EGU2020-11831
https://doi.org/10.5194/egusphere-egu2020-11831
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

OClO as observed by TROPOMI on Sentinel 5P

Janis Pukite, Christian Borger, Steffen Dörner, and Thomas Wagner
Janis Pukite et al.
  • Max Plank Institute for Chemistry, Satellite Remote Sensing, Mainz, Germany (janis.pukite@mpic.de)

The TROPOspheric Monitoring Instrument (TROPOMI) is an UV-VIS-NIR-SWIR instrument on board of Sentinel-5P satellite developed for monitoring the Earth’s atmosphere. It was launched on 13 October 2017 in a near polar orbit. It measures spectrally resolved earthshine radiances at an unprecedented spatial resolution of around 3.5x7.2 km2 (3.5x5.6 km2 starting from 6 Aug 2019) (near nadir) with a total swath width of ~2600 km on the Earth's surface providing daily global coverage. From the measured spectra high resolved trace gas distributions can be retrieved by means of differential optical absorption spectroscopy (DOAS).

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 relation of its formation to chlorine oxide (ClO).

Here we present a new DOAS retrieval algorithm of the slant column densities (SCDs) of chlorine dioxide (OClO) and correlate this TROPOMI OClO signal with meteorological data for both Antarctic and Arctic regions.

How to cite: Pukite, J., Borger, C., Dörner, S., and Wagner, T.: OClO as observed by TROPOMI on Sentinel 5P, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-11831, https://doi.org/10.5194/egusphere-egu2020-11831, 2020