Abstract

Chlorine dioxide (OClO) is a by-product of the ozone depleting halogen chemistry in the stratosphere. Although being rapidly photolysed at low solar zenith angles (SZAs) it plays an important role as an indicator of the chlorine activation in polar regions during polar winter and spring at twilight conditions because of the nearly linear dependence of its formation to chlorine oxide (ClO). Here we compare slant column densities (SCDs) of chlorine dioxide (OClO) retrieved by means of differential optical absorption spectroscopy (DOAS) from spectra measured by the TROPOspheric Monitoring Instrument (TROPOMI) with meteorological data for both Antarctic and Arctic regions for the first three winters in each of the hemispheres (November 2017–October 2020). TROPOMI, a UV-VIS-NIR-SWIR instrument on board of the Sentinel-5P satellite monitors the Earth’s atmosphere in a near polar orbit at an unprecedented spatial resolution and signal to noise ratio and provides daily global coverage at the equator and thus even more frequent observations at polar regions. The observed OClO SCDs are generally well correlated with the meteorological conditions in the polar winter stratosphere: e.g. the chlorine activation signal appears as a sharp gradient in the time series of the OClO SCDs once the temperature drops to values well below the Nitric Acid Trihydrate (NAT) existence temperature TNAT. Also a relation of enhanced OClO values at lee sides of mountains can be observed at the beginning of the winters indicating a possible effect of occurring lee waves on chlorine activation. The dataset is also compared with CALIPSO Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) polar stratospheric cloud (PSC) observations. In general, OClO SCDs coincide well with CALIOP measurements for which PSCs are detected. Very high OClO levels are observed for the northern hemispheric winter 2019/2020 with an extraordinarly long period with a stable polar vortex being even close to the values found for Southern Hemispheric winters. Also the extraordinary winter in 2019 in the Southern Hemisphere with a minor sudden stratospheric warming at the beginning of September was observed. In this winter similar OClO values were measured in comparison to the previous (usual) winter till that event but with a 1–2 week earlier OClO deactivation.

Highlights

  • It is well established that catalytic halogen chemistry is responsible for stratospheric ozone depletion in polar regions in spring (WMO, 2018)

  • We have found in sensitivity studies that this displacement is expected to be less than 100 km, and typical polar stratospheric clouds (PSCs) concentrations do not largely affect it

  • Mean and maximum PSC evidence calculated for all Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) measurements at latitudes for polar areas of the respective hemispheres above 60◦ is plotted in the bottom panel (x axis), along with the daily maximum OClO slant column densities (SCDs) (y axis)

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Summary

Introduction

It is well established that catalytic halogen chemistry is responsible for stratospheric ozone depletion in polar regions in spring (WMO, 2018). Once the air within the polar vortex cools down below a certain threshold (which varies with altitude), polar stratospheric clouds (PSCs) can form, providing surfaces for the heterogeneous reactions of the chlorine activation (Solomon, 1999). Chlorine starts to deactivate when PSCs evaporate (temperature rises above TNAT) by converting most chlorine into the form of the reservoir species ClONO2, with concentrations higher than before the activation (Müller et al, 1994) This deactivation process takes 1 to 2 weeks depending on the nitrate concentration (Kühl et al, 2004b). We compare OClO SCDs with CALIPSO Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) polar stratospheric cloud (PSC) observations In these comparisons in the first place, the initial period of the potential chlorine activation is of large interest, since we can see even localized activation events.

Relating meteorological parameters with OClO SCDs
CALIOP PSC observations
Winter 2017/18
Winter 2018/19
Winter 2019/20
Winter 2018
Winter 2019
Winter 2020
Conclusions
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