And now:Ish <[EMAIL PROTECTED]> writes:

Activist Mailing List - http://get.to/activist

Chill in the air

In the thin, frigid atmosphere beyond the global greenhouse it's
getting colder than ever.  And that, says Fred Pearce, spells big
trouble down on the ground.

New Scientist, 1 May 1999
Copyright New Scientist, RBI Limited 1999
<http://www.newscientist.com/ns/19990501/chillinthe.html>


THEY CALL IT the "ignoro-sphere" because so little is known about
it.  Even so, the upper atmosphere is becoming the hot topic in
the global warming debate.  But not because it is heating up.
The uppermost parts of our atmosphere are growing steadily colder
and, paradoxically, the greenhouse effect is being held to blame.

Until recently, scientists concerned about the greenhouse effect
have concentrated on the lowest layer of the atmosphere, the
troposphere.  This is understandable enough.  Although the
tropo-sphere is only 12 to 15 kilometres thick, it contains 75
per cent of the mass of the atmosphere.  It is where our weather
occurs, where our planes largely fly--and where there is growing
evidence that the accumulation of greenhouse gases is causing
global warming.

Wide-open spaces
~~~~~~~~~~~~~~~~
But in spatial terms, the troposphere is only a small part of the
atmosphere, and there is no reason to believe that the greenhouse
effect won't be just as important for the layers above the
troposphere--the wide-open spaces of the stratosphere, mesosphere
and thermosphere.  Already, researchers have found that the
changes occurring in these higher reaches are far greater than
those below.  And they are moving the opposite way: cooling
rather than warming.

Take the stratosphere, the layer immediately above the
troposphere.  This extends from around 15 kilometres to about 50
kilometres above the Earth's surface and contains the layer of
ozone that protects us from the worst of the Sun's ultraviolet
rays.  Last year researchers warned that if greenhouse gases
continue to accumulate in the atmosphere, cooling in the
stratosphere could accelerate ozone destruction and yield an
Arctic ozone hole as severe as the one over the Antarctic.

Meanwhile, we now find that the meso-sphere, between 50 and 90
kilometres up, has been cooling by as much as a degree every year
for the past 30 years--ten times faster than anyone had
predicted.  For some experts, such as Gary Thomas of the
Laboratory for Atmospheric and Space Physics at the University
of Colorado in Boulder, the cooling of the mesosphere may be the
"miner's canary".  He believes it is the latest, the biggest and
the most unequivocal signal that the global climate really is
changing.

It's around a decade since climate scientists began to calculate
how the greenhouse effect might influence the upper atmosphere.
Their logic then was simple: the troposphere is warmed largely
by heat radiating from the surface of the planet.  As the
concentration of greenhouse gases such as carbon dioxide and
methane increases in the atmosphere, more of this radiated heat
will be trapped close to the ground, warming the troposphere from
the bottom up.  The more this happens, the less heat will be
available for the rest of the atmosphere.  The upshot: as the
troposphere warms, the upper parts of the atmosphere cool.  This
effect, known as radiative cooling, would not matter if the heat
at the lower levels could gradually diffuse upwards.  The problem
is, it can't.

When warm air rises through the troposphere--in the huge storm
clouds of the tropics, for instance--it is forced to a halt at
the tropopause, where the troposphere ends and the stratosphere
begins.  This happens because the ozone in the lower stratosphere
is very efficient at absorbing solar heat directly, making the
air there warmer than in the upper troposphere.  The result is
a temperature inversion that blocks the air below in much the
same way that a layer of warm air will seal in a city's smog.
Warm air rising through the troposphere and entering the
stratosphere swiftly finds that it is no longer warmer than the
surrounding air.  It loses its buoyancy and cannot rise further.
So the heat trapped by greenhouse gases in the troposphere cannot
be redistributed, and the upper atmosphere cools down.

When researchers such as Nobel prizewinner Paul Crutzen of the
Max Planck Institute for Chemistry in Mainz, Germany, first
included this radiative cooling effect in their atmospheric
models a decade ago, it was considered little more than a
curiosity.  Now it's becoming clear that the cooling has real
implications for life on the Earth's surface.

In particular, stratospheric cooling contributes to thinning of
the ozone layer because the chemical processes that cause ozone
to be destroyed most quickly depend critically on temperature.
The ozone-eating chemicals from old fridges and air-conditioners
do their damage in conjunction with ice particles inside polar
stratospheric clouds that form below -80 degrees C.  This figure
happens to be close to the temperature in winter at the bottom
of the Antarctic stratosphere.  The Arctic is generally milder,
and until now has been spared the kind of severe ozone hole that
appears every year in the south.  But there are signs that the
Arctic is catching up.

"Stratospheric climate has changed considerably during the last
decades," says Hans-Friederich Graf, a senior scientist at the
Max Planck Institute for Meteorology in Hamburg.  In particular,
the Arctic has grown colder.  Researchers had expected some
cooling, but until recently they assumed that it would be more
than counterbalanced by the reduction in the quantity of
ozone-eating chemicals reaching the stratosphere, so that there
would be no increased threat to ozone.

Too cool
~~~~~~~~
What has caused alarm is the realisation that the cooling of the
stratosphere over the past five years has been greater than
predicted, especially over the polar regions in winter.  The
suspicion is growing that something besides radiative cooling is
at work lowering the temperature of the upper atmosphere.  So
what is happening? One factor is that despite the
temperature-inversion lid that the stratosphere puts on the
troposphere, the two zones are not entirely cut off from one
another.  The cold base of the Arctic stratosphere is
periodically heated up when slugs of warm, buoyant air from the
troposphere break through the barrier.  The fear now is that
these breakouts have become less frequent.  "In the past ten
years, there have been only two major warmings in the Arctic
during December-February," says Drew Shindell of NASA's Goddard
Institute for Space Studies (GISS) in New York.  "That is a big
change from the 1980s, when there were five."  Shindell thinks
global warming can be blamed directly for this and for the
resulting cooling in the regions where ozone holes form.

In April last year, Shindell published a paper in Nature (vol
392, p 589) describing a new analysis of how the atmosphere
responds to the greenhouse effect.  He suggested that the answer
to the extra stratospheric cooling over the Arctic lies in the
tropics.  Shindell's model predicts that as the world's
temperature rises, stronger upward currents of hot air over the
warm tropical oceans will create intense heating in the upper
troposphere there.  This will increase the difference in
temperature between the tropics and higher latitudes.

Increasing the temperature gradient from tropics to poles, he
calculates, will also increase the strength and speed of a strong
winter wind, known as the polar night jet, which encircles the
Arctic in the lower stratosphere.  Strengthening the polar night
jet isolates the cold Arctic air from surrounding influences.
The warmer tropics and cooler polar regions predicted by this
model are just what we have begun to see in the past decade, says
Shindell.  The radiative cooling has been amplified by changes
in atmospheric circulation caused by the greenhouse effect.

Shindell predicts that the Arctic vortex will become more like
its southern cousin in the next few years.  By 2020, he says, the
Arctic lower stratosphere will be 8 degrees C to 10 degrees C
colder than it would have been without the greenhouse effect.
As a result, ozone loss will be double what it would have been,
and the repair of the ozone layer as the world reduces emissions
of ozone-eating gases will be delayed.  While chlorine levels are
expected to peak in the stratosphere within the next five years,
Shindell says that ozone loss over the Arctic will continue to
rise for a further 10 or 15 years.  To add a frisson to those who
live in the North, Shindell's model runs predict that over
Greenland and northern Europe more ozone will be destroyed than
anywhere within the Antarctic ozone hole.

And where the stratosphere goes, the mesosphere seems to follow.
Though the evidence is more fragmentary, the same unexpectedly
intense cooling is extending into the mesosphere, only more so.

In February this year, specialists on these rarefied regions of
the atmosphere met in Pune, India.  Though everyone there
admitted that these are still early days, there was widespread
concern that not enough is known about how changes in the upper
atmosphere might affect the planet's inhabited zones.  The
director of the UN's World Climate Research Programme, Hartmut
Grassl, called the upper atmosphere his new number one priority.

The mesosphere is just about the least explored part of the
atmosphere, says John Plane of the University of East Anglia in
Norwich.  It is too high for research aircraft, which can reach
20 kilometres, and weather balloons, which can get to 45
kilometres.  But it is too low for satellites, which can't easily
be maintained in orbits below 140 kilometres.

Trickle down
~~~~~~~~~~~~
It has always been the coldest part of the planet.  At its base,
where it meets the warmer stratosphere, temperatures are about
0 degrees C.  But the thermometer falls to -100 degrees C or
lower at the top, the meso-pause, and a steady trickle of data
since the 1960s indicates that it is getting colder.

These data come from a variety of sources.  They include
instruments strapped to Russian rockets as they headed into space
in the 1960s, and two proxies for temperature: laser radar
(lidar) measurements of distinctive layers of metal atoms in the
mesosphere, and the height at which radio waves bounce back
towards the Earth.  There is also evidence that the mesosphere
is becoming more cloudy, a sign of colder temperatures that
Thomas discovered almost a decade ago.  Moreover, the atmosphere
seems to be shrinking--another sign of cooling aloft (see "The
sky is falling", p 28).  Thomas is still analysing the data, but
he announced at Pune that the mesosphere appears to have been
cooling by as much as 1 degree C a year over the past 30 years.

That the mesosphere is getting colder is not unexpected; like the
stratosphere it should be subject to cooling as the troposphere
warms.  It is the size of this cooling that has taken everyone
by surprise.  Ray Roble of the High Altitude Observatory at the
National Center for Atmospheric Research in Boulder, Colorado,
predicted in 1989 that a doubling of carbon dioxide and methane
levels in the atmosphere--which should take around a century at
the current rate--would cool the mesosphere by about 10 degrees
C and the thermosphere above it by some 40 degrees C.

Hot bursts
~~~~~~~~~~
Nobody knows why the mesosphere should be cooling so much faster
than this, says Thomas.  Given the size of the change, he
believes it is unlikely to be radiative cooling alone that is to
blame, or even a knock-on effect of the cooling stratosphere.
"The models predict a decreasing effect with height, whereas the
data show the opposite.  There are clearly other things
involved."

The most popular view in Pune was, once again, that circulatory
changes were amplifying the radiative cooling.  Plane suggests
that the cause could, confusingly, be bursts of warm air from the
stratosphere pushing upwards on the mesosphere during the summer
months when the atmosphere is exposed to long hours of sunlight.
As the air rises and the surrounding pressure decreases, it is
forced to expand.  This requires energy, and as the only energy
source is the heat in the air itself, it is forced to cool.  The
process is known as adiabatic cooling.

Of course, the importance of these upward surges of air is still
debatable, not least because nobody yet knows what could cause
them.  However, Thomas has a suggestion.  He thinks the culprit
may be planetary waves--huge atmospheric waves created by weather
systems in the troposphere, with wavelengths measured in
thousands of kilometres.  Although the waves are barely
perceptible at lower altitudes, they cause much stronger air
movements in the thinner air of the upper atmosphere.  In the
mesosphere they become unstable and "break", says Thomas.  The
energy that they create produces strong winds searing through the
mesosphere which suck up air from below, forcing it to cool
adiabatically.

Thomas and Plane both believe that changes in planetary waves may
be the mysterious driving force behind the massive cooling of the
mesosphere.  Are such changes caused by global warming in the
troposphere? We can't be sure, they say, but what else could it
be?

And there's an extra twist to the plot.  As in the stratosphere,
cooling in the mesosphere may be influencing the processes that
create ozone holes.  Plane warns that the air upwelling into the
mesosphere will eventually travel to polar regions in winter.
The air will then descend, he says, into the stratospheric polar
vortex, where it could help lower the temperature still further
and encourage the formation of polar stratospheric clouds.

Of course, many of these connections remain to be proved--this
isn't called the ignoro-sphere for nothing.  But whatever the
cause, the whole region does appear to be cooling at an alarming
rate.  And unexplained changes to planetary waves, jet streams
and a plethora of little-known features of upper atmosphere
circulation are probably amplifying the radiative cooling from
the greenhouse effect.

Should we care about events so far above our heads? Yes, we
should, says Thomas.  For one thing, they seem to be a sign that
global warming really has arrived.  For another, he says, they
could change the way we understand the troposphere.  "If we don't
get our models right for what is happening up there, we could get
things wrong down below."

The sky is falling
~~~~~~~~~~~~~~~~~~
PERHAPS THE MOST COMPELLING evidence that the upper atmosphere
is indeed cooling is the fact that it seems to be shrinking.
There, as anywhere else, cooler gases will take up less room.
And last year, scientists from the British Antarctic Survey (BAS)
in Cambridge reported in the Journal of Geophysical Research that
the sky is indeed falling in.  Measurements of the height of
certain layers in the mesosphere that reflect radio waves showed
that, as one American newspaper put it:  "Chicken Little may have
been right".  Over Antarctica, the top of the mesosphere has
descended by about 8 kilometres over the past four decades.
Similar observations have also been obtained over Europe.  The
measurements are not easy.  The boundaries of various parts of
the atmosphere expand and contract dramatically from day to night
as temperatures fluctuate.  There are also variations through the
seasons and in response to changes in solar activity and the
Earth's magnetism.  But Martin  Jarvis of BAS says the long-term
signal is now clear.  He has little doubt that radiative cooling
caused by the greenhouse effect, perhaps amplified by changes in
atmospheric circulation, is to blame.  "It is another warning
signal," he says.  With the greenhouse effect likely to
accelerate, few doubt that the atmosphere will continue to get
smaller.  Ray Roble from the NCAR in Boulder, Colorado, for
instance, calculates that the doubling of carbon dioxide levels
anticipated within the next century will bring the edge of space
20 kilometres closer.  He also believes the region above the
mesosphere, the thermosphere, will become less dense.  A
contracting atmosphere could have unpredictable effects, not
least for satellites.  Roble estimates the density of the
atmosphere at  any given height in the thermosphere, where some
satellites orbit, could be 50 per cent less within a few
decades--and a less dense atmosphere means less drag.  This would
disrupt satellites' orbits and could require complex redesigns.
More worryingly space debris will last longer before burning up
in the atmosphere, adding to the hazards for satellites and
astronauts.

Graphics:
Temperature ranges from the Earth's surface to the thermosphere

< http://www.newscientist.com/ns/19990501/chillinthe.html >
Reprinted under the fair use http://www4.law.cornell.edu/uscode/17/107.html
doctrine of international copyright law.
           &&&&&&&&&&&&&&&&&&&&&&&&&&
          Tsonkwadiyonrat (We are ONE Spirit)
                     Unenh onhwa' Awayaton
                  http://www.tdi.net/ishgooda/       
           &&&&&&&&&&&&&&&&&&&&&&&&&&
                             

Reply via email to