Preprints
https://doi.org/10.5194/egusphere-2024-2396
https://doi.org/10.5194/egusphere-2024-2396
20 Aug 2024
 | 20 Aug 2024

Mechanisms of surface solar irradiance variability under broken clouds

Wouter Mol and Chiel van Heerwaarden

Abstract. Surface solar irradiance variability is present under all broken clouds, but the patterns, magnitude of variability, and mechanisms behind it vary greatly with cloud type. In this study, we performed numerical experiments to understand which main mechanisms drive surface solar irradiance extremes across a diverse set of cloud conditions based on observations. The results show that we can capture the essence in four mechanisms. We find that for optically thin (τ < 6) and clouds, scattering in the forward direction (forward escape) is the dominant mechanism. In cloud types such as altocumulus, it is able to produce irradiance enhancements of up to 50 % of clear-sky values due to small gaps in the cloud field. For flat, optically thick clouds (τ > 6) like stratus, downward escape becomes the dominant mechanism, and the irradiance extremes are found underneath the cloud edge or gaps. Albedo has a significant effect under optically thick cloud cover, contributing 10 to 60 % of the total irradiance enhancement for low (0.2) to high (0.8) albedo. For deep convective clouds, side escape is the dominant mechanism enhancing domain-averaged diffuse irradiance. This effect has a large area of influence, extending over 20 km from the sunlit side of the cloud. Extreme irradiance enhancement, however, comes from downward escape and forward escape just underneath the cloud edge on the sunlit side, not from side escape. These results provide a framework for understanding the vast diversity and complexity found in surface solar irradiance and cloudiness. A next step is to apply this analysis to multi-layered cloud fields and non-isolated deep convective clouds.

Competing interests: The contact author has declared that neither of the authors has any competing interests.

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 preprint. The responsibility to include appropriate place names lies with the authors.
Share

Journal article(s) based on this preprint

23 Apr 2025
Mechanisms of surface solar irradiance variability under broken clouds
Wouter Mol and Chiel van Heerwaarden
Atmos. Chem. Phys., 25, 4419–4441, https://doi.org/10.5194/acp-25-4419-2025,https://doi.org/10.5194/acp-25-4419-2025, 2025
Short summary
Wouter Mol and Chiel van Heerwaarden

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comments and recommendations about manuscript by Mol and Heerwaarden', Anonymous Referee #1, 24 Sep 2024
    • AC2: 'Reply on RC1', Wouter Mol, 15 Jan 2025
  • RC2: 'Comment on egusphere-2024-2396', Philipp Gregor, 15 Oct 2024
    • AC3: 'Reply on RC2', Wouter Mol, 15 Jan 2025
  • AC1: 'Comment on egusphere-2024-2396', Wouter Mol, 15 Jan 2025

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comments and recommendations about manuscript by Mol and Heerwaarden', Anonymous Referee #1, 24 Sep 2024
    • AC2: 'Reply on RC1', Wouter Mol, 15 Jan 2025
  • RC2: 'Comment on egusphere-2024-2396', Philipp Gregor, 15 Oct 2024
    • AC3: 'Reply on RC2', Wouter Mol, 15 Jan 2025
  • AC1: 'Comment on egusphere-2024-2396', Wouter Mol, 15 Jan 2025

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Wouter Mol on behalf of the Authors (15 Jan 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (16 Jan 2025) by Johannes Quaas
RR by Anonymous Referee #1 (30 Jan 2025)
RR by Philipp Gregor (04 Feb 2025)
ED: Publish subject to minor revisions (review by editor) (04 Feb 2025) by Johannes Quaas
AR by Wouter Mol on behalf of the Authors (16 Feb 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (17 Feb 2025) by Johannes Quaas
AR by Wouter Mol on behalf of the Authors (26 Feb 2025)

Journal article(s) based on this preprint

23 Apr 2025
Mechanisms of surface solar irradiance variability under broken clouds
Wouter Mol and Chiel van Heerwaarden
Atmos. Chem. Phys., 25, 4419–4441, https://doi.org/10.5194/acp-25-4419-2025,https://doi.org/10.5194/acp-25-4419-2025, 2025
Short summary
Wouter Mol and Chiel van Heerwaarden

Data sets

Supplementary data for "Mechanism of surface solar irradiance variability under broken cloud cover" Wouter Mol and Chiel van Heerwaarden https://doi.org/10.5281/zenodo.11503610

Wouter Mol and Chiel van Heerwaarden

Viewed

Total article views: 685 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
248 88 349 685 28 32
  • HTML: 248
  • PDF: 88
  • XML: 349
  • Total: 685
  • BibTeX: 28
  • EndNote: 32
Views and downloads (calculated since 20 Aug 2024)
Cumulative views and downloads (calculated since 20 Aug 2024)

Viewed (geographical distribution)

Total article views: 709 (including HTML, PDF, and XML) Thereof 709 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 23 Apr 2025
Download

The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.

Short summary
Sunlight varies often and quickly under broken cloud cover, and every cloud field creates a unique pattern of sunlight on the surface below. These variations affect many processes in the Earth system, from photosynthesis and chemistry, to cloud formation itself. The exact way in which cloud particles interact with sunlight is complex and expensive to calculate. We demonstrate a simplified framework which explains how sunlight changes for potentially any cloud field.
Share