Moreover, the longer the continuous plowed spaces, the higher the erosion and then the dust storms. As a result of dust storms, dust clouds are formed that can rise several kilometers from the earth's surface. The most devastating was the case of a dust storm in 1928. When in the steppe and forest-steppe regions of Ukraine, the wind tore off a layer of soil up to 15 mm thick from an area that is about four times the size of the UK. The height of the dust cloud reached 500 meters. The black earth dust moved westward, settling in the Carpathian Mountains, Romania and Poland. Dust storms are usually observed in the spring (March—May), but they may occur at any time of the year. Dust storms occur in the fields of the United States, Canada, Australia and other countries.
Taming the wind, in particular with the help of forest protection strips, non-tillage plowing and other methods of cultivating and strengthening the soil and soil significantly counteract the occurrence of dust storms and reduce their harmful effects. If a number of effective measures are used to tame the dust genie on earth, then dust storms in the atmosphere of other planets arise spontaneously and stop just as spontaneously. Particularly significant dust storms were observed in the Martian atmosphere. Even during the flight of the Mars and Mariner interplanetary stations in late 1971 and early 1972, a unique opportunity was created to compare Martian dust storms with terrestrial ones. In addition to local dust storms on Mars, global ones were also observed, which were repeated once or twice a year. The atmosphere of Mars is constantly (and heavily) dusted. The increased concentration of aerosols causes the light orange color of the Martian sky. During dust storms, Martian soil particles rise 30 or even 60 kilometers from the surface of the planet, i.e. significantly higher than during terrestrial dust storms. On Mars, the wind speed, which turns soil particles into an aerosol system, is from 30 to 60 m/s, i.e. more than on Earth. It is assumed that the size of particles that enter the Martian atmosphere during dust storms ranges from 10 to 300 microns. The differences between Martian dust storms and terrestrial ones are explained by the fact that Mars has a lower atmospheric density and gravitational potential. Therefore, dust storms on Mars practically spread throughout the planet and have a significant impact on the weather and climate of the planet as a whole, rather than its individual area. Dust clouds absorb some of the solar radiation, which helps to cool the planet's surface and increase the temperature of the Martian atmosphere. To make your first experience on a betting platform as profitable as possible, it is worth using all available tools. One of them is the promo code in the registration form. It instantly increases the size of the welcome reward. After entering
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