the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
A Lagrangian Perspective on the Lifecycle and Cloud Radiative Effect of Deep Convective Clouds Over Africa
Abstract. The anvil clouds of tropical deep convection have large radiative effects in both the shortwave (SW) and longwave (LW) spectra with the average magnitudes of both over 100 Wm-2. Despite this, due to the opposite sign of these fluxes, the net average of anvil cloud radiative effect (CRE) over the tropics has been found to be neutral. Research into the response of anvil CRE to climate change has primarily focused on the feedbacks of anvil cloud height and anvil cloud area, in particular regarding the LW feedback. However, tropical deep convection over land has a strong diurnal cycle which may couple with the shortwave component of anvil cloud radiative effect. As this diurnal cycle is poorly represented in climate models it is vital to gain a better understanding of how its changes impact anvil CRE.
To study the connection between deep convective cloud (DCC) lifecycle and CRE, we investigate the behaviour of both isolated and organised DCCs in a 4-month case study over sub-Saharan Africa (May–August 2016). Using a novel cloud tracking algorithm, we detect and track growing convective cores and their associated anvil clouds using geostationary satellite observations from Meteosat SEVIRI. Retrieved cloud properties and derived broadband radiative fluxes are provided by the CC4CL algorithm. By collecting the cloud properties of the tracked DCCs, we produce a dataset of anvil cloud properties along their lifetimes. While the majority of DCCs tracked in this dataset are isolated, with only a single core, the overall coverage of anvil clouds is dominated by those of clustered, multi-core anvils due to their larger areas and lifetimes.
We find that the distribution of anvil cloud CRE of our tracked DCCs has a bimodal distribution. The interaction between the lifecycles of DCCs and the diurnal cycle of insolation results in a wide range of SW anvil CRE, while the LW component remains in a comparatively narrow range of values. The CRE of individual anvil clouds varies widely, with isolated DCCs tending to have large negative or positive CREs while larger, organised systems tend to have CRE closer to zero. Despite this, we find that the net anvil cloud CRE across all tracked DCCs is indeed neutral within our range of uncertainty (0.86 ± 0.91 Wm-2). Changes in the lifecycle of DCCs, such as shifts in the time of triggering, or the length of the dissipating phase, could have large impacts on the SW anvil CRE and lead to complex responses that are not considered by theories of LW anvil CRE feedbacks.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
(3849 KB)
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3849 KB) - Metadata XML
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2023-2059', Adam Sokol, 11 Oct 2023
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AC1: 'Reply on RC1', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC1-supplement.pdf
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AC1: 'Reply on RC1', William Jones, 23 Feb 2024
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RC2: 'Comment on egusphere-2023-2059', Anonymous Referee #2, 27 Oct 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-RC2-supplement.pdf
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AC2: 'Reply on RC2', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC2-supplement.pdf
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AC2: 'Reply on RC2', William Jones, 23 Feb 2024
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AC3: 'Comment on egusphere-2023-2059', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC3-supplement.pdf
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2023-2059', Adam Sokol, 11 Oct 2023
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AC1: 'Reply on RC1', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC1-supplement.pdf
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AC1: 'Reply on RC1', William Jones, 23 Feb 2024
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RC2: 'Comment on egusphere-2023-2059', Anonymous Referee #2, 27 Oct 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-RC2-supplement.pdf
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AC2: 'Reply on RC2', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC2-supplement.pdf
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AC2: 'Reply on RC2', William Jones, 23 Feb 2024
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AC3: 'Comment on egusphere-2023-2059', William Jones, 23 Feb 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2059/egusphere-2023-2059-AC3-supplement.pdf
Peer review completion
Journal article(s) based on this preprint
Data sets
Cloud-CCI+ SEVIRI CRE case study dataset William K. Jones https://zenodo.org/record/8317025
Model code and software
tobac-flow v1.7.6 William K. Jones https://zenodo.org/record/8317062
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Cited
1 citations as recorded by crossref.
William K. Jones
Martin Stengel
Philip Stier
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3849 KB) - Metadata XML