EGU24-14103, updated on 05 Apr 2024
https://doi.org/10.5194/egusphere-egu24-14103
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Detection of iodine over the continental United States: Implications for ozone and mercury oxidation

Christopher Lee1,2, Tyler Elgiar3, Liji David4, Kai Wilmot5, Margarita Reza1,2, Noah Hirshorn5, Ian McCubbin5, Seth Lyman3, Gannet Hallar5, Lynne Gratz6, and Rainer Volkamer1,2
Christopher Lee et al.
  • 1Department of Chemistry, University of Colorado Boulder, Boulder, CO, United States of America
  • 2Cooperative Institute for Research in Environmental Sciences, Boulder, CO, United States of America
  • 3Department of Chemistry and Biochemistry, Utah State University, Logan, UT, United States of America
  • 4Bingham Research Center, Utah State University, Vernal, UT, United States of America
  • 5Department of Atmospheric Sciences, University of Utah, Salt Lake City, UT, United States of America
  • 6Department of Chemistry, Reed College, Portland, OR, United States of America

Most of our knowledge about the global distribution of atmospheric iodine is based on measurements of iodine monoxide (IO) radicals in the marine boundary layer and at high latitudes. Recent evidence of IO in the free troposphere is limited to few available aircraft measurements over oceans. We report the first ground-based Multi-AXis Differential Optical Absorption Spectroscopy (MAX-DOAS) observations of tropospheric IO radicals over the central continental United States. IO vertical columns measured at Storm Peak Laboratory, CO (40.455°N, 106.744°W, 3220 m.a.s.l.) are similar to those over oceans and vary significantly. A priori sensitivity studies indicate that IO mixing ratios increase with altitude. Back trajectory modeling indicates that IO is consistently observed in air masses quickly transported from over the Pacific Ocean. We compare the IO columns and their variability with predictions by a global model and use the observations to constrain a chemical box model to assess the atmospheric implications for ozone and mercury oxidation. Iodine-induced mercury oxidation is currently missing in atmospheric models, understudied, and helps to partially explain the elevated concentrations of oxidized mercury measured at SPL.

How to cite: Lee, C., Elgiar, T., David, L., Wilmot, K., Reza, M., Hirshorn, N., McCubbin, I., Lyman, S., Hallar, G., Gratz, L., and Volkamer, R.: Detection of iodine over the continental United States: Implications for ozone and mercury oxidation, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-14103, https://doi.org/10.5194/egusphere-egu24-14103, 2024.