EGU21-4203
https://doi.org/10.5194/egusphere-egu21-4203
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Detection of Fourth Generation Synthetic Halocarbons in the Upper Troposphere

Tanja Schuck1, Katharina Meixner1, Peter van Velthoven2, Simon O’Doherty3, Martin Vollmer4, Andreas Engel1, and Andreas Zahn5
Tanja Schuck et al.
  • 1Goethe University Frankfurt, Institute for Atmospheric and Environmental Sciences, Geosciences, Frankfurt a. Main, Germany (schuck@iau.uni-frankfurt.de)
  • 2Royal Netherlands Meteorological Institute (KNMI), De Bilt, The Netherlands
  • 3School of Chemistry, University of Bristol, Bristol, United Kingdom
  • 4Empa - Materials Science & Technology, Dübendorf, Switzerland
  • 5Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany

Synthetic halocarbons are used for a wide range of applications, for example air conditioning or foam blowing. Many of them are long-lived greenhouse gases contributing to climate change and, in addition, may contribute to stratospheric ozone depletion if containing chlorine or bromine. Therefore, their production and use are regulated by the Montreal Protocol and its amendments. These long-lived halocarbons are increasingly replaced by a fourth generation of unsaturated short-lived halocarbons, the hydrochlorofluoroolefines (HCFOs) and hydrofluoroolefines (HFOs). The main removal process of these compounds in the atmosphere is reaction with OH radicals, and their average lifetimes are of the order of up to a few tens of days.

As part of the IAGOS-CARIBIC instrument package we operate an automated air sample collection system during regular flights in the upper troposphere and lowermost stratosphere. At altitudes around 10-12 km, samples are collected in stainless steel and glass flasks at predefined times. Post-flight laboratory analyses include gas chromatography - mass spectrometry measurements of a wide range of halocarbons. The short-lived compounds HFO-1234ze(E) and HCFO-1233zd(E) were detected in a small number of samples, indicating that these compounds are sufficiently long lived for transport into the upper troposphere. There were not found in stratospheric samples.

At this altitude, low abundance of OH and low temperatures may slow down chemical decay, and tracer lifetimes may increase significantly. Based on average temperatures and OH abundance, we estimate local lifetimes of HFO-1234ze(E) and HCFO-1233zd(E)  in the mid-latitudes of up to 75 days and 200 days, respectively. Short-lived H(C)FOs reaching the upper troposphere could thus be transported over large distances and their degradation products may be deposited  far from their emission sources.

How to cite: Schuck, T., Meixner, K., van Velthoven, P., O’Doherty, S., Vollmer, M., Engel, A., and Zahn, A.: Detection of Fourth Generation Synthetic Halocarbons in the Upper Troposphere, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-4203, https://doi.org/10.5194/egusphere-egu21-4203, 2021.

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