https://egusphere.copernicus.org/preprints/2024/egusphere-2024-2559/

*Authors*
Kai Jeggle, David Neubauer, Hanin Binder, and Ulrike Lohmann

*Citations*: Jeggle, K., Neubauer, D., Binder, H., and Lohmann, U.: Cirrus
formation regimes – Data driven identification and quantification of
mineral dust effect, EGUsphere [preprint],
https://doi.org/10.5194/egusphere-2024-2559, 2024.

*Received: 13 Aug 2024 – Discussion started: 26 Aug 2024*

*Abstract*
The microphysical and radiative properties of cirrus clouds are strongly
dependent on the ice nucleation mechanism and origin of the ice crystals.
Due to sparse temporal coverage of satellite data and limited observations
of ice nucleating particles (INPs) at cirrus levels it is notoriously hard
to determine the origin of the ice and the nucleation mechanism of cirrus
clouds in satellite observations. In this work we combine three years of
satellite observations of cirrus clouds from the DARDAR-Nice retrieval
product with Lagrangian trajectories of reanalysis data of meteorological
and aerosol variables calculated 24 h backward in time for each observed
cirrus cloud. In a first step, we identify typical cirrus cloud formation
regimes by clustering the Lagrangian trajectories and characterize observed
microphysical properties for in situ and liquid origin cirrus clouds in
midlatitudes and the tropics. On average, in situ cirrus clouds have
smaller ice water content (IWC) and lower ice crystal number concentration
(Nice) and a strong negative temperature dependence of Nice, while liquid
origin cirrus have a larger IWC and higher Nice and a strong positive
temperature dependence of IWC. In a second step, we use MERRA2 reanalysis
data to quantify the sensitivity of cirrus cloud microphysical properties
to a change in the concentration of dust particles that may act as INPs. By
identifying similar cirrus cloud formation pathways, we can condition on
ice-origin, region, and meteorological dependencies, and quantify the
impact of dust particles for different formation regimes. We find that at
cloud top median Nice decreases with increasing dust concentrations for
liquid origin cirrus. Specifically, the sensitivities are between 5 % and
11 % per unit increase of dust concentration in logarithmic space in the
tropics and between 12 % and 18 % in the mid-latitudes. The decrease in
Nice can be explained by increased heterogeneous ice nucleation in the
mixed-phase regime, leading to fewer cloud droplets freezing homogeneously
once the cloud enters the cirrus temperatures and glaciates. The resulting
fewer, but larger ice crystals are more likely to sediment, leading to
reduced IWC, as for example observed for liquid origin cirrus in the
mid-latitudes. In contrast, for in situ cirrus in the tropics, we find an
increase of Nice median values of 21 % per unit increase of dust aerosol in
logarithmic space. We assume that this is caused by heterogeneous
nucleation of ice initiated by dust INPs in INP limited conditions with
supersaturations between the heterogeneous and homogeneous freezing
thresholds. Such conditions frequently occur at high altitudes, especially
in tropical regions at temperatures below 200 K. Our results provide an
observational line of evidence that the climate intervention method of
seeding cirrus clouds with potent INPs may result in an undesired positive
cloud radiative effect (CRE), i.e. a warming effect. Instead of producing
fewer but larger ice crystals, which would lead to the desired negative
CRE, we show that additional INPs can lead to an increase in Nice, an
effect called overseeding.

*Source: EGUsphere *

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