
Environmental Encyclopedia 3
Climate
shapes, surface features, and locations of continents change.
The atmosphere’s composition changes from time to time,
so that different wavelengths are reflected or pass through.
The amount of energy the earth receives also shifts over time.
During the course of a decade the rate of solar energy
input varies by a few watts per square meter. Changes in
energy input can be much greater over several millennia.
Energy intensity also varies with the shape of the earth’s
orbit around the sun. In a period of 100 million years the
earth’s elliptical orbit becomes longer and narrower, bringing
the earth closer to the sun at certain times of year, then
rounder again, putting the earth at a more uniform distance
from the sun. When the earth receives relatively intense
energy, heating and evaporation increase. Extreme heating
can set up exaggerated convection currents in the atmo-
sphere, with extreme low pressure areas receiving intensified
rains and high pressure areas experiencing extreme
drought
.
The earth’s albedo depends upon surface conditions.
Extensive dark forests absorb a great deal of energy in heat-
ing, evaporation of water, and photosynthesis. Light, colored
surfaces, such as
desert
or snow, tend to absorb less energy
and reflect more. If highly reflective continents are large or
are located near the equator, where energy input is great,
then they could reflect a great deal of energy back into the
atmosphere and contribute to atmospheric heating. How-
ever, if those continents are heavily vegetated, their reflective
capacity might be lowered.
Other features of terrestrial geography that can influ-
ence climate conditions are mountains and glaciers. Both
rise and fall over time and can be high enough to interrupt
wind and precipitation patterns. For instance, the growth
of the Rocky Mountains probably disturbed the path of
upper atmospheric winds known as the jet stream. In south-
ern Asia, the Himalayas block humid air masses flowing
from the south. Intense precipitation results on the windward
side of these mountains, while the downwind side remains
one of the driest areas on Erth.
Atmospheric composition is a climate variable that
began to receive increased attention during the 1980s. Each
type of gas molecule in the atmosphere absorbs a particular
range of energy wavelengths. As the mix of gases changes,
the range of wavelengths passing through the filter shifts.
For instance, the gas
ozone
(O
3
) selectively blocks long
wave UV radiation. A drop in upper atmospheric ozone
levels discovered in the late 1980s has caused alarm because
harmful UV rays are no longer being intercepted as effec-
tively before they reach the earth’s surface. Water vapor and
solid particulates (dust) in the upper atmosphere also block
incoming energy. Atmospheric dust associated with ancient
meteor impacts is widely thought responsible for climatic
cooling that may have killed the earth’s dinosaurs 65 million
years ago. Climate cooling could occur today if bombs from
267
a nuclear war threw high levels of dust into the atmosphere.
With enough radiation blockage, global temperatures could
fall by several degrees, a scenario known as
nuclear winter
.
A human impact on climate that is more likely than
nuclear winter is global warming caused by increased levels
of
carbon dioxide
(CO
2
) in the upper atmosphere. Most
solar energy enters the atmospheric system as long wave-
lengths and is reflected back into space in the form of short
wavelength (heat) energy.
Carbon
dioxide blocks these
short, warm wavelengths as they leave the earth’s surface.
Unable to escape, this heat energy remains in the atmosphere
and keeps the earth warm enough for life to continue. How-
ever, many studies suggest that the burning of
fossil fuels
and
biomass
have raised atmospheric carbon dioxide levels.
Rising CO
2
levels could trap excessive amounts of heat and
raise global air temperatures to dangerous levels. This sce-
nario is popularly known as the
greenhouse effect
. Extreme
amounts of trapped heat could disturb precipitation patterns.
Ecosystems could overheat, killing plant and animal species.
Polar ice caps could melt, raising global ocean levels and
threatening human settlements.
Increased anthropogenic production of other gases
such as
methane
(CH
4
) also contributes to atmospheric
warming, but carbon dioxide has been a focus of concern
because it is emitted in much greater volume.
No one knows how seriously human activity may be
affecting the large and turbulent patterns of climate. Some-
times a very subtle event can have magnified repercussions in
larger wind, precipitation, and pressure systems, disturbing
major climate patterns for decades. In many cases the climate
appears to have a self-stabilizing capacity—an ability to initi-
ate internal reactions to a destabilizing event that return it
to equilibrium. For example, extreme greenhouse heating
should cause increased evaporation of water. Resulting
clouds could block incoming sunlight, producing an overall
cooling effect to counteract heating.
Furthermore, human influences work on climate
within a context of continually changing natural conditions
and events. On a geologic time scale, temperatures, precipita-
tion, and ocean levels have fluctuated enormously. A long
series of ice ages and warmer interglacial periods began 2.5
million years ago and may still be going on. The last glacial
maximum, with low sea levels because of extreme ice vol-
umes, ended only 18,000 years ago—an instant in the earth’s
climate history.
Natural fluctuations occur on a more human time scale,
as well. A summer of extreme drought and high temperatures
in the United States in 1988 brought threats of global warm-
ing to the public’s attention, but the drought itself resulted
from a temporary aberration in high altitude wind patterns
that centered an unusually stable high pressure zone over the
Midwest. This temporary departure from normal conditions