The role of hydrogen sulfide in a Permian-Triassic boundary ozone collapse

Using a three-dimensional chemistry-climate model of the troposphere and stratosphere, we find that hydrogen sulfide alone is unlikely to directly affect stratospheric ozone, even for hydrogen sulfide emission rates as large as 5000 Tg(S) per year. However, we also find that large quantities of hydrogen sulfide create a significant decrease in tropospheric hydroxyl radical, leading to a commensurate increase in atmospheric methane. Therefore a large methane flux (possibly from methane clathrate destabilization, Siberian traps or hydrothermal vent complexes) combined with a large hydrogen sulfide oceanic flux is much more likely to lead to an ozone collapse than methane or hydrogen sulfide alone with implications to the Permian-Triassic boundary extinction 250 million years ago.

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Copyright 2007 American Geophysical Union.


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Author Lamarque, Jean-Francois
Kiehl, Jeffrey
Orlando, John
Publisher UCAR/NCAR - Library
Publication Date 2007-01-16T00:00:00
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Topic Category geoscientificInformation
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Metadata Date 2023-08-18T18:38:54.468560
Metadata Record Identifier edu.ucar.opensky::articles:6949
Metadata Language eng; USA
Suggested Citation Lamarque, Jean-Francois, Kiehl, Jeffrey, Orlando, John. (2007). The role of hydrogen sulfide in a Permian-Triassic boundary ozone collapse. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d7hx1czk. Accessed 21 July 2025.

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