https://egusphere.copernicus.org/preprints/2026/egusphere-2026-81/

*Authors: *Tom Goren, Goutam Choudhury, and Graham Feingold

*08 January 2026*

*Abstract*
We introduce a new framework for defining marine stratocumulus cloud
morphologies using a ternary diagram. A ternary diagram is a triangular
representation of three components, with each vertex corresponding to 100%
of one component, and any point within the triangle representing a mixture
of all three that sums to 100%. We use cloud optical thickness (τc) as the
diagnostic physical variable and accordingly define three corresponding τc
classes. Different combinations of the three τc classes define different
cloud morphologies, which vary continuously within the ternary space. The
method is applied to one year of satellite observations of stratocumulus
clouds and reveals the frequency of occurrence of the different
morphologies across the ternary space. Large-eddy simulations complement
the satellite analysis and show that cloud evolution tends to follow
preferred paths across the ternary morphology space, explaining why the
observations are concentrated within a limited range of morphologies. We
further investigate the susceptibility of cloud liquid water path (LWP),
cloud albedo, and cloud fraction to variations in droplet number
concentration, conditioned on cloud morphology. We find that for the most
frequent observed morphologies, LWP and cloud albedo susceptibilities
largely offset each other, resulting in a net in-cloud albedo response
close to zero. The cloud fraction susceptibility is found to be positive in
precipitating morphologies and negative in non-precipitating morphologies.
These findings have important implications for marine cloud brightening,
whose effectiveness needs to be evaluated in a morphology-dependent
framework to achieve the intended outcomes.

*Source: EGUsphere *

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