EGU23-11662, updated on 19 Apr 2024
https://doi.org/10.5194/egusphere-egu23-11662
EGU General Assembly 2023
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

High spatial resolution retrieval of cloud droplet size distribution from polarimetric specMACS observations and application to simulated data

Veronika Pörtge1, Tobias Kölling2, Anna Weber1, Lea Volkmer1, Claudia Emde1, Tobias Zinner1, Linda Forster3, and Bernhard Mayer1
Veronika Pörtge et al.
  • 1Ludwig-Maximilians University, Meteorological Institute, Experimental Meteorology, Munich, Germany
  • 2Max Planck Institute for Meteorology, Hamburg, Germany
  • 3Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California

We present novel remote sensing observations of cloud droplet size distributions retrieved from polarimetric observations of the wide-field airborne imaging system specMACS. The measurements were collected during the EUREC4A field campaign which took place in January and February 2020 in the trade wind region east of Barbados. We focus on observations of the cloudbow which is an optical phenomenon that results from single scattering of sunlight by liquid droplets close to the cloud top. The cloudbow signal strongly depends on the cloud droplet size distribution. By fitting model simulations (stored in a look-up table) to the cloudbow observations, both the effective radius and the effective variance (i.e., the width) of the droplet size distribution are retrieved. Traditional retrieval techniques based on total reflectance measurements are able to determine the effective radius but do not provide information on the effective variance. However, to fully understand cloud growth processes and the interaction between clouds and solar radiation, both parameters must be known. Furthermore, the cloudbow is only weakly affected by 3-D radiative transfer effects which is beneficial since these are usually a problem for traditional methods.

High-resolution maps of the cloud droplet size distribution with a spatial resolution of 100 m by 100 m are presented. The maps reveal patterns within the cloud droplet size distribution at cloud top that could originate from mechanisms like entrainment or mixing processes. We further show first results of an application of the retrieval to simulated specMACS observations. The images were generated using the 3-D radiative transfer model MYSTIC and are based on realistic LES cloud field simulations. We will investigate limitations and uncertainties of the retrieval using the simulated dataset.

How to cite: Pörtge, V., Kölling, T., Weber, A., Volkmer, L., Emde, C., Zinner, T., Forster, L., and Mayer, B.: High spatial resolution retrieval of cloud droplet size distribution from polarimetric specMACS observations and application to simulated data, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-11662, https://doi.org/10.5194/egusphere-egu23-11662, 2023.

Supplementary materials

Supplementary material file