A one-dimensional, second-order turbulence model with bulk cloud micro
physics and detailed radiative transfer is used to simulate the evolut
ion of a thermal internal boundary layer (TIBL) which develops above a
wide, open lead. A mixed-phase cloud, originally based at the surface
, is produced within the TIBL. The cloud initially fills the entire TI
BL but is later elevated above the surface with its top coincident wit
h the top of the TIBL. Model-derived cloud ice and cloud liquid water
mixing ratios exceed 0.06 g kg(-1) directly above the open lead, with
a secondary maximum near the top of the TIBL. In addition, precipitati
ng ice particles or snow fills the TIBL with a maximum snow mixing rat
io of about 0.05 g kg(-1). Radiative flux divergence results in strong
cooling at cloud top (which contributes to the local maxima in cloud
water mixing ratio at this level) and warming near the surface. The le
ad-induced cloud increases the downwelling long-wave irradiance receiv
ed at the surface by up to 70 W m(-2) (reducing the surface radiative
cooling by over 40%) during the baseline case. This value is quite sen
sitive to the assumed particle size and cloud particle concentration.
The vertical structure and composition of the lead-induced cloud is sh
own to strongly depend on the rate of snow production and the cloud wa
ter partitioning.