EGU26-3004, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3004
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 14:05–14:15 (CEST)
 
Room M1
Stratospheric aerosol perturbation by tropospheric biomass burning and deep convection
Xiaoli Shen1,11, Justin Jacquot1,12, Yaowei Li2,13, Steven Sharpe3, John Dykema2, Gregory Schill4, Kenneth Bowman5, Cameron Homeyer6, Matthew Fraund7, Ryan Moffet8, Temitope Olayemi3, Jasna Pittman2, Felipe Rivera-Adorno3, Daniel Murphy1,4, Jessica Smith2, Alexander Laskin1,3, Frank Keutsch2,9,10, and Daniel Cziczo1
Xiaoli Shen et al.
  • 1Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, USA
  • 2School of Engineering and Applied Sciences, Harvard University, Cambridge, USA
  • 3Department of Chemistry, Purdue University, West Lafayette, USA
  • 4Chemical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, USA
  • 5Department of Atmospheric Sciences, Texas A&M University, College Station, USA
  • 6School of Meteorology, University of Oklahoma, Norman, USA
  • 7Fraund Consulting, Pleasant Hill, USA.
  • 8Spheros Environmental, Inc., Petaluma, USA
  • 9Department of Chemistry and Chemical Biology, Harvard University, Cambridge, USA
  • 10Department of Earth and Planetary Sciences, Harvard University, Cambridge, USA
  • 11now at: Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany
  • 12now at: Earth Observing Laboratory, Research Aviation Facility, National Center for Atmospheric Research, Boulder, USA
  • 13now at: Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA

The stratosphere is often considered to be dynamically stable with limited vertical exchange; however, episodic deep convection can even transport tropospheric air masses into the upper troposphere (UT) and even across the tropopause into lower stratosphere (LS). We deployed a newly developed airborne single particle mass spectrometer, Particle Analysis by Laser Mass Spectrometry – Next Generation (PALMS-NG), aboard a NASA ER-2 stratospheric aircraft to characterize aerosol particles in the UTLS during the Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) mission. Here, we present observations revealing substantial perturbations of the stratospheric aerosol layer during an active convection and wildfire season in 2022.

We show that carbonaceous–sulfate particles of tropospheric origin account for up to 90% of stratospheric particles with physical diameters between 0.1 and 1.5 µm within an approximately 4 km layer above the tropopause. Approximately 43% of these stratospheric carbonaceous–sulfate particles are directly attributed to biomass burning. The injected particles are chemically complex and organic-rich, and some exhibit internally mixed signatures containing both tropospheric and stratospheric components.

Our observations further demonstrate that biomass-burning-related aerosols do not remain chemically unchanged following injections into the stratosphere. Instead, they undergo chemical mixing with stratospheric components, indicating a pronounced perturbation of the stratospheric aerosol layer driven by convective transport.

These results highlight the coupling between dynamics and chemistry in modulating UTLS aerosol populations. As wildfire frequency and intensity increase alongside enhanced deep convection in a warming climate, convective delivery of biomass-burning products to the stratosphere may become increasingly important, with implications for ozone chemistry and radiative forcing.

How to cite: Shen, X., Jacquot, J., Li, Y., Sharpe, S., Dykema, J., Schill, G., Bowman, K., Homeyer, C., Fraund, M., Moffet, R., Olayemi, T., Pittman, J., Rivera-Adorno, F., Murphy, D., Smith, J., Laskin, A., Keutsch, F., and Cziczo, D.: Stratospheric aerosol perturbation by tropospheric biomass burning and deep convection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3004, https://doi.org/10.5194/egusphere-egu26-3004, 2026.