by FMI
Schematically the vertical structure of stratocumulus-topped BL can be described as follows:
The mixing processes in a cloud layer are most important. Mixing processes are generated primarily by seven different mechanisms, which either support or dissolve the Sc Sheets. According to Stull (1991) they can be listed as follows:
Radiative processes above, within and below the cloud sheet are important factors in stratocumulus development. Short-wave solar radiation as well as long-wave IR radiation from the surface generate convective instability, which in turn is released as turbulent eddies. Hence the radiative processes and turbulence are closely connected.
Large-scale anticyclones represent one kind of favourable environment for Sc Sheets to form and develop, as the associated subsidence produces large-scale adiabatic warming and hence significant temperature inversions above the boundary layer. Climatologically, the most common (at least, most often referred to in meteorological literature) locations for extensive Sc Sheets are relatively cool waters such as the North Sea (see below) or the areas over cool oceanic currents adjacent to the North American west coast, where they have a quasi-permanent character. Sc Sheets in connection with high pressure ridges between frontal systems have a more transient character.
Over land Sc Sheets often form during the cool season either near the centre of high pressure (however, stratus formation is more likely there due to weak mechanical turbulence) or on the cool (eastern) side of it, where fresh and moist air flows in a shallow layer southwards (see cloud structure in satellite image ). An example of favourable locations for Sc can be found in eastern parts of Finland and adjacent land areas over Russia: cold, shallow and relatively moist north-easterly - northerly air streams east of an anticyclone cntered over, say, Scandinavia or the Norwegian Sea often cause an extensive Sc layer to form.
Sc Sheet formation is also often observed after a cold front passage as well as on the rear side of the low pressure. Cool air flow with reasonable wind shear, stable stratification and a large amount of moisture (not necessarily because of advection of moisture from the sea, but by evaporation of rain and from wet ground) form a suitable condition for Sc formation.
Sea areas are an example of a moisture source, which in synoptically favourable (anticyclonic) environments can produce long-lasting Sc Sheets. If the anticyclone is stationary causing steady wind conditions within the cloud sheet, the Sc Sheet can last even for several days without breaking up.
There are also other typical occasions when Sc cloudiness is reported. An example of this is the Sc cloudiness formed in summertime evenings by spreading of cumulus clouds. Sc clouds produced this way will not typically last for a long time. However, they can be seen even in satellite images (best in visible channel) as convective cellular daytime cumulus cloudiness turning into night-time Sc cloudiness with a smoother texture.
The fetch over sea is one of the key parameters for cloudiness. Sometimes these Sc will exist for days. Other key parameters for maintaining or dissipate the cloudiness are insulation, change in wind direction, wind shear just above and just beneath the inversion.
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02 July 1997/13.26 UTC - NOAA RGB image (channel 1, 2 and 4)
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02 July 1997/06.29 UTC - NOAA RGB image (channel 1, 2, and 4)
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The remarkable differences, both in radiation and turbulence factors, between the adjacent cloudy and cloud-free areas have an effect on the horizontal spreading of the Sc Sheet. Typically during the daytime (especially during summer months) the sun heats the lowest layers of cloud-free areas, the result being only fair-weather cumulus cloudiness. The solar radiation can even affect the edges of Sc Sheet and slow down its spreading. Hence the initially cloud-free areas close to the Sc Sheet can stay cloud-free all day. This feature can often be seen in Finland in connection with summertime outbreaks of cold air from the White Sea: the Sc Sheet is at first rapidly advected to eastern Finland and Karelia. However, later during the day the edges of the cloud start to erode and further movement of the sheet stops, as solar radiation dries and warms up the cool boundary layer ahead of the cloud sheet.
The most permanent and extensive Sc Sheets form, as previously mentioned, mostly in connection with cool and moist air streams. As Sc Sheets often form in the vicinity of anticyclones, their movement can be slow. If strong upward motions generated by fronts, depressions, etc. are absent, the development of the Sc Sheet is driven mainly by slower processes, such as large-scale subsidence. Thus, the appearance of the Sc Sheet can be identifiable for a longer period. In some cases an individual Sc Sheet can last days without significant change. Entrainment instability at the cloud top is needed for breaking up this kind of quasi-permanent cloud sheet. The more the cloud sheet breaks up, the more solar radiation penetrates it, hence generating a positive feedback for the continuing dispersal of cloud, given sufficiently low humidity of boundary layer air.