Meteorology: The Science of the AtmosphereTalman, Charles Fitzhugh
Science
Meteorology: The Science of the Atmosphere
Talman, Charles Fitzhugh
Meteorology
The dust of which we have to speak in the present chapter embraces all
small particles of solid matter found anywhere, or at any time, in the
earth’s atmosphere. Particular kinds of dust have, of course, their
special names. Soot, the visible part of smoke, is a form of dust that
has played a very conspicuous part in human affairs; hence the separate
mention of smoke in the heading of this chapter.
While there are many agencies that help to charge the atmosphere with
dust, the most important of them all is the wind. Let us see what
happens when the wind blows over the surface of a dusty road, for
example. If the air flowed in a smooth horizontal stream over such
a surface, its friction would drag the dust along on the ground,
but would not lift it. Such surface drifting, due to the horizontal
component of the wind’s motion, does, of course, occur, and its effects
are strikingly visible in the shifting dunes that often form over a
broad surface of sand or snow. All winds near the earth’s surface are,
however, full of waves and eddies, and in many cases, as over a stretch
of strongly heated soil, there are strong updrafts, sometimes extending
to a great height in the atmosphere. All kinds of dust are heavier
than air, and, contrary to popular belief, never truly “float” in the
atmosphere. Dust may enter the atmosphere at high levels, through the
disintegration of meteors, or it may be spouted up by volcanoes, but
dust blown up from the earth’s surface rises only because the air is
rising with it; and, in still air, all dust sinks more or less rapidly
toward the ground. The rate of its fall depends upon its specific
gravity, and upon the size and shape of the dust particles. Other
things being equal, the finest particles fall most slowly. Exceedingly
fine dust, even without upward air movements to support it, requires
months or even years to fall to the ground from the higher levels of
the atmosphere.
Public-domain text, read in full here on John Shaqi.
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