Articles | Volume 14, issue 8
https://doi.org/10.5194/amt-14-5349-2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/amt-14-5349-2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Measurements of CFC-11, CFC-12, and HCFC-22 total columns in the atmosphere at the St. Petersburg site in 2009–2019
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
Anatoly Poberovsky
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
Maria Makarova
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
Yana Virolainen
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
Yuri Timofeyev
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
Anastasiia Nikulina
Department of Atmospheric Physics, St. Petersburg State University, 7–9 Universitetskaya Emb., St. Petersburg 199034, Russia
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Short summary
The photolysis of CFCs, and to a lesser extent of HCFCs, in the stratosphere leads to the appearance of so-called ozone holes. We improve the retrieval strategies for deriving CFC-11, CFC-12, and HCFC-22 from ground–based IR solar radiation spectra measured by a Bruker FS125HR spectrometer, analyze the time series at the Network for the Detection of Atmospheric Composition Change (NDACC) site in St. Petersburg, Russia, and compare them to the independent data.
The photolysis of CFCs, and to a lesser extent of HCFCs, in the stratosphere leads to the...