LEE CLOUDINESS - METEOROLOGICAL PHYSICAL BACKGROUND

by ZAMG


There are two possibilities for air to flow past a mountain ridge. Either the air parcels go round the mountain or is forced to rise over the mountain: Which of these cases occurs, is dependant on several parameters:
The static stability (N), the height of the mountain or mountain ridge (h) and the wind component perpendicular to the mountain (U). The term Nh/U combining these parameters gives an idea whether there is a flow across the mountain or not: If U is small the mountain is difficult to cross; also if N increases (i.e. the atmosphere becomes more stable) the mountain will be more difficult to cross.

But even in the case of air partially streaming around the mountain, those streamlines approaching a greater height will cross the mountains.

When the wind has a component perpendicular to a mountain chain the air accumulation due to deceleration of wind speed by the obstacle on the upwind side creates high pressure. Part of the air is deflected upward giving rise to mountain waves. According to the theory of internal gravity waves, an air parcel within a stable stratified atmosphere will start to oscillate, as long as the waves are damped by friction.

Waves can only occur in a stable atmosphere. An air parcel which is removed from its original place cannot oscillate if there is no returning force. Lee Cloudiness will form where there is a sufficient supply of humidity near the wave crests and where there is upward motion. In the regions with downward motion the clouds will evaporate. The result is the pattern of parallel cloud lines perpendicular to the mountains.

One parameter to describe the state of the atmosphere in this situation is the Brunt - Vaisala frequency N2 which is defined by the following formula:

where
T temperature
θ potential vorticity
g gravity constant
cp specific heat at constant pressure

N2>0 stable atmosphere
N2 = 0.02 -0.03 inversions
N2 = 0 neutral atmosphere

Another important parameter is the Scorer parameter (symbolised by l) which combines stability and characteristics of the wind field; it is approximated by following formula:

where
U(z) profile of the wind speed on the windward side of the mountains
N(z) Brunt-Vaisala frequency

The typical profile of the Scorer parameter shows a high gradient in low levels due to increasing wind speeds. Higher levels often show values of about 0.0005/m, rarely exceeding 0.001/m. The smaller the Scorer parameter the easier waves are formed.

This parameter and the dimension of the mountain (L) determines if Lee Waves can be formed. The broader the mountain the easier waves can be formed. This relation can be expressed (assuming N and U are constant with height) by:

no Lee Waves are formed, but there are perturbations decreasing with height

Lee Waves are formed

The dimension of a critical width (L) is several kilometres, increasing with wind speed, but decreasing with increasing stability. If a mountain is not wide enough, Lee Waves will not develop.

Lee Waves are a form of vertical energy propagation. At higher levels the density of the air is less, that means the amplitude has to increase. Therefore the wavelength increases with height, which clearly is reflected in the more extended area of High Lee Cloudiness.

The wavelengths also depend on the shape of the mountains. There often is a dominating wave length.

The example from 18 January 2000 shows some of the parameters mentioned above. The image shows a region with Lee Cloudiness extending from the South Alps to the Adriatic Sea. The nearest available radiosonde was Milan which is indicated on the image. The Lee Cloud is quite high in this case and can be found just below 200 hPa.

18 January 2000/12.00 UTC - Meteosat IR image
18 January 2000/12.00 UTC - radiosonde Milan; column: stability analysis (blue: absolutely stable, yellow: conditionally unstable, red: absolutely unstable, green: inversion
The air column above Milan shows two conditionally unstable layers (yellow) restricted by inversions (green). The Lee Cloudiness under consideration is within a stable layer (blue) just below the upper inversion. This is in agreement with the above mentioned statement that Lee Cloud can only develop in a stable atmosphere.

18 January 2000/12.00 UTC - radiosonde Milan; wind direction
18 January 2000/12.00 UTC - radiosonde Milan; wind speed
18 January 2000/12.00 UTC - radiosonde Milan; Scorer Parameter
18 January 2000/12.00 UTC - radiosonde Milan; Brunt - Vaisälä - frequency (N2, solid curve) and Ns2 )Brunt - Vaisälä - frequency for saturation; dashed curve)

Trapped Lee Waves

A special class of Lee Waves are called "Trapped Lee Waves". This phenomenon is characterised by waves only occurring at lower levels. They occur when the vertical distribution of the Scorer-parameter can be approximated by two levels: an upper level with a quite low value for l (due to the increase of wind speed and the decrease of the Brunt - Vaisaila- frequency) and a lower level with a much higher value for l. In some cases (depending on the mountain range) the upper atmosphere cannot form waves, but the lower levels can. So the waves are trapped in this lower layer. In satellite imagery the height of the Lee Wave varies significantly from case to case. The trapped Lee Wave theory might be an explanation for apparently low cloud tops.

Sometimes in the lee of the mountains one can find inversions or at least strong stability near the surface and quite strong winds above it. Waves are found in these layers. In these situations displacements are large, which might result in a breaking of the waves.

N - S oriented mountain chain

If the N. - S. extent of a mountain range is large, effects of earth rotation are no longer negligible. As a consequence the flow over the mountain is no longer symmetrical. Due to changes in wind speed during ascent there is a changing in its Coriolis force. When a westerly flow passes a long mountain range extending north to south (e.g. the Scandinavian mountains) there will tend to be higher wind speeds to the south and lower wind speeds to the north.

Determination of Wind speed

The wind direction is quite similar at all levels but the wind speed increases with height. The typical wind speed lies between 10 and 20 m/s at the 700 hPa level, between 15 and 25m/s at the 500 hPa level and 15 to 35 m/s at the 300 hPa level. In literature it is said that - depending on the shape and scale of the mountain chain - the maximum wind is either found at the top of the mountain ridge or at the leeward side. Since ECMWF data were used in the study made by ZAMG, no change in the wind field by the mountains can be seen (problem of resolution).

There is a connection between mean wind speed and wave length of Lee Waves, although with rather a low coefficient of correlation. It can be approximated by a linear function (the higher the wind speed the longer the waves). However, such a linear regression is only valid for a certain indicated area.

Correlation between mean wind speed and Lee Wave length (from Cruette 176).
The straight lines symbolise different linear regressions found by different authors for different regions.

Unsolved problems

There are some unsolved questions relating to Lee Cloudiness which are discussed below:

Lee Cloud exceeds the mountain ridge line

There are cases which give the impression that Lee Cloudiness is more extensive than suggested by the orography. This can even lead to apparent "Lee Cloudiness" over the sea.
17 May 1999/06.00 UTC - Meteosat IR image
This effect is sometimes observed east of Iceland but it is difficult to find an explanation.

Cloud stripes parallel to the wind direction

There are sometimes cloud stripes aligned parallel to the wind direction. They look like waves, but they are, in fact, perpendicular to the typical direction of Lee Waves.

There are some possible explanations:

The single lee bands are generated separately by each mountain, so the cloudiness follows the orography (as shown below). Arguments in favour are:

06 February 1999/06.00 UTC - Meteosat VIS image; green: wind vectors 850 hPa

SUB-MENU OF LEE CLOUDINESS
CLOUD STRUCTURE IN SATELLITE IMAGES
KEY PARAMETERS