Met Office College - Course Notes Conceptual Models of Cyclogenesis Contents 1. Introduction 2. Types of cyclogenesis 2.1 2.2 2.3 Emerging cloud head cyclogenesis Instant occlusion cyclogenesis Comma cloud cyclogenesis 3. Cyclogenesis – summary 4. Further reading Crown Copyright. Permission to quote from this document must be obtained from The Principal, Met Office College, FitzRoy Road, Exeter, Devon. EX1 3PB. UK. Page 1 of 10 Last saved date: 13 February 2016 FILE: MS-TRAIN-COLLEGE-WORK-D:\106739730.DOC 1. Introduction This course note builds on the ideas described in the Met. Office College course note entitled Conveyor Belt Conceptual Models. These two notes should be used together. Cyclogenesis in extra-tropical latitudes usually occurs in association with an upper trough. The shape and orientation of this trough can vary greatly from cyclone to cyclone. Despite this, the component parts of most cyclogenesis events can be described in terms of conveyor belts and dry intrusions associated with the jet streaks around the trough. Several classification schemes have been developed which aim to categorise cyclogenesis into characteristic types. Perhaps the most widely used is that of Young (1993) which is described in detail in chapter 5 of Images in Weather Forecasting. Young’s scheme can be further simplified, and here we will look at just 3 classes of cyclogenesis, as listed below. Emerging cloud head cyclogenesis Instant occlusion cyclogenesis Comma cloud, or cold air cyclogenesis Within these 3 categories a wide range of configurations are possible depending on the shape of the trough and the interaction between the different flows in the developing system. 2. Types of cyclogenesis 2.1 Emerging cloud head cyclogenesis In this category, cyclogenesis occurs in association with a warm conveyor belt flow on the forward side of an upper trough. Fig. 1 summarises the main stages in this type of cyclogenesis. (i) W1 is a pre-existing WCB on the warm side of jet J1, ahead of the upper trough. Associated with this is a band of cloud known as the polar front cloud band. This can be oriented meridionally as in the satellite image in figure 3, or more zonally depending on the shape of the upper trough. J2 indicates a jet-streak to the rear of the trough axis, within the dry descending air. (ii) The first sign that cyclogenesis may occur is the development of an ‘S’ shaped curve to the sharp poleward edge of the cloud in the WCB. The presence of a jet left exit associated with the jet streak in Page 2 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc the dry intrusion flow (J2) induces ascent and cyclonic vorticity near the surface on the flank of the WCB. The evidence for this in satellite imagery is the appearance of an emerging cloud head, formed by a branching of the WCB at low levels, labelled W2. The cloud tops in this emerging cloud head will typically be lower than the cloud in W1. (iii) At a later stage the emerging cloud head may be reinforced by the development of a cold conveyor belt flow (CCB) feeding moisture into the cloud head. The presence of a CCB also indicates easterly system relative flow. The dry intrusion is now cutting into the centre of the system between W1 and the cloud head. This is often evident as a clear slot on IR imagery or a dark slot on WV pictures. If this dark slot becomes darker with time it indicates that the dry intrusion is descending to lower levels of the system, possibly undercutting the high w air in W1/W2, forcing more intense ascent and deepening of the system. Figure 1. Emerging cloud head cyclogenesis. J2 is the jet streak associated with the dry air to the rear of the upper trough. W1 is the pre-existing warm conveyor belt flow associated with jet J1. W2 is the secondary branch of the WCB which initially forms the emerging cloud head. CCB is the cold conveyor belt which develops once cyclogenesis is underway, indicating system-relative easterly flow at low levels. Figure 2 shows an IR satellite image of a developing cyclone at the stage of fig. 1(ii). At this stage the depression centre is located beneath the WCB at L, but as development continues the low centre will move towards the poleward edge of the WCB, eventually moving into the cloud free dry slot between the polar front cloud band and the emerging cloud head. Page 3 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc Figure 2. Emerging cloud head cyclogenesis as seen in an IR satellite image. This stage corresponds to fig. 1(ii). F indicates the polar front cloud band associated with the WCB. E indicates the emerging cloud head. At this stage the low centre is located at L. Young’s scheme further divides this category of cyclogenesis depending on whether the trough is confluent, diffluent or symmetrical. However, all 3 types exhibit similar signals at the early stages of development. In the case of a diffluent trough the W2 flow is likely to become more extensive as development continues and is often over-run by the dry intrusion producing a split cold front. 2.2 Instant occlusion cyclogenesis A long wave upper trough will often have a short wave trough embedded in the flow on the upstream side. On the forward side of this short wave trough there will be an area of positive vorticity advection (PVA) leading to ascent. This is often shown in satellite imagery by an area of enhanced convection in the cold air, with higher cloud tops than the surrounding cumulus cloud cells. Instant occlusion cyclogenesis involves an interaction of this cloud area in the cold air and the main polar front cloud band conveyor belt. The sequence of events leading to cyclogenesis is shown in fig. 3. (i) Although the cloud area in the cold air has convective cells embedded within it, it still shows some characteristics of a WCB, with slantwise ascent along the isentropic surfaces. This WCB is labelled W2. W1 is the main polar front cloud band WCB. Page 4 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc (ii) As W2 rounds the base of the long wave trough and approaches W1, new cloud is observed in the gap between the two. This shows that a CCB flow is emerging from beneath W1. PVA and warm advection associated with W2 have induced low level cyclonic vorticity and a system relative easterly flow. (iii) Eventually W2 merges with W1. The resulting cloud formation resembles the Norwegian model occlusion of a mature depression, but studying a sequence of imagery shows that the processes which lead to this state are completely different to the Norwegian model occlusion process. Once again, the dry intrusion is cutting into the system between the cloud head and W1. Figure 3. Instant occlusion cyclogenesis. J2 is the jet streak associated with the dry intrusion flow. W1 is the main WCB associated with jet J1. W2 is a WCB associated with a short wave trough embedded in the flow to the rear of the long wave trough axis, which then moves around the base of the main trough. CCB is the cold conveyor belt that forms once cyclogenesis is under way. Figure 3(iii) is very similar to fig. 1(iii) for the case of emerging cloud head cyclogenesis. However, in this case the cloud head did not emerge from beneath W1, but started out as a completely separate entity in the cold air. Figure 4 shows an IR image prior to instant occlusion cyclogenesis. C is the cloud area associated with W2 and F is the polar front cloud band associated with W1. As the image shows, C consists of a merged area of convective clouds, but there is also evidence for slantwise conveyor belt ascent. The cloud tops to the south west of C are low, and there appears to be a coherent band feeding into C. The highest cloud tops are on the northern side of C. Page 5 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc Figure 4. IR satellite image prior to instant occlusion cyclogenesis. C is the cloud area in the cold air associated with W2. F is the polar front cloud band associated with W1. The dry intrusion between W1 and the cloud head can result in overrunning and potential instability on the inside edge of the cloud head. Mass ascent of this potentially unstable air can result in the rapid formation of heavy convective precipitation and thunderstorms. Such a case is shown in fig. 5, with convective cloud forming in the dry slot of an instant occlusion. Figure 5. An instant occlusion cyclone in IR imagery. The dry intrusion is over-running air in the cloud head (C), resulting in potential instability and CB activity indicated by CON. In Young’s classification scheme, a further type of cyclogenesis is described which is a combination of the emerging cloud head and instant occlusion types. The cloud area C with its associated forcing for cyclonic development moves towards W1, but in this case, a cloud head emerges from beneath W1 without the two cloud areas (C and F) Page 6 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc merging. Cloud area C often begins to dissipate at this stage. Young describes this as induced wave cyclogenesis as the ascent associated with C induces a wave on F without the two areas merging. This type is described more fully on pages 259-266 of Images in Weather Forecasting. 2.3 Comma cloud cyclogenesis This category of cyclogenesis occurs entirely within the cold air to the poleward side of the polar front cloud band and so is sometimes referred to as cold air cyclogenesis. Figure 6 illustrates the sequence of events leading to cyclogenesis in such a case. (i) This picture is identical to fig. 3(i) for the case of instant occlusion cyclogenesis. Once again there is a WCB (W2) associated with a short wave trough to the poleward side of the main WCB W1. (ii) W2 with its associated cloud area, which often resembles a comma punctuation mark, moves around the base of the long wave trough. Studies suggest that if W2 approaches to within 300km of W1 then cyclogenesis will occur beneath W1 as in the instant occlusion case. However, if W2 remains more than 300km to the poleward side of W1 then cyclogenesis will occur beneath W2 without any interaction with the main polar front cloud band. (iii) Once W2 has rounded the base of the trough, the cloud area expands due to mass ascent and convection, and may start to rotate cyclonically as it moves. This indicates that cyclogenesis has occurred beneath W2, independently of the polar front cloud associated with W1. At this stage the polar front cloud band may actually start to dissipate as the comma cloud develops further. Figure 6. Comma cloud cyclogenesis. J2 is the jet streak associated with the dry intrusion flow. W1 is the main WCB associated with jet J1. W2 is a WCB associated with a short wave trough embedded in the flow to the rear of the long wave trough axis, which then moves around the base of the main trough. As the cyclone develops under W2, the cloud associated with W1 will often start to dissipate. Comma cloud cyclones tend to have quite a distinctive appearance on satellite imagery. There will often be convective cloud elements Page 7 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc embedded within the comma, and no high cirrus shield due to the lack of warm advection. The frontal structure of a comma cloud cyclone is not well marked since it forms completely within the cold air. A surface trough with a well marked wind veer and pressure kick but no clear dewpoint contrast takes the place of the surface cold front. Figure 7. IR satellite images of a comma cloud cyclone. (a) shows the system in its early stages, with the cold air cloud area C and the polar front cloud band F. (b) shows the system at a stage corresponding to fig 6(iii), 15 hours later. C has developed a typical comma shape with very cold cloud tops. F has started to dissipate. Figure 6 shows a comma cloud cyclone at 2 different stages of development.Figure 6(a) is very similar to fig. 4 for the instant occlusion case, with the cloud area C and polar front cloud band F. In this case C does not merge with F but, as shown in 7(b), it develops into a comma cloud cyclone polewards of F, which has started to dissipate in this picture. The cloud tops in C cool considerably in the 15 hours from 7(a) to 7(b). 3. Cyclogenesis – summary The classes of cyclogenesis described in this section are typical of the way many cyclones develop. Sometimes the real atmosphere is more complex than these models. Even so, most cyclogenesis events in midlatitudes will contain some elements which are recognisable from these simple conceptual models. Monitoring satellite imagery allows us to spot the early signs of cyclogenesis, and we can then apply simple conceptual models to make some assessment of how the system will develop in the future. By being able to recognise patterns of cyclogenesis from satellite imagery and other data, we have an early indication that development is Page 8 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc occurring. One of the most useful applications of this is in verifying an NWP model forecast. If the patterns we see in imagery are consistent with cyclogenesis predicted by the model, we can use the forecast products with some degree of confidence. However, if we can see cyclogenesis occurring in reality that has not been predicted by the NWP model then we know that some modifications to the forecast will be necessary. A classic example of when signs of cyclogenesis in satellite imagery were not recognised by forecasters or predicted by the NWP model was the October Storm in 1987. Ten years later, on Christmas Eve 1997, the Chief Forecaster at NMC did spot rapid cyclogenesis occurring that had not been predicted by the NWP model. He was able to adjust all the forecast products and the forecasts that were issued to customers were remarkably accurate. 4. Further reading Although this is a fairly lengthy course note, it should be regarded as an introduction to the subject of fronts and cyclogenesis. It is certainly worth doing more reading on the subject to get a better idea of some of the concepts introduced here. This is a short list of some good books and papers that cover the subject in more detail, or are of interest for historical reasons. T.W. Harrold. 1973. Mechanisms influencing the distribution of precipitation within baroclinic disturbances. Quarterly Journal of the Royal Meteorological Society. 99. 232-251. A pioneering paper on the subject of air flows within developing depressions. The first reference to conveyor belts. K.A. Browning. 1990. Organisation of clouds and precipitation in extratropical cyclones. Erik Palmen Memorial volume. American Met. Soc. An excellent summary of conveyor belt ideas. K.A. Browning. 1997. The dry intrusion perspective of extra-tropical cyclone development. Meteorological Applications. 4. 317-324. A descriptive paper discussing the importance of the dry intrusion in cyclogenesis and the evolution of fronts. M.J. Bader, G.S. Forbes, J.R.Grant, R.B.E. Lilley and A.J. Waters. 1995. Images in Weather Forecasting. Cambridge University Press. A comprehensive description of fronts and cyclogenesis from the viewpoint of features in satellite imagery. Section 4.2 deals with split cold fronts and section 5.2 describes Young’s scheme of cyclone classification. T.N. Carlson. 1991. Mid-Latitude Weather Systems. Routledge. Chapter 12 consists of a very detailed discussion of airflow through depressions, including a section on system-relative isentropic flow. Page 9 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc A. T. Semple 1998. Conceptual Models of Cyclogenesis. JCMM Internal report no. 92. A summary of the various conceptual models of fronts and cyclogenesis developed over the last 60 years, concentrating on conveyor belt ideas. Young’s cyclogenesis classes are described and unified into a life cycle model that includes the full spectrum of cyclogenesis events. Page 10 of 10 Last Saved Date: 13 February 2016 File: ms-train-college-work-d:\106739730.doc