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Plateau-cooled air falls into the Makhtesh Ramon, traced by radiation fog, just after dawn. Radiative cooling of the desert highlands chills the air,
Plateau-cooled air falls into the Makhtesh Ramon, traced by radiation fog, just after dawn. Radiative cooling of the desert highlands chills the air, making it more dense than the air over the lowlands. Cooler air can also hold less water vapour; it condenses out as tiny fog droplets, which re-evaporate as the air warms. Here, the falling air is warming adiabatically, and so the fog re-evaporates as it falls.[citation needed]
Katabatic wind in Antarctica
Katabatic wind in Antarctica
The makhtesh is 40 km long, 2–10 km wide and 500 meters deep.
The makhtesh is 40 km long, 2–10 km wide and 500 meters deep.
A Nubian ibex on the edges of Makhtesh Ramon
A Nubian ibex on the edges of Makhtesh Ramon
A Nubian ibex on the edges of Makhtesh Ramon
A Nubian ibex on the edges of Makhtesh Ramon
Wide panorama of the Makhtesh Ramon crater, Israel
Wide panorama of the Makhtesh Ramon crater, Israel