Warm-phase microphysical evolution in  large-eddy simulations of tropical cumulus  congestus: evaluating drop size distribution  evolution using polarimetry retrievals, in situ measurements, and a thermal-based framework

Stanford, McKenna W.; Fridlind, Ann M.; Ackerman, Andrew S.; van Diedenhoven, Bastiaan; Xiao, Qian; Wang, Jian; Matsui, Toshihisa; Hernandez-Deckers, Daniel; Lawson, Paul

doi:https://doi.org/10.5194/acp-25-11199-2025

Articles | Volume 25, issue 18

https://doi.org/10.5194/acp-25-11199-2025

© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.

Special issue:

Cloud, Aerosol and Monsoon Processes Philippines Experiment...

https://doi.org/10.5194/acp-25-11199-2025

© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 25, issue 18

Research article

|

25 Sep 2025

Research article |

| 25 Sep 2025

Warm-phase microphysical evolution in large-eddy simulations of tropical cumulus congestus: evaluating drop size distribution evolution using polarimetry retrievals, in situ measurements, and a thermal-based framework

McKenna W. Stanford, Ann M. Fridlind, Andrew S. Ackerman, Bastiaan van Diedenhoven, Qian Xiao, Jian Wang, Toshihisa Matsui, Daniel Hernandez-Deckers, and Paul Lawson

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Dec 2024	35	7	6	48
Jan 2025	47	10	5	62
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Cumulative views and downloads (calculated since 05 Aug 2024)

Month	HTML	PDF	XML	Total
Aug 2024	154	45	57	256
Sep 2024	88	20	23	131
Oct 2024	69	5	30	104
Nov 2024	37	7	47	91
Dec 2024	35	7	6	48
Jan 2025	47	10	5	62
Feb 2025	36	4	2	42
Mar 2025	28	5	0	33
Apr 2025	39	7	1	47
May 2025	33	6	2	41
Jun 2025	41	3	1	45
Jul 2025	46	5	1	52
Aug 2025	127	6	3	136
Sep 2025	662	10	3	675

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Short summary

The evolution of cloud droplets, from the point they are activated by atmospheric aerosol to the formation of precipitation, is an important process relevant to understanding cloud–climate feedbacks. This study demonstrates a benchmark framework for using novel airborne measurements and retrievals to constrain high-resolution simulations of moderately deep cumulus clouds and pathways for scaling results to large-scale models and space-based observational platforms.


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