What are valley and mountain winds?
The mountain and valley wind circulation is a thermally driven local wind system found in mountainous regions. It is a diurnal wind system that mainly occurs during calm, stable high-pressure weather. The driving force behind the mountain and valley wind circulation is solar radiation, which means that valley and mountain winds are thermally driven winds, driven by temperature differences.
How do valley and mountain winds form?
The following factors occur in mountainous areas due to the topography, ultimately ensuring that the air over the mountain slopes warms up faster than in the valley:
- A more favourable angle of incidence: the slopes exposed to the sun and the adjacent air warm up faster.
- The smaller air volume in the mountain valleys (in comparison to the lowlands) that needs to be warmed (known as the ‘volume effect’).
- Lower air density at higher altitudes: correspondingly less energy is needed to heat the air (high-altitude heating surface).
At sunrise, the mountain slopes are the first to be directly exposed to sunlight, and so they warm up quickly (see factor 1 above). Since warm air is lighter than cold air, it rises in warm air bubbles on the sunny slopes. This produces a lower air pressure on the slopes compared to the atmosphere directly above the valley. As air tends to balance out pressure differences, air flows from the valleys towards the mountains, thus creating the upslope wind (see Figure 1a). At the same time, the air above the mountains warms up more quickly on a somewhat larger scale than over the lowlands (see factors 1–3 above), causing the pressure to drop more rapidly and to a greater extent in the mountains. This creates a pressure gradient between the Alps and the lowlands, with higher pressure in the lowlands, and lower pressure over the mountains. As a result, the thermal low that forms draws in air from the lowlands (see Figure 1b). This gives rise to an additional wind that blows up the valley: the valley wind.