triggering a range of rapid processes including photochemistry, oxidation and aerosol formation. These processes are critical to understanding the reactivity and evolution of volcanic emissions in the atmosphere yet are typically challenging to observe directly at the lava-atmosphere interface due to the nature of volcanic activity. Inferences are instead drawn largely from observations of volcanic plumes as they drift across a crater’s edge and further downwind and the application of thermodynamic models that neglect reaction kinetics as gas and air mix and thermally equilibrate. Here, we foreground chemical kinetics in simulating this critical zone. Volcanic gases are injected into a chain-of-reactors model that simulates time-resolved high-temperature chemistry in the dispersing plume. Boundary conditions of decreasing temperature and increasing proportion of air interacting with volcanic gases are specified with time according to an offline plume dynamics model. In contrast to equilibrium calculations, our chemical kinetics model predicts that CO is only partially oxidised, consistent with observed CO in volcanic plumes downwind from source. Formation of sulfate precursor SO3 at SO3/SO2 = 10-3 mol/mol is consistent with the range of reported sulfate aerosol to SO2 ratios observed close to crater rims. High temperature chemistry also forms oxidants OH, HO2, and H2O2. The H2O2 will likely augment volcanic sulfate yields by reacting with SO2(aq) in the cooled-condensed plume. Calculations show that high-temperature OH will react with volcanic halogen halides (HBr, HCl) to yield reactive halogens (Br, Cl) in the young plume. Strikingly, high-temperature production of radical oxidants (including HOx) is enhanced by volcanic emissions of reduced gases (CO, H2, H2S) due to chemical feedback mechanisms, although the kinetics of some reactions are uncertain, especially regarding sulfur. Our findings argue strongly that the chemistry of the hot near-source plume cannot be captured by equilibrium model assumptions, and highlight the need for development of more sophisticated, kinetics-based, high-temperature CHONS-halogen reaction models.

Keywords: High-Temperature, emission, Oxidants, HO2, OH, H2O2, sulfate, kinetic, Model, plume, eruption, hot, Oxidizing

Received: 06 Oct 2018; Accepted: 03 Jun 2019.

Edited by:

Alessandro Aiuppa, University of Palermo, Italy

Reviewed by:

J. Maarten De Moor, OVSICORI-UNA
Taryn Lopez, University of Alaska Fairbanks, United States  

Copyright: © 2019 Roberts, Dayma and Oppenheimer. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Dr. Tjarda Roberts, UMR7328 Laboratoire de physique et chimie de l'environnement et de l'Espace (LPC2E), Orleans, France,