Abstract. The properties of a warm convective cloud are determined by the competition
between the growth and dissipation processes occurring within it. One way to
observe and follow this competition is by partitioning the cloud to core and
margin regions. Here we look at three core definitions, namely positive vertical
velocity (Wcore), supersaturation (RHcore), and positive buoyancy (Bcore),
and follow their evolution throughout the lifetime of warm convective
clouds. Using single cloud and cloud field simulations with bin-microphysics
schemes, we show that the different core types tend to be subsets of one
another in the following order: Bcore⊆RHcore⊆Wcore. This property is seen for several different thermodynamic profile
initializations and is generally maintained during the growing and mature
stages of a cloud's lifetime. This finding is in line with previous works
and theoretical predictions showing that cumulus clouds may be dominated by
negative buoyancy at certain stages of their lifetime. The RHcore–Wcore
pair is most interchangeable, especially during the growing stages of the
cloud. For all three definitions, the core–shell model of a core (positive values)
at the center of the cloud surrounded by a shell (negative values) at the
cloud periphery applies to over 80 % of a typical cloud's lifetime. The
core–shell model is less appropriate in larger clouds with multiple cores
displaced from the cloud center. Larger clouds may also exhibit buoyancy
cores centered near the cloud edge. During dissipation the cores show less
overlap, reduce in size, and may migrate from the cloud center.