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:
09 June 1999/12.00 UTC - Meteosat VIS image; magenta: height contours 1000 hPa, red: height contours 700 hPa, blue: wind vectors 1000 hPa
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.
13 June 1999/12.00 UTC - Meteosat VIS image; blue: wind vectors 1000 hPa

3. Convergence Lines over the French Mountains

11 June 1999/12.00 UTC - Meteosat VIS image; magenta: height contours 1000 hPa, cyan: height contours 700 hPa, blue: wind vectors 1000 hPa

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.
09 June 1999/06.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa
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

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.
09 June 1999/12.00 UTC - Meteosat VIS image; wind vectors 925 hPa
09 June 1999/12.00 UTC - Meteosat VIS image; wind vectors 700 hPa
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.
09 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 925 hPa, cyan dashed: divergence 925 hPa
09 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 700 hPa, cyan dashed: divergence 700 hPa
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.
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
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
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.
09 June 1999/18.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa; position of vertical cross section indicated
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

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

11 June 1999/12.00 UTC - Meteosat VIS image; green: wind vectors 925 hPa
11 June 1999/12.00 UTC - Meteosat VIS image; cyan solid: convergence 925 hPa, cyan dashed: divergence 925 hPa
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

SUB-MENU OF OROGRAPHICALLY INDUCED CONVERGENCE LINES
METEOROLOGICAL PHYSICAL BACKGROUND
TYPICAL APPEARANCE IN VERTICAL CROSS SECTIONS