EGU2020-18036
https://doi.org/10.5194/egusphere-egu2020-18036
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Camera Observation and Modelling of 4D Tracer Dispersion in the Atmosphere

Kerstin Stebel1, Massimo Cassiani1, Hamidreza Ardeshiri1, Cirilo Bernardo2, Anna Solvejg Dinger1,3, Arve Kylling1, Soon-Young Park4, Ignacio Pisso1, Norbert Schmidbauer1, and Andreas Stohl1,5
Kerstin Stebel et al.
  • 1NILU - Norwegian Institute for Air Research, Kjeller, Norway (kst@nilu.no)
  • 2Aires Pty. Ltd., Mount Eliza, Australia
  • 3Institute of Environmental Physics, University of Heidelberg, Heidelberg, Germany
  • 4Center for Earth and Environmental Modeling Studies, Gwangju Institute of Science and Technology, Gwangju, Republic of Korea
  • 5Institute for Meteorology and Geophysics, University of Vienna, Austria

In the frame of the COMTESSA (Camera Observation and Modelling of 4D Tracer Dispersion in the Atmosphere) project, tracer dispersion release experiments were performed during three field campaigns in Norway in July 2017, 2018, and 2019.  The main goal of the project is to improve our understanding of turbulence and plume dispersion on local scale in the planetary boundary layer by bringing together full four-dimensional (space and time) observations of a (nearly) passive tracer (sulfur dioxide, SO2), with advanced data analysis and turbulence and dispersion modelling. By means of tomographic reconstruction of the 3D tracer concentration distribution, not only the mean but also higher moments of the probability density function of the tracer concentration field can be revealed. In 2017 first field tests were made, releasing SO2 in continuous plumes and puffs from a 10 m tower, while in the following years SO2 was released from a 60 m tower, located in the centre of a fenced-in 900 m x 400 m wide flat gravel field. The masts were equipped with eddy covariance measurement systems to continuously record turbulent fluxes of heat and momentum during the field campaigns. Up to six ultraviolet (UV) and in 2019 also three infrared (IR) SO2 cameras, were placed in a ring around the SO2 release tower at varying distances up to ~1.2 km to simultaneously image the movement and spread of the 2d integrated SO2 tracer column densities.

Here we present an overview of the field experiments and lessons learned, with focus on results from the 2019 summer campaign. It was a challenge to find a location where hazardous gas could be released and a main obstacle for the imaging-based experiment were the unfavourable weather conditions. Despite these challenges, progress was made throughout the years. During consecutive summers the release equipment was improved and optimized and in 2019 puff releases were made by filling balloons with SO2 and exploding them. The cameras were continuously developed, the setup of the cameras at the site was adjusted to allow observations for longer timescales.  During July 11-28, 2019 ~130 puffs were released from balloons holding between 250 g and 325 g SO2. Those are used to give an overview of the image/data processing and type of results that can be obtained from our observations, e.g. relative dispersion and meandering, Eulerian and Lagrangian integral time scales and their relation, tomographic reconstruction. The focus lies on the plume spread, i.e. relative dispersion processes we recorded under different stability conditions in July 2019.

How to cite: Stebel, K., Cassiani, M., Ardeshiri, H., Bernardo, C., Dinger, A. S., Kylling, A., Park, S.-Y., Pisso, I., Schmidbauer, N., and Stohl, A.: Camera Observation and Modelling of 4D Tracer Dispersion in the Atmosphere, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-18036, https://doi.org/10.5194/egusphere-egu2020-18036, 2020