How the Atmosphere Influences Aridity

We live at the bottom of a gaseous envelope—the atmosphere—that is bound

gravitationally to the planet Earth. The circulation of our atmosphere

is a complex process because of the Earth’s rotation and the tilt of its

axis. The Earth’s axis is inclined 23½° from the ecliptic, the plane of

the Earth’s orbit around the Sun. Due to this inclination, vertical rays

of the Sun strike 23½° N. latitude, the Tropic of Cancer, at summer

solstice in late June. At winter solstice, the vertical rays strike 23½°

S. latitude, the Tropic of Capricorn. In the Northern Hemisphere, the

summer solstice day has the most daylight hours, and the winter solstice

has the fewest daylight hours each year. The tilt of the axis allows

differential heating of the Earth’s surface, which causes seasonal

changes in the global circulation.

[Illustration: The circulation pattern of the Earth’s atmosphere. Most

of the nonpolar deserts lie within the two trade winds belts.]

On a planetary scale, the circulation of air between the hot Equator and

the cold North and South Poles creates pressure belts that influence

weather. Air warmed by the Sun rises at the Equator, cools as it moves

toward the poles, descends as cold air over the poles, and warms again

as it moves over the surface of the Earth toward the Equator. This

simple pattern of atmospheric convection, however, is complicated by the

rotation of the Earth, which introduces the Coriolis Effect.

To appreciate the origin of this effect, consider the following. A stick

placed vertically in the ground at the North Pole would simply turn

around as the Earth rotates. A stick at the Equator would move in a

large circle of almost 40,000 kilometers with the Earth as it rotates.

The Coriolis Effect illustrates Newton’s first law of motion—a body in

motion will maintain its speed and direction of motion unless acted on

by some outside force. Thus, a wind travelling north from the equator

will maintain the velocity acquired at the equator while the Earth under

it is moving slower. This effect accounts for the generally east-west

direction of winds, or streams of air, on the Earth’s surface. Winds

blow between areas of different atmospheric pressures.

The Coriolis Effect influences the circulation pattern of the Earth’s

atmosphere. In the zone between about 30° N. and 30° S., the surface air

flows toward the Equator and the flow aloft is poleward. A low-pressure

area of calm, light variable winds near the equator is known to mariners

as the _doldrums_.

Around 30° N. and S., the poleward flowing air begins to descend toward

the surface in subtropical high-pressure belts. The sinking air is

relatively dry because its moisture has already been released near the

Equator above the tropical rain forests. Near the center of this

high-pressure zone of descending air, called the “Horse Latitudes,” the

winds at the surface are weak and variable. The name for this area is

believed to have been given by colonial sailors, who, becalmed sometimes

at these latitudes while crossing the oceans with horses as cargo, were

forced to throw a few horses overboard to conserve water.

The surface air that flows from these subtropical high-pressure belts

toward the Equator is deflected toward the west in both hemispheres by

the Coriolis Effect. Because winds are named for the direction from

which the wind is blowing, these winds are called the northeast trade

winds in the Northern Hemisphere and the southeast trade winds in the

Southern Hemisphere. The trade winds meet at the doldrums. Surface winds

known as “westerlies” flow from the Horse Latitudes toward the poles.

The “westerlies” meet “easterlies” from the polar highs at about 50-60°

N. and S.

Near the ground, wind direction is affected by friction and by changes

in topography. Winds may be seasonal, sporadic, or daily. They range

from gentle breezes to violent gusts at speeds greater than 300

kilometers/hour.

[Illustration: These dunes in the Algodones Sand Sea of southeastern

California move as much as 5 meters per year. The dunes in this

photograph, looking south, move toward the east (left) (photograph by

Peter Kresan).]

[Illustration: Searles Lake, California (photograph courtesy of

Kerr-McGee, Inc.).]

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