Dust storms and haboobs
Dust storms and haboobs
复制标题
沙尘暴和哈布暴
作者:
Marsham J
Dust storms are most common in the world’s arid regions and deserts, but can form anywhere where strong winds combine with sediment that can be easily uplifted into the air. Dust is normally generated by a process called ‘saltation’: winds above a threshold wind-speed (typically around 6 to 11 m/s) entrain larger particles (0.1 to 1 mm) which bounce across the surface. These particles are themselves too heavy to be lifted high into the air, but energy released when they impact the soil can overcome binding forces, allowing smaller particles (typically 0.1 to 50 microns) to be emitted and entrained into the atmosphere. Dust aerosol is typically an external mixture of quartz, clays (such as kaolinite, illite), calcite, gypsum and iron oxides. Particles are typically non-spherical and platelet shaped. Ideal conditions for dust uplift are strong winds, little or no vegetation and a dry, sediment-based surface. Emission rates are usually considered to be a cubic function of friction velocity, with no emission below a threshold corresponding to a 10-m wind-speed of around 6 to 11 m/s. Emission is therefore a highly non-linear response that depends only on the relatively rare high wind-speed events, making it a challenge to model. Major dust sources include dried up lake beds (eg the Bodélé Depression in the southern Sahara), and areas affected by rare flash floods which bring new supplies of sediment to be uplifted, as soon as it becomes dry again.
DOI:
10.1007/978-94-017-8978-3
发表时间:
2014-04
期刊:
Mineral Dust
影响因子:
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作者:
P. Knippertz;J. Stuut
通讯作者:
P. Knippertz;J. Stuut