EGU2020-5186
https://doi.org/10.5194/egusphere-egu2020-5186
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Total columns of freons retrieved from ground-based IR solar spectra measurements near Saint Petersburg, Russia

Alexander Polyakov, Maria Makarova, Yana Virolainen, Anatoly Poberovsky, and Yury Timofeyev
Alexander Polyakov et al.
  • Saint Petersburg State University, the Physics of Atmosphere, Saint Petersburg, Russian Federation (a.v.polyakov@spbu.ru)

Measurements of the atmospheric total columns (TCs) of trichlorofluoromethane CCl3F (CFC-11), dichlorodifluoromethane CCl2F2 (CFC-12), and chlorodifluoromethane CHClF2 (HCFC-22)  at the NDACC station St. Petersburg are considered. These gases are the most common representatives of a group of aliphatic organic compounds often called by the DuPont brandname "Freons". Since the 30-ies of the last century, they have been used in industrial applications as refrigerants and propellants. Due to their destructive effect on the ozone layer the production of CFC-11 and CFC-12 has been phased out under the Montreal Protocol entered into force in 1989, which led to the beginning of a decrease in their content. Nevertheless, they are still one of the major anthropogenic sources of active chlorine that destroys ozone in the stratosphere. HCFC-22 became a replacement for the most dangerous for ozone layer freons, but later it was also recognized as a dangerous compound for stratospheric ozone. Nowadays, the production and consumption of HCFC-22 are reduced and it is planned to be completely phased out. Therefore, the monitoring the content of freons in the atmosphere is very important.

Although the content of freons is measured by satellite methods and the sampling method, only the ground-based IR method based on the measurement of IR solar radiation allows obtaining TCs of freons.

A technique for ground-based measurements of the TCs of CFC-11, CFC-12, and HCFH-22 has been developed. The technique is based on the ground-based measurements of solar IR spectra by IFS125HR instrument. For the processing of spectra, the SFIT4 software is used. The analyzed spectral windows are: 1160 – 1162 cm-1 for CFC-12, 828.75 – 829.4cm-1 for HCFC-22, and  830 – 860 cm-1 for CFC-11. Due to the wide spectral interval for CFC-11 retrieval, the preliminary measured spectral transmission function of the instrument filter, the water vapor continuum, and the absorption of radiation by an ice on the MCT detector are taken into account as well. Systematic and random errors of TCs retrieval are estimated as 7.4% and 2.9% for the CFC-11 TCs, 5.0% and 3.7% for the CFC-12 TCs, and 2.0% and 2.7% for the HCFH -22 TCs.

Estimates of TCs above Saint Petersburg have been obtained using the developed technique for the period of 2009 – 2019. The variability during  a day is of 0.8, 0.9, and 3.7 %, the total variabilitiey for 2009 – 2019 is of 3.7, 2.4 and 5.6%, for CFC-11, CFC-12 and HCFC-22, respectively. Trend estimates of CFC-11, CFC-12 and HCFC-22 for 2009 –2019 are –0.31±0.07%, –0.45 ± 0.06% and +2.2 ± 0.14%, respectively, which  are consistent with data from other authors.

In recent years, a tendency toward a decrease of HCFC-22 TCs in the atmosphere above St. Petersburg has been observed, that can be associated with the restriction of HCFC-22 production and use.

Acknowledgements

Measurements of solar radiation were performed with the equipment of the resource center "Geomodel". The investigation was supported by grant 18-05-00426 of the Russian Foundation for Basic Research.

How to cite: Polyakov, A., Makarova, M., Virolainen, Y., Poberovsky, A., and Timofeyev, Y.: Total columns of freons retrieved from ground-based IR solar spectra measurements near Saint Petersburg, Russia, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-5186, https://doi.org/10.5194/egusphere-egu2020-5186, 2020

Display materials

Display file

Comments on the display material

AC: Author Comment | CC: Community Comment | Report abuse

Display material version 2 – uploaded on 04 May 2020, no comments
small correction
Display material version 1 – uploaded on 01 May 2020, no comments