Earth's Smoke Viewed From Space
NASA
RESEARCHERS CLOSELY MONITORED this year's fires in Mexico, using
the unique perspective of space, to see how smoke from natural and
human-induced fires contribute to global air pollution and climate
changes. Since the beginning of the Mexican fires in late March
and early April of this year, NASA atmospheric researchers used
the Total Ozone Mapping Spectrometer (TOMS) to observe the smoke
aerosols emitted by the fires.
The TOMS instrument has the ability to obtain daily images of
the amount of smoke present in any atmospheric conditions anywhere
in the world. TOMS makes 35 measurements every eight seconds, each
covering 30 to 125 miles wide, from Earth's surface to the atmosphere's
top.
Fires such as those in Mexico interest scientists because smoke
contributes to the overall regional air pollution levels that can
impact the quality of air that humans breathe, especially those
with asthma. Increased smoke concentration from human-induced fires
could contribute to global climate change.
The current NASA-developed TOMS instrument is a second-generation
backscatter ultraviolet ozone sounder. It measures ozone indirectly
by comparing ultraviolet light emitted by the Sun to that scattered
from Earth's atmosphere back to the satellite at six wavelengths.
Backscattered radiation is solar radiation that has penetrated Earth's
lower atmosphere and is then scattered by air molecules and clouds
back through the stratosphere to the satellite sensors. Along that
path, a fraction of the ultraviolet is absorbed by ozone.
By comparing the amount of backscattered radiation to observations
of incoming solar energy at identical wavelengths, scientists can
calculate Earth's albedo, the ratio of light reflected by Earth
compared to that which it receives. Changes in albedo at the selected
wavelengths can be used to derive the amount of ozone above the
surface.
The fires started in southern Mexico and northern Guatemala near
the end of March 1998. Some fires were started as part of the annual
clearing of agricultural fields; others started naturally with lightning
because of the extremely dry conditions.
The small particles, called aerosols, can affect the amount of
energy reaching Earth's surface by reflecting and/or absorbing sunlight.
Smoke aerosols also can act as small particles on which clouds can
form. Clouds containing smoke aerosols are believed to reflect and
absorb energy in different ways than clouds formed from natural
particles, such as dust or sea salt.
"Shortly after the fires started, we noticed the huge increase
in the amount of aerosols (in this case smoke) in the region,"
said Dr. Jay R. Herman, an atmospheric scientist at NASA's Goddard
Space Flight Center in Greenbelt, Maryland. Large amounts of smoke
extended into Florida, Texas, New Mexico, California and Wisconsin.
On May 16, the smoke plume extended across the eastern United States,
passing through Ohio and into southern Canada.
Because of the difficulties in extinguishing the fires, some large
smoke plumes are lingering in Mexico. The smoke tends to extend
from the ground up to an altitude of about three to four kilometers
(1.8 miles) and to follow the prevailing winds. Because of wind
shear in this altitude range, there is frequently more than one
plume, with smoke blowing from west to east and from south to north.
The fires and accompanying smoke lasted through the middle of
June, when rain finally relieved the drought conditions associated
with El Niño weather patterns. Since then, there have been
major fires observed in Russia and South America, as well as extraordinary
amounts of Saharan dust blowing across the Atlantic into the Caribbean
and across the southern United States and Mexico.
TOMS is part of NASA's Earth Science Enterprise, a long-term,
coordinated research effort to study Earth as a global system. The
TOMS program is managed by the Goddard Space Flight Center for NASA's
Office of Earth Science in Washington, D.C.
For more information, contact Dr. Jay R. Herman at Goddard Space
Flight Center.
Call: 301/286-7821, E-mail: Herman@TPARTY.gsfc.nasa.gov Please
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