Optimizing cloud motion estimation and detection of raindrop contamination in ARM cameras

 

Submitter

Collis, Scott Matthew — Argonne National Laboratory

Area of research

Cloud Distributions/Characterizations

Journal Reference

Raut B, P Muradyan, R Sankaran, R Jackson, S Park, S Shahkarami, D Dematties, Y Kim, J Swantek, N Conrad, W Gerlach, S Shemyakin, P Beckman, N Ferrier, and S Collis. 2023. "Optimizing cloud motion estimation on the edge with phase correlation and optical flow." Atmospheric Measurement Techniques, 16(5), 10.5194/amt-16-1195-2023.

Science

This study investigated the factors affecting cloud motion estimations from camera images using different settings of the phase correlation (PC) and optical flow (OF) methods, concluding that shorter frame intervals provides the most accurate results while image resolution has small effect. The OF algorithm is more stable than PC for the fast-moving targets.

Impact

Improved cloud motion estimation and image sampling has the potential to significantly enhance the local prediction of solar irradiance. In addition, a sky-viewing camera is being tested to identify and track clouds for real-time optimization of mini micropulse lidar (MiniMPL) scan strategies to increase the density of scans for targeted clouds.

Summary

This study used the phase correlation and optical flow methods to estimate cloud motion vectors (CMV) from sky camera images. The study investigated the stability of the method by altering block size, frame interval, and RGB channels, using data from the United States Atmospheric Radiation Measurement user facility's Southern Great Plains observatory. The investigators found that shorter frame intervals and larger block sizes lead to stable CMV estimates and that the choice of RGB channels and resolution has a limited effect. The study's results are critical for optimizing algorithms for edge-computing sensor systems and have the potential to improve cloud identification and local solar irradiance prediction. They also detected raindrop-contaminated images using the rotation of the total sky imager (TSI) mirror in the motion field.