EGU26-18282, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-18282
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Wednesday, 06 May, 15:25–15:35 (CEST)
 
Room 1.61/62
Custom High-Resolution UV Laser Systems for new Accurate Ozone Absorption Cross Section measurements in the Huggins bands
Coline Mahob1,2, Gérard Ancellet3, Ariane Bazureau3, Marie-Renée Debacker4, Hadj Elandaloussi1, Sophie Godin-beekmann3, Ruizhe Gu5, Adèle Hilico6, Pascal Jeseck1, Patrick Marie-jeanne1, Andrea Pazmiño3, Christian Rouille1, Giorgio Santarelli5, Thomas Zanon1, and Christof Janssen1
Coline Mahob et al.
  • 1Sorbonne Université, CNRS, MONARIS, Paris, France
  • 2Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LUX, Paris, France
  • 3LATMOS/IPSL, UVSQ, Sorbonne Université, CNRS, Guyancourt, France
  • 4GSMA, CNRS, University of Champagne and Ardenne, Reims, France
  • 5LP2N, IOGS, CNRS, Université de Bordeaux, Talence, France
  • 6LPL, Université Sorbonne Paris Nord, CNRS, Villetaneuse, France

Accurate and traceable observation of atmospheric ozone is a fundamental requirement for reliable analyses of climate evolution, air quality, and ultraviolet radiation exposure, as ozone simultaneously limits biologically harmful UV radiation and contributes to radiative forcing. Detecting and interpreting long-term ozone variability and trends requires spectroscopic inputs with high accuracy. However, ozone absorption cross sections in the UV Huggins bands (310–360 nm), used by ground-based lidars, Brewer and Dobson spectrometers, and UV-visible satellite instruments, remain a major source of uncertainty. It has been established that recommended and widely used datasets in this spectral region exhibit uncertainties exceeding 1 % at room temperature and rising above 3 % at low stratospheric temperatures. These inconsistencies introduce systematic biases when measurements from multiple platforms are combined. To address this limitation, a dedicated laser-based experimental approach was developed to determine ozone absorption cross sections with high spectral resolution and accurate frequency control across a significant part of the Huggins bands. Because continuous-wave UV laser sources are not commercially available in this wavelength range, ultraviolet radiation was produced through frequency doubling of tunable visible lasers derived from fiber-based infrared systems. These lasers were specifically designed and built for this experiment, providing narrow linewidths, stable tuning, and performance tailored to high-precision ozone spectroscopy. Two complementary laser systems were implemented: one operating between 307.8 and 308.2 nm, targeting wavelengths relevant for stratospheric lidar applications, and a second system covering 308–318 nm to match the spectral requirements of Brewer and Dobson spectrometers as well as satellite instruments. The experimental setup includes a purpose-built absorption cell that allows measurements over a controlled temperature range from −80 °C to +30 °C, thereby reproducing atmospheric conditions encountered from the ground to the lower stratosphere. Ozone used in the experiments is generated on site and has a purity of 99.8 %. In connection with simultaneous ozone measurements at 254 nm, this ensures traceability to the photometric ozone standard and minimizes contamination effects. The use of custom high-resolution laser sources and a temperature-controlled measurement cell significantly reduces biases associated with conventional broadband UV spectroscopy. The developed methodology provides a robust framework for improving existing ozone absorption datasets and for harmonizing measurements across different observing platforms.

How to cite: Mahob, C., Ancellet, G., Bazureau, A., Debacker, M.-R., Elandaloussi, H., Godin-beekmann, S., Gu, R., Hilico, A., Jeseck, P., Marie-jeanne, P., Pazmiño, A., Rouille, C., Santarelli, G., Zanon, T., and Janssen, C.: Custom High-Resolution UV Laser Systems for new Accurate Ozone Absorption Cross Section measurements in the Huggins bands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18282, https://doi.org/10.5194/egusphere-egu26-18282, 2026.