OROGRAPHICALLY INDUCED CONVERGENCE LINES - KEY PARAMETERS
by ZAMG
Since these convective convergence lines are small-scale to meso-scale phenomena, data from a relevant Limited Area Model (LAM) area absolutely necessary to supplement ECMWF forecast data. In the study made by ZAMG, both models were used: the synoptic situation can be described sufficiently by ECMWF data, whereas the LAM model (ALADIN) is excellent for the interpretation of divergence, vertical motion and the wind field. The most important level for the detection of convection is 925 hPa. Nevertheless, Convergence Lines can also be detected in the model up to 800 hPa or in a few cases even higher. Whilst Convergence Lines show differences synoptically, they are similar in terms of small scale key parameters.
Typical synoptic environment
1. Greek convective Convergence Lines
These lines seem to occur in certain synoptic situations:
- There is a low or, at least, an upper level low over Turkey and a low over Central Europe.
- An upper level ridge (sometimes also a surface ridge) is situated over Greece.
- As there is no frontal situation over Greece, the equivalent thickness shows only a small gradient; The TFP sometimes shows a
positive value originating from a frontal system passing by to the north.
- The isobars at low levels show a weak gradient but with winds from a northerly direction.
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09 June 1999/12.00 UTC - Meteosat VIS image; magenta: height contours 1000 hPa, red: height contours 700 hPa, blue: wind
vectors 1000 hPa
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In this image, there is an upper level low over Turkey and low pressure covering northern Central Europe. Greece is situated at the eastern edge of a ridge at 700 hPa.
2. The Carpathian Convergence Lines
In such a situation there is no distinct synoptic pattern such as ridge or trough features or even a frontal system.
- Large scale winds show quite a homogeneous flow with mainly northerly and easterly components.
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13 June 1999/12.00 UTC - Meteosat VIS image; blue: wind vectors 1000 hPa
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3. Convergence Lines over the French Mountains
- The typical synoptic situation is characterised by a north-westerly upper level flow, a surface low in the Mediterranean near
the Gulf of Genoa and high pressure west of the Massif Central (France).
- Situations with a strong north-westerly flow creating a Mistral situation. However, in the case presented here the wind speed
is rather low, since the pressure gradients are relatively weak.
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11 June 1999/12.00 UTC - Meteosat VIS image; magenta: height contours 1000 hPa, cyan: height contours 700 hPa, blue: wind
vectors 1000 hPa
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Typical small scale parameters
Wind, convergence and vertical motion data detected in small scale model output show remarkable changes during day. The Greek Convergence Line is chosen to show common features. Some additional features are noted for the two other Convergence Lines.
Typical distribution of wind fields in the morning
In the morning (06 UTC) divergence (fields not shown here) prevails over the mountain chains whereas convergence occurs at higher levels. The wind fields show a flow around the mountains rather than over them. Orographic effects vanish at 800 hPa where a more or less uniform flow pattern (north-west wind) can be observed.
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09 June 1999/06.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa
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The example shows northerly winds around the mountain chain, with difluence at the northern edge. Some confluence can be found east of the mountains.
Typical distribution of wind fields, convergence and vertical motion at noon
- Wind fields are influenced by orography up to about 700 hPa: There is a confluence at lower levels (north-westerly winds in
the west, north-easterly winds in the east).
- As a consequence of this wind field, small scale convergence can be observed up to 800 hPa. At the 925 hPa level, the maximum
of convergence is shifted to the west (the windward side of the mountain ridge).
- Therefore, the maximum of upward motion can also often be found west of the mountain chain (around 1 degree), in a layer
which is somewhat thicker than can be observed for the convergence. Above 700 hPa, there appears to be no upward motion which can
be related to convergence cloudiness.
Typical distribution of wind-fields at noon
There is general confluence at low levels. At high levels, the wind direction is more or less parallel to the mountain chain.
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09 June 1999/12.00 UTC - Meteosat VIS image; wind vectors 925 hPa
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09 June 1999/12.00 UTC - Meteosat VIS image; wind vectors 700 hPa
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The image shows pronounced confluence around the mountain chain generated by easterly winds in the east and westerly winds in the west. Winds are parallel to the mountain chain at higher levels.
Typical distribution of divergence
Low level convergence is occuring at the mountain, divergence alongside. The situation at higher levels is reversed.
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09 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 925 hPa, cyan dashed: divergence 925 hPa
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09 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 700 hPa, cyan dashed: divergence 700 hPa
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The convective convergence line closely follow a narrow zone of convergence (solid lines) at 925 hPa.
At 700 hPa the flow is more divergent suggesting that the phenomenon is rather shallow.
Typical distribution of vertical motion at noon
There is low level upward motion occuring at he mountain, downward motion alongside. The situation at higher levels is reversed.
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09 June 1999/12.00 UTC - Meteosat VIS image; yellow solid: vertical motion - upward motion 925 hPa, yellow dashed:
vertical motion - downward motion 925 hPa
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09 June 1999/12.00 UTC - Meteosat VIS image; yellow solid: vertical motion - upward motion 700 hPa, yellow dashed:
vertical motion - downward motion 700 hPa
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Both images show upward motion in the region of the mountains. At 925 hPa, the velocities are much higher. At 700 hPa there is still some upward motion, although at this level there is also some areas of divergence (see above).
Typical distribution of wind-fields in the afternoon
In the evening (18.00 UTC) the model parameter are similar to those at 06.00 UTC, but occasionally they show some remnants of "daytime features". The convergence zone that developed at noon is decaying at this point in time and, consequently, does not show a distinct pattern.
Wind fields are revertoing to a typical night-time non-convergent flow.
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09 June 1999/18.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa; position of vertical cross section indicated
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The image shows northerly to easterly winds in the east, northerly winds in the west. The noon confluent pattern is disappearing.
Additional features apparent in the Carpathian Convergence Lines
- In general, the wind field can be characterised by north-easterly winds east of the Eastern Carpathians which become
south-easterly winds at the Southern Carpathians. Therefore, there are components directed towards the mountain ranges. In
Transylvania southerly and easterly winds prevail. In addition, the wind field shows a lot of small vortices within this
orographic region.
- As a consequence of the wind field, areas of convergence can be found at lower levels. At 925 hPa it is more or less
associated with the lines of cloudiness. The Southern Carpathians and the Eastern Carpathians show two separate areas of
convergence with a small area of divergence at the "corner".
- In the afternoon and evening, some small areas of convergence still exist, although they are more likely connected with huge
convective cells (MCS) which can survive for longer points of time.
11 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 925 hPa, cyan dashed: divergence 925 hPa
The image shows pronounced orographically induced convergence at 925 hPa. At the transition between the Southern and Eastern Carpathians there is almost no convergence, and even some divergence.
11 June 1999/12.00 UTC - Meteosat VIS image; yellow solid: vertical motion - upward motion 925 hPa, yellow dashed: vertical
motion - downward motion 925 hPa
The image shows pronounced upward motion at 925 hPa. At the "corner", downward motion is found, the postion of this area is more clearly seen with this parameter than with the field of convergence.
Additional features for the Convergence Lines in the French mountains
- The wind fields show northerly directions becoming northwest and west with height but show distinct confluence at several
mountain ridges (Massif Central, Jura mountains, West Alps) leading to upward motion from the surface up to levels of 850/800
hPa.
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11 June 1999/12.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa
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11 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 925 hPa, cyan dashed: divergence 925 hPa
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11 June 1999/12.00 UTC - Meteosat VIS image; lyellow solid: vertical motion - upward motion 925 hPa, yellow dashed:
vertical motion - downward motion 925 hPa
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