Articles | Volume 16, issue 5
https://doi.org/10.5194/amt-16-1195-2023
https://doi.org/10.5194/amt-16-1195-2023
Research article
 | 
08 Mar 2023
Research article |  | 08 Mar 2023

Optimizing cloud motion estimation on the edge with phase correlation and optical flow

Bhupendra A. Raut, Paytsar Muradyan, Rajesh Sankaran, Robert C. Jackson, Seongha Park, Sean A. Shahkarami, Dario Dematties, Yongho Kim, Joseph Swantek, Neal Conrad, Wolfgang Gerlach, Sergey Shemyakin, Pete Beckman, Nicola J. Ferrier, and Scott M. Collis

Viewed

Total article views: 4,455 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,532 1,871 52 4,455 37 28
  • HTML: 2,532
  • PDF: 1,871
  • XML: 52
  • Total: 4,455
  • BibTeX: 37
  • EndNote: 28
Views and downloads (calculated since 10 Jun 2022)
Cumulative views and downloads (calculated since 10 Jun 2022)

Viewed (geographical distribution)

Total article views: 4,455 (including HTML, PDF, and XML) Thereof 4,751 with geography defined and -296 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 25 Apr 2024
Download
Short summary
We studied the stability of a blockwise phase correlation (PC) method to estimate cloud motion using a total sky imager (TSI). Shorter frame intervals and larger block sizes improve stability, while image resolution and color channels have minor effects. Raindrop contamination can be identified by the rotational motion of the TSI mirror. The correlations of cloud motion vectors (CMVs) from the PC method with wind data vary from 0.38 to 0.59. Optical flow vectors are more stable than PC vectors.