The heat balance of the Earth is a delicate thing, and we must take whatever actions are possible to ensure that we don't upset that balance.  The natural balance, which takes radiative heat from the Sun, redistributes it, and re-emits part of the heat back into space, is what makes life possible on Earth.  The heat balance of the planets Venus and Mars became disrupted early in their history; so the surface of Venus is like a very hot oven, and Mars is too cold to sustain any complex life as we know it. 
The development of complex life on Earth is a direct consequence of the
relatively stable heat balance, and the retention of an atmosphere and
oceans.  That balance is largely due to greenhouse gases in the
atmosphere.  Those greenhouse gases are a blessing; but too much
can cause unwanted warming.  It has been well documented that
the Earth has recently entered a period of gradual Global Warming. 
This promises to be the greatest scientific, engineering, poltical,
social, and economic challenge of the twenty-first century.
The onset of global warming has called
attention to the importance of "greenhouse gases", particularly carbon
dioxide (CO2), methane (CH4), and water vapor
(H2O).  The first two are byproducts of man's
activities; and have been continuously increasing since they were first
measured.  Research workers have attacked the problem using
geochemical models and various kinds of paleoclimatic data,
particularly from ice cores in Greenland and Antarctica.  The
results are highly dependent on the other data that went into the
geochemical models, such as temperatures, amount of ice locked in
glaciers, etc., but they do indicate some interesting trends.
There are two major research problems associated assessing the effects of
greenhouse gases:
One of the great problems with the Milankovitch
theory of glacial cycles is its inability to account for the long
ice-free periods, which may have lasted as long as 40 million or more
years.  Calculations for the past 100 million years indicate that
the CO2 concentration during the time of the dinosaurs may
have been as great as 90 times the values at the beginning of the
20th century.  The concentrations dropped continuously
though the Cretaceous period, to a value comparable with present values at
the time of the dinosaurs' extinction, about 65 million years ago. 
The concentration rose again during the early Cenozoic era to several times present
values, but fell dramatically at the beginning of the ice ages.  After
the early Cenozoic, beginning about 50 million years ago, the climate began
to gradually coola trend that continued until the present time.
Research workers have been impressed with the instability of the Earth's
climate, and the complexity of the interrelationships between the
various components.  During times when the Earth was quite warm, the
amount of water in glaciers and ice caps has been almost
negligible.  At the same time the amount of water vapor in the
atmosphere had increased.  Water can act as a greenhouse gas in its
vapor state, thus contributing to the warming, or it can cause cooling
if dense clouds form.
After the continental glaciers began to melt, in response to
increased solar heating, the warming process was accelerated
by increases in the amount of water vapor and CO2
in the air.  The warming was also accelerated as more land
was exposed to absorb solar energy.  The figure schematically
shows the progress of those effects along with the increase in solar
radiation during the summer.
The greenhouse effect is easily explained, though most textbooks on
weather and climate do not present the whole story.  The
temperature of the Sun's radiating surface is about 6000 Kelvin
(a Kelvin degree is the same as a Celsius, or Centigrade degree, or 9/5
times a Fahrenheit degree, the Kelvin scale begins at absolute zero =
-273 C = -459 F).  The peak radiation is at a wavelength of about
5.5 micron, which corresponds to yellow-green light in the middle of
the visible spectrum.  The total radiant energy emitted by a hot
body like the Sun is proportional to the 4th power of the temperature. 
A tiny change in the temperature would result therefore in a large
increase in the total radiated energy.  Fortunately the Sun's
output is quite constant; though a tiny change in the average temperature
might have caused the Little Ice Age.
If the Earth were completely surrounded by a radiating body at a
temperature of 6000 K it would attain a radiative equilibrium temperature of
6000 K.  This is equivalent to being in the center of an intensely
hot oven.  Of course the Earth is not fully surrounded by the Sun;
in fact the Sun fills only 4.76 millionths of the entire sky (including
both the night and day hemispheres).  The radiant energy received
at the Earth's surface is therefore "diluted" by the same
proportion. 
In radiative equilibrium the Earth must radiate back into space the same
amount of energy it absorbs from the Sun.  The laws of radiant energy
balance tell us that the average radiant energy emitted by the Earth is
proportional to the Earth's effective temperature to the 4th power. 
Thus the emission temperature of the Earth must be Te =
(Tsun times (0.00000476)) to the 1/4 power.  If there
were no atmosphere, and the Earth radiated energy like a theoretical
black body, the average temperature of the Earth would thus be
about 280 K.  This is much too cold to sustain abundant life, and
is less than the average at the worst of the ice ages.
Beginning sometime between the late 19th century and the mid 20th century
the Earth has entered a period of gradual warming.  A suspected major
contributor to this warming trend is the accumulation of so-called
greenhouse gases in the atmosphere: primarily carbon dioxide, methane, and
chloroflurocarbons (such as Freon).  These are all produced by man's
activities.  There are also other greenhouse gases such as water
vapor on which man has little effect, and which have not shown
rapid rises in concentration.  The evidence that these gases
have actually contributed to the warming trend has been controversial,
but in the past several years the evidence has become incontrovertable.
A part of the warming trend may be related to the end of the Little Ice Age, which cooled the
entire world until about 170 years ago.  Another possible contributor
to the warming is the dearth of major volcanic eruptions in the 20th
century.  The character of the present warming is, however, quite
different from warming spells of the past.  Moreover the effects of
the recovery from the Little Ice Age should have peaked before the
mid 20th century.  The last several decades of the 20th century
also witnessed a resumption of a "normal" level of volcanic activity,
so that influence can be ruled out for the past several decades. 
There is also some evidence that the weather patterns are changing. 
In the past, cycles of drought were generally associated with increased
warmth.  In the late twentieth century that correlation of
warmth and drought has been suppressed in many regions; in some
places, such as the U.S. Great Plains, the warming has been
accompanied by an increasingly moist climate.  This should
serve as a warning that large scale atmospheric circulation may
be changing, and that the results of warming may not be simple.
The future is uncertain only in the amount of warming to be
expected.  There is no disagreement among scientists that the
warming will continue, and that the greenhouse gases will play a larger
and larger role.  By the end of the twenty-first century, mid
latitudes are expected to warm by 2 to 6 C, or possibly even more
according to the most pessimistic predictions.  This may not seem
like much when averaged over a year, but such temperature differences
have accounted for major differences in the distributions of vegetation
and life on the Earth in the distat past.
The present warming trend began about the year 1840, with the
end of the Little Ice Age.  The cause of the Little Ice Age is not
understood, but it may related to fluctuations in the output of the
sun.  The warming trend was rather weak until the mid 20th century. 
The general trend was difficult to discern because the total change in
average temperature was far less than the daily and annual variations;
and several times the trend was briefly reversed by natural year-to-year
variations.  There were some cold years in the 1950's and 1960's
when it seemed that the Earth was in for a new round of cooling. 
Occasionally warnings were uttered that
the Earth might soon be subject to another Ice Age.  Then, in the
late 1960's the warming trend resumed.  That trend accelerated at
the end of the century.
The primary concern of scientists is the accumulation of so-called
"greenhouse gases." These include many familiar substances, both
natural and man-made.  Actually greenhouse gases such as oxygen
and carbon dioxide make life possible on Earth.  If there were no
atmosphere, the Earth would attain an equilibrium average temperature
too low to sustain life: a temperature much lower than experienced
at the worst of the ice ages.  The greenhouse gases raise the
temperature at the surface by preventing the escape of a portion of the infrared radiation that the Earth radiates back
into space.  The Global
Warming problem arises because the greenhouse gases over the past
several thousand years have achieved a relatively stable natural
balance, which has dictated the ways and places that man lives. 
Upsetting that balance, leading to a warming rate too fast for nature
and man's activities to compensate, could cause immense social and
economic difficulties.
Warming by itself might be endurable; and man and nature might cope by
migrating to other places; though that might require extreme poltical
adjustments.  But a true catastrophe is in
store if the Greenland Ice Cap and substantial portions of the Antarctic
Ice Cap were to melt.  The release of such huge amounts of fresh
water into the oceans could upset the oceanic circulation, and would
surely flood many of the world's large cities and coastal areas. 
Even a melting of part of those ice caps could raise the sea level
by many meters.
There are several principal greenhouse gases whose concentrations in
the atmosphere are increasing rapidly.  The greatest total
increases have been observed in carbon dioxide.  Carbon dioxide is
a natural product of combustion of carbon-rich fuels such as coal and
wood.  The burning of petroleum products produces less carbon
dioxide per energy unit, but the huge total amounts of petroleum
products burnt offsets that advantage.  The next most important
greenhouse gas for considerations of Global Warming is methane. 
Methane is a more efficient absorber of infrared radiation, and is much
more important per ton than carbon dioxide.  Methane is produced by
many natural processes.  Cattle are among the most prolific
producers of methane; their rich diet generates large amounts of
methane.  Another class of greenhouse gases that have raised great
concern are the chloro-fluorocarbons, including freon. 
Chloro-fluorocarbons are especially undesirable because they also cause
depletion of the stratospheric ozone layer. 
These are even more effective greenhouse gases than methane.  Fortunately the
release of Chloro-fluorocarbons into the atmosphere can be controlled
fairly easily, and international agreements are now in place to limit their
production.
If current trends continue, and if scientists are right in their
predictions about the effects of accumulating greenhouse gases, future
climates will be even more complex and more variable than present
climates.  The temperature increases that have been reported for
mid and high latitudes have generally pointed to warmer winters and
relatively unchanged summers.  While trees and many other plants
are extremely sensitive to the climatic conditions, the distribution of
heat and moisture over the year is more important than averages. 
As yet we have no simple way of predicting how plants will be affected
by a temperature increase as great as several degrees.
Though significant warming has been observed in the past 50 years, the
rate of warming has not yet been too great for plants to make appropriate
compensations.  That situation may not hold in the future if the
warming rate increases.  Another compensating factor is that the
twentieth century has seen increased rainfall and moisture in those places
where large amounts of the world's food is grown.  The warming
over much of North America, especially on the Plains, has been
accompanied by increased moisturecontrary to what might have been
deduced from the association of previous warming events and droughts.
While single species may adapt to Global Warming, the response of
symbiotic species and entire ecosystems may not keep up with the changes. 
The problem is complicated by the fact that many species have adapted to
the timing of another species; and those interrelated species may fall
out of syncronism.  What happens, for instance, if a bird has to
time the laying and hatching of eggs to take advantage of the flowering
of a particular plant or the emergence of particular insects?  Evidence
has been accumulating in recent years that such asyncronizations are
indeed occuringthough no species have yet been shown to be in
immediate danger.
There is no doubt that Global Warming will cause changes in the oceanic
and atmospheric circulation.  As a consequence, it has been
suggested that the 21st century will see more storms and violent
weather.  The effects of circulation changes will especially
affect the mountain regions of western North America, where there are
great geographical variations in rainfall.  The northern Great
Plains could also be strongly affected, since the weather there depends
so critically on how the atmospheric currents make it over (or around)
one of the longest north-south oriented mountain chain in the world.  The North
American Cordillera has a tremendous influence on the global climate,
since they are largely responsible for turning the winds and
establishing the high and low pressure systems that dominate northern
hemisphere weather.
In North America the effects of Global Warming will vary considerably
by region.  The desert Southwest may see warmer, drier summers and
winters.  The Southern Plains may experience elevated
temperatures, though no one can predict with confidence how the
rainfall will be affected.  In regions that already have warm
climates a relatively large increase in moisture may be needed to
compensate for hotter summers.  The cooler Northern Plains may
actually become more favorable for agriculture.  A longer growing
season could be beneficial there, if it is accompanied by increased
moisture.  Since the warming there may most noticeable in
the winter, more of the winter precipitation may be absorbed by
the soil, which could lead to increased moisture available to growing crops.
One of the most important concerns which has arisen in recent years is
the possibility that much of the Greenland and Antarctic Ice Caps could
melt, causing a rise in the sea level.  The rate of melting in
Greenland has increased alarmingly in recent years, but it is not yet
possible to assess the likely severity.  The total rise in sea level
since 1900 is still measured in millimeters; if that should become
meters the results would be devastating.  It does seem likely that
there will be a noticeable rise in the sea level long before the end of
the twenty-first century, leading to the need for large projects to
protect coastal cities.  A sea level rise of several meters
or more would flood many huge coastal cities, whose total population
exceeds 100 million.  The problem would only be exacerbated by the
expected increase in the frequency of large cyclonic storms.  The
expense of protecting cities like London or New York from such a sea
level rise is unimaginable.
The north polar sea ice has also been melting much faster than
expected.  This poses some serious ecological challenges, such as
the survival of polar bears.  It could also lead to increased use
of the Arctic Ocean by ships.  Drilling for oil in the Arctic
seabed has also been suggested.  It would be a great irony if one
of the principal effects of Global Warming were to be the increased
production of petroleum
The lack of progress in achieving world-wide reductions in the
production of greenhouse gases has led some scientists and engineers
to begin thinking about whether there are ways to remove the
greenhouse gases from the atmosphere.  There are many ways
that this might be achieved, though none of them are yet practical
on a large scale.
The most obvious way to eliminate greenhouse gases would be to scrub
them from the emissions at the source.  Scrubbing the gases seems
relatively easy; the big problem is what to do with the waste carbon
dioxide.  Carbon dioxide could be converted to relatively
inert limestone and buried; the logistics of this kind of operation are
quite staggering to contemplate.  Or, the carbon dioxide might be
injected deep underground. 
Some favor replacing coal and petroleum with renewable combustion
energy sources.  The objective would be to grow plants which absorb
carbon dioxide from the air.  Then, when the plant material is
burned, the net contribution to atmospheric carbon dioxide
is negligible.  The idea is sound, but logistically and
economically impractical at the present.
One of the more audacious schemes would to remove the carbon dioxide
from the atmosphere by constructing huge scrubbers that would intercept
the wind.  It is rather difficult to imagine how this could be
achieved without using a significant portion of the world's energy
to run the scrubbers.  Wallace Broecker, one of the leaders in
Global Warming research, makes the point that such a system would be
very expensive, but not more expensive than the billions of dollars of
infrastructure that are already in use to process garbage and other
such wastes.  Such a scheme would probably be much cheaper than
the cost of moving the cities of New York, London, Hong Kong, and
almost the entire nation of Bangladesh.
Another major deterioration of the global environment is the depletion
of the stratospheric ozone layers.  The stratospheric ozone
provides a beneficial shield against solar ultraviolet radiation. 
Ultraviolet radiation causes sunburn and skin damage to humans; it can
also have detrimental effects on vegetation and the food crops on which
we all depend.  There are, however, no significant direct effects
on the climate from depletion of stratospheric ozone.
Unfortunately the stratospheric ozone layer is easily destroyed by
reactions with certain compounds containing chlorine and fluorine, such as
freon.  The reactions destroy ozone without affecting the amounts
of the destructive agents.  Each molecule of the destructive agent
can catalytically destroy hundreds of ozone molecules.  Because of
their great efficiency, relatively small amounts of freon and related compounds
have caused a nearly total depletion of the ozone layer at the south
pole, and a considerable depletion of the ozone layer around the north
pole.  The effect extends to relatively low latitudes, so Canada
and northern Europe are especially susceptible to excessive ultraviolet
exposure.
The problem was recognized several decades ago, and international agreements now
limit the production and release of freon and similar compounds. 
It will take many years before the destructive agents are fully removed
from the atmosphere by natural processes, so the depletion of
stratospheric ozone will be a serious concern for many decades. 
In the meantime Canada and several European countries were the leaders
in establishing ultraviolet exposure standards, and setting up networks
of ultraviolet monitors.  Such monitors are in place in the United
States, and ultraviolet exposure indices are routinely issued along
with weather summaries.
There has been much controversy over the stratospheric ozone; some
scientists suspect that other phenomena, such as volcanic eruptions,
can also release ozone destroying gases.  Up to now, however the
principal culprit appears to be chlorofluorocarbons.
The effect of ultraviolet exposures on organisms are not well understood
because of strong latitude and seasonal effects.  While the dangers
cannot be dismissed, it should also be kept in mind that the increases in
ultraviolet exposure due to ozone depletion at mid latitudes are
equivalent to the increases that would result from moving several
hundred miles closer to the equator.
GREENHOUSE GASES
The "other" greenhouse gas, water vapor,
could have been a major factor in maintaining the high temperatures
of periods in the distant past, such as the period from the Jurassic
through the early Cenozoic.  The relative amounts of atmospheric
water in clouds and in the vapor phase depends strongly on the
atmospheric circulation.  In times when there was a reduced
difference between the equator and the poles, there might have been
more water vapor in the atmosphere, leading to a positive
feedback which raised the temperatures even more.
OF THE EARTH
Life is possible on
Earth only because of the presence of greenhouse gases in the
atmosphere.  These are quite transparent to the visible light from
the Sun, where a major part of the solar energy is concentrated. 
Greenhouse gases are especially effective in absorbing the outgoing
infrared radiation.  At temperatures below 500 K most of the radiation
emitted by the Earth is in the infrared region of the spectrum.  There
is only one broad spectral "window" at wavelengths of 8 to 13 microns
where the radiation can escape.  Radiation from the Earth's
surface, at a temperature of 280 K or more, is concentrated near
10 micronsin the far infrared.  Since much of the
outgoing radiation is blocked by the greenhouse gases, the fourth power
law tells us that the average surface temperature must be greater than
280 K in order to attain a balance with incoming solar radiation. 
The actual average is near 300 K = 27 C, sufficient to sustain
life on the Earth's surface.  The illustration shows how the greenhouse
gases cut off part of the spectrum of radiation that would otherwise
escape to space.
THE EARTH'S PRESENT CLIMATE
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