Cirrus clouds play an important role in determining the radiation budget of the earth, but many of their properties
remain uncertain, particularly their response to aerosol variations and to warming. Part of the reason for this uncertainty is
the dependence of cirrus cloud properties on the cloud formation mechanism, which itself is strongly dependent on the local
meteorological conditions.
In this work, a classification system (Identification and Classification of Cirrus or IC-CIR) is introduced to identify cirrus
clouds by the cloud formation mechanism. Using re-analysis and satellite data, cirrus clouds are separated in four main types:
orographic, frontal, convective and synoptic. Through a comparison to convection-permitting model simulations and back-
trajectory based analysis, it is shown that these observation-based regimes can provide extra information on the cloud scale
updraughts and the frequency of occurrence of liquid-origin ice, with the convective regime having higher updraughts and a
greater occurrence of liquid-origin ice compared to the synoptic regimes. Despite having different cloud formation mecha-
nisms, the radiative properties of the regimes are not distinct, indicating that retrieved cloud properties alone are insufficient to
completely describe them.
This classification is designed to be easily implemented in GCMs, helping improve future model-observation comparisons
and leading to improved parametrisations of cirrus cloud processes