Convective Cloud Features In Typical Synoptic Environments: The Warm Sector - Typical Appearance In Vertical Cross Sections

by ZAMG


A cross section of the typical environment for the development of MCSs within the warm sector ahead of a frontal zone is characterised by the following (typical) features:
08 August 2004/18.00 UTC - Meteosat 8 IR 10.8 image; position of vertical cross section indicated

Isentropes


08 August 2004/18.00 UTC - Vertical cross section; lines: black: isentropes (ThetaE)

Temperature Advection


08 August 2004/18.00 UTC - Vertical cross section; lines: black: isentropes (ThetaE), red: temperature advection

Divergence


08 August 2004/18.00 UTC - Vertical cross section; lines: black: isentropes (ThetaE), magenta thin: divergence/convergence

The diagrams above show a vertical cross section across the frontal cloud band and the MCSs which have developed ahead of it. In the cross section the MCSs are characterised by an unstable stratification seen ahead of the frontal system around 44N/4E. These unstable stratified isentropes (decreasing values of equivalent potential temperature with height) reach the lower layers of the troposphere, up to approximately 700 hPa.
WA is associated to the MCSs and will contribute slightly to the upward motions. Not surprising, WA is found ahead and aloft of the Cold Front in the area of the Warm sector.

In the divergence field a pronounced maxima of convergence can be seen near the surface in the area of the warm sector. Aloft there is divergence causing outflow of air.


Menu Of Convective Cloud Features In Typical Synoptic Environments: The Warm Sector
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