POLAR LOW - TYPICAL APPEARANCE IN VERTICAL CROSS SECTIONS

by KNMI


Although the Polar Low is a small-scale system, the typical polar environment and main dynamic forcing mechanisms can be observed in a vertical cross section.
19 March 2001/16.50 UTC - NOAA CH4 image; position of vertical cross section indicated. A developing polar low south west of Svalbard

ThetaW

19 March 2001/18.00 UTC - Vertical cross section; black: isentropes (ThetaE)

Vorticity advection

19 March 2001/18.00 UTC - Vertical cross section; green: vorticity advection - PVA, black: isentropes (ThetaE)

Potential Vorticity

19 March 2001/18.00 UTC - Vertical cross section; green: potential vorticity, black: isentropes (ThetaE)

Vertical Motion (Omega)

19 March 2001/18.00 UTC - Vertical cross section; cyan: vertical motion (omega), black: isentropes (ThetaE)

MATURE PHASE

20 March 2001/23.30 UTC - Meteosat IR image; position of vertical cross section indicated

Vertical Motion (Omega)

In the mature phase, a deep layer of negative omega is surrounded by areas of positive omega. Although the ascending air motions are sometimes situated in an area of PVA and some warm advection, this negative omega can not be completely explained by these mechanisms alone. Convective instability is playing an important role too. The descending air motion to the rear of a Polar Low is often enhanced by cold air advection. Because of the relative small resolution of most operational models compared to the scale of a Polar Low, descending air motion at the centre of a Polar Low is difficult or impossible to see in a vertical cross section.
21 March 2001/00.00 UTC - Vertical cross section; cyan: vertical motion (omega), black: isentropes (ThetaE)

SUB-MENU OF POLAR LOW
KEY PARAMETERS
WEATHER EVENTS