Preprints
https://doi.org/10.5194/egusphere-2025-3158
https://doi.org/10.5194/egusphere-2025-3158
22 Aug 2025
 | 22 Aug 2025
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Influence of secondary ice formation on tropical deep convective clouds simulated by the Unified Model

Mengyu Sun, Paul J. Connolly, Paul R. Field, Declan L. Finney, and Alan M. Blyth

Abstract. Secondary ice production (SIP) plays an important role in tropical deep convection, yet its representation in models remains uncertain. This study incorporates multiple SIP mechanisms, including droplet fragmentation (Mode 1 and Mode 2) and ice–ice collisional breakup, into the CASIM microphysics scheme of the UK Met Office Unified Model, and evaluates their impacts through a real-case simulation of a Hector thunderstorm. SIP enhances ice number concentration in upper cloud layers, with values up to 3 orders of magnitude higher than the no-SIP case, particularly above −10 °C. Ice water content (IWC) increases by a factor of 3–5 in the anvil region, contributing to more extensive upper-level cloud coverage. These microphysical changes reduce outgoing longwave radiation (OLR) by ~3.2 W m2 (1.3 %) and increase outgoing shortwave radiation (OSR) by ~4.5 W m2 (1.8 %) over a 6-hour analysis period and a 110 km × 110 km domain. SIP modifies precipitation structure, enhancing local rainfall near the convective core while reducing domain-averaged precipitation by ~8 %. Peak rainfall rates remain only slightly affected, consistent with the minor changes (<1 m s1) in maximum updraft velocity. Among the tested mechanisms, ice–ice collisional breakup shows negligible impact under warm, graupel-sparse tropical conditions. Ensemble experiments confirm that these effects are robust and exceed the influence of meteorological variability. These results highlight the importance of representing SIP processes in cloud-resolving models of tropical convection and accounting for their environmental dependence.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
Share
Mengyu Sun, Paul J. Connolly, Paul R. Field, Declan L. Finney, and Alan M. Blyth

Status: open (until 03 Oct 2025)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-3158', Anonymous Referee #1, 08 Sep 2025 reply
  • RC2: 'Comment on egusphere-2025-3158', Anonymous Referee #2, 10 Sep 2025 reply
  • RC3: 'Comment on egusphere-2025-3158', Pierre Grzegorczyk, 12 Sep 2025 reply
Mengyu Sun, Paul J. Connolly, Paul R. Field, Declan L. Finney, and Alan M. Blyth
Mengyu Sun, Paul J. Connolly, Paul R. Field, Declan L. Finney, and Alan M. Blyth

Viewed

Total article views: 1,619 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,590 23 6 1,619 14 19
  • HTML: 1,590
  • PDF: 23
  • XML: 6
  • Total: 1,619
  • BibTeX: 14
  • EndNote: 19
Views and downloads (calculated since 22 Aug 2025)
Cumulative views and downloads (calculated since 22 Aug 2025)

Viewed (geographical distribution)

Total article views: 1,617 (including HTML, PDF, and XML) Thereof 1,617 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 12 Sep 2025
Download
Short summary
We investigated how extra ice particles form inside tropical storm clouds and how they affect rainfall and sunlight reflection. By using a weather model, we found that these extra ice particles can change how clouds grow, reduce heat escaping to space, and slightly shift where rain falls. This helps improve how weather and climate models predict tropical storms.
Share