Articles | Volume 17, issue 21
https://doi.org/10.5194/acp-17-13317-2017
https://doi.org/10.5194/acp-17-13317-2017
Research article
 | 
09 Nov 2017
Research article |  | 09 Nov 2017

The role of 1-D and 3-D radiative heating in the organization of shallow cumulus convection and the formation of cloud streets

Fabian Jakub and Bernhard Mayer

Viewed

Total article views: 4,399 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,851 1,382 166 4,399 177 198
  • HTML: 2,851
  • PDF: 1,382
  • XML: 166
  • Total: 4,399
  • BibTeX: 177
  • EndNote: 198
Views and downloads (calculated since 08 May 2017)
Cumulative views and downloads (calculated since 08 May 2017)

Viewed (geographical distribution)

Total article views: 4,399 (including HTML, PDF, and XML) Thereof 4,374 with geography defined and 25 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Saved (final revised paper)

Latest update: 17 Jun 2026
Download
Short summary
The formation of shallow cumulus cloud streets was historically attributed primarily to dynamics. Here, we focus on the interaction between radiatively induced surface heterogeneities and the resulting patterns in the flow. Our results suggest that solar radiative heating has the potential to organize clouds perpendicular to the sun's incidence angle.
Share
Altmetrics
Final-revised paper
Preprint