EGU25-9344, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-9344
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
PICO | Wednesday, 30 Apr, 16:32–16:34 (CEST)
 
PICO spot 5, PICO5.7
Enhanced inorganic iodine in the upper troposphere potentially driven by elevated emission and/or fast vertical transport by tropical cyclone
Karolin Voss1, Benjamin Weyland1, André Butz1,2,3, Valentin Lauther4, C.Michael Volk4, Bärbel Vogel5, Andreas Engel6, Tanja Schuck6, Timo Keber6, Meike Rotermund1,7, and Klaus Pfeilsticker1
Karolin Voss et al.
  • 1Institute of Environmental Physics, Heidelberg University, Heidelberg, Germany (karolin.voss@uni-heidelberg.de)
  • 2Heidelberg Center for the Environment, Heidelberg University, Heidelberg, Germany
  • 3Interdisciplinary Center for Scientific Computing, Heidelberg University, Heidelberg, Germany
  • 4Institute for Atmospheric and Environmental Research, University of Wuppertal, Wuppertal, Germany
  • 5Institute of Energy and Climate Research – Stratosphere (IEK-7), Forschungszentrum Jülich, Jülich, Germany
  • 6Institute for Atmospheric and Environmental Science, Goethe University Frankfurt, Frankfurt, Germany
  • 7now at: Department of Physics, University of Toronto, Toronto, Canada

Halogens are known to deplete ozone both in the troposphere and stratosphere. As the source distribution and thus the local contribution of chlorine and bromine containing species to atmospheric ozone depletion is reasonably well known, the respective role of iodine containing species is subject of current research. In contrast to the major sources of chlorine in the stratosphere which derive from man-made chlorinated hydrocarbons, about half of stratospheric bromine stems from bromocarbons of natural origin while iodine predominantly originates from inorganic species (I2, and HOI) emitted from the oceans. It has been indicated previously that tropical cyclones emit elevated amounts of brominated species (e.g. CHBr3 and CH2Br2) which are efficiently transported into the extratropical upper troposphere and eventually into the lower stratosphere. Here we provide evidence that also significant amounts of inorganic iodine emitted from the ocean surface and/or through sea-spray are transported to the extratropical upper troposphere through tropical cyclone driven fast vertical transport.

Our finding is based on the simultaneous detection of elevated amounts of brominated very short-lived substances (VSLS) and iodine oxide (IO, ~0.3 pptv) while simultaneously relatively low mixing ratios of the anthropogenically emitted CH2Cl2 were measured in the upper troposphere (~13 km, θ~360 K) of the mid-Atlantic on October 1st,2017. CLaMS back-trajectory calculations driven by ECMWF ERA-Interim reanalysis suggest that these iodine-rich air masses originate from marine surface air masses being uplifted by the category 5 hurricane Maria.

The measurements were performed from aboard HALO (High Altitude and LOng range Aircraft) during the WISE (Wave-driven ISentropic Exchange) campaign over the mid-Atlantic in September and October 2017. IO was detected in limb scattered skylight using the miniDOAS instrument, while the organic chlorinated and brominated species were detected by the HAGAR-V and GhOST GC/MS instruments.

Our findings suggest that tropical storms lead to elevated emissions of inorganic iodine rapidly transported from the tropical marine boundary layer into the upper troposphere. This mechanism implies a potentially significant role of iodine in ozone destruction in the remnant air of tropical storms and a possible pathway for iodine to enter the lower stratosphere in significant amounts.

How to cite: Voss, K., Weyland, B., Butz, A., Lauther, V., Volk, C. M., Vogel, B., Engel, A., Schuck, T., Keber, T., Rotermund, M., and Pfeilsticker, K.: Enhanced inorganic iodine in the upper troposphere potentially driven by elevated emission and/or fast vertical transport by tropical cyclone, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9344, https://doi.org/10.5194/egusphere-egu25-9344, 2025.