by KNMI and ZAMG
However, within this manual and the satellite report, the conceptual model of the so-called Emerging Cloud Head is associated with Rapid Cyclogenesis and will therefore now be described in more detail.
While classical cyclogenesis through Wave development (see
Wave
) is often slow and the Wave bulge dissolves after some time or produces a spiral after some days, Rapid Cyclogenesis usually leads to a fast development of a cloud spiral.
Within the polar front theory no separation between Wave development and Rapid Cyclogenesis can be found, and the distribution of the key parameters is very similar to, and even more distinct than, that for Wave development (see Key parameters). In addition to the Wave model, the jet streak and surrounding sinking dry air play key roles. The emerging cloud head in the initial stage usually appears in the left exit region of a jet streak. The jet streak is parallel to the initial cloud band with dry stratospheric air approaching downstream into the cloud head. This is seen as the typical black stripe in the WV imagery as well as the field of PV showing values higher than one PV units. While in the case of Wave development stratospheric air (if present at all) does not reach down to levels lower than 300 hPa, in the case of Rapid Cyclogenesis stratospheric air is a key feature and protrudes much further downward (down to approximately 500 hPa or even lower).
The dry sinking stratospheric air has a significant impact upon the cloud configuration. As it dissolves the cloudiness between the front and the cloud head, a spiral structure as well as the typical V - pattern develop. This is closely connected with special characteristics of relative streams.
There are several conveyor belts involved belonging to the different cloud systems. The cloudiness of the main frontal zone is produced by a typical Warm Conveyor Belt together with a humid relative stream from behind (see Cold Front ) while the dry stream from behind appears behind the poleward edge of the frontal cloud band. This is the dry stream containing stratospheric air described above. The cloud head is formed within the lower and mid-levels of the troposphere by a rapidly ascending conveyor belt advecting warm and moist air from lower latitudes beneath the Warm Conveyor Belt of the frontal zone. After crossing this Cold Front zone the conveyor belt often splits into a westward and an eastward flowing branch. This splitting of the relative flow leads to the convex-formed cloud edge at the pole ward side of the cloud head. This is comparable to the Occlusion process in Wave development (see Wave and Occlusion: Warm Conveyor Belt Type ).
As the advected air of the dry intrusion originates from the lower levels of the stratosphere, this flow is characterized by high values of potential vorticity. In the area where the dry intrusion is superimposed on the ascending conveyor belt from southern directions a potentially unstable stratification of the troposphere develops in which thunderstorms frequently occur (see Cloud structure in satellite images and Weather events).
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14 October 2002/06.00 UTC - Meteosat WV image; height of 2 units potential vorticity (in meters); magenta:
potential vorticity
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14 October 2002/12.00 UTC - Meteosat WV image; height of 2 units potential vorticity (in meters); magenta
potential vorticity
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14 October 2002/18.00 UTC - Meteosat WV image; height of 2 units potential vorticity (in meters); magenta
potential vorticity
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Comparing again Wave development (see Wave ) and Rapid Cyclogenesis, a main difference can be found in the orientation of the relative stream forming the cloud head, or cloud bulge. It is similar to a Warm Conveyor Belt in the case of the Wave turning to east/north-eastern direction, but quite opposite in the case of Rapid Cyclogenesis turning to west/south-western directions. There are some differences between the two models, which can lead to this different behaviour:
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31 January 2002 12.00 UTC - Meteosat IR image; Magenta: height 1000 hPa, Cyan: height 500 hPa
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12 December 2002 18.00 UTC - Meteosat IR image; Magenta: height 1000 hPa, Cyan: height 500 hPa
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31 January 2002/18.00 UTC - Vertical cross section; black: isentropes (ThetaE), red: temperature advection,
orange: WV pixel values
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31 January 2002/18.00 UTC - Meteosat WV image; magenta: relative streams 302K - system velocity: 262° 10 m/s,
yellow: isobars 302K, magenta: relative streams, position of vertical cross section indicated
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