SAM II, SAGE I, SAGE II, SAGE III (passive
solar and lunar occultation), and LITE (shuttle-
borne lidars). He is continuing his work as an
endowed professor at the Center for Atmospheric
Sciences at Hampton University in Hampton,
Virginia.
5 McIntyre, Michael Edgeworth
(1941– )
English
Physicist
Michael McIntyre was born on July 28, 1941, in
Sydney
, Australia, to Archibald McIntyre, a uni-
versity research neurophysiologist, and Anne
McIntyre, a painter. As a youngster, McIntyre’s
education was international, starting in nursery
school in Sydney, Australia. He then attended
P.S. 16 in Yonkers, New York, in 1947, then the
Newnham Croft School in Cambridge, England,
the following year, followed by George St. Nor-
mal School, McAndrew Intermediate School,
and King’s High, all in Dunedin, New Zealand,
from 1949 to 1958. His early childhood interests
included classical music (violin, piano, composi-
tion), model aircraft, radio, and electronics. At
age five, seeing what Beethoven’s Eighth Sym-
phony looked like on an oscilloscope made a deep
impression. He found occasional work as a local
professional musician during his college years,
was concertmaster of the New Zealand National
Youth Orchestra from 1960 to 1962, and was
later to give concerts at the Wigmore Hall and
Purcell Room, top professional venues in Lon-
don, England. He easily could have made a life in
music, but his interests turned to science.
He attended the University of Otago in
Dunedin, New Zealand, from 1959 to 1962,
receiving a B.Sc. (First-class honors) in mathe-
matics in 1963. That same year, he became assis-
tant lecturer in mathematics at Otago. In 1967,
he earned his Ph.D. in geophysical fluid dynam-
ics at Cambridge University, his thesis titled
“Convection and baroclinic instability in rotat-
ing fluids.”
McIntyre and his coworkers have made sev-
eral notable contributions to atmospheric science
research, centered around understanding the
fluid dynamics of the Earth’s atmosphere, with
emphasis on the stratosphere, the layer lying
between altitudes of about 10 to 50 kilometers.
The stratosphere contains the bulk of the ozone
shield that protects the Earth from harmful solar
ultraviolet radiation. McIntire’s research has
helped to explain why the strongest humanmade
ozone depletion occurs in the Southern Hemi-
sphere in the form of the so-called Antarctic
ozone hole, even though the chlorofluorocarbons
and other chemicals known to cause it enter the
atmosphere mainly in the Northern Hemisphere.
Part of the answer is that the chlorofluorocarbon
molecules go on epic journeys, circumnavigating
the globe and visiting both hemispheres many
times in the lower atmosphere before eventually
arriving in the stratosphere.
Measured concentrations of chlorofluorocar-
bons show that they are almost uniformly mixed
in the lower atmosphere. Air carrying chloroflu-
orocarbons is gradually pulled up from the lower
atmosphere into the tropical stratosphere and
then pushed poleward and back downward into
the lower atmosphere by an inexorable, persistent
fluid-dynamical process in the stratosphere called
gyroscopic pumping.
This is a global-scale pumping action and is
called gyroscopic because it depends on the Earth’s
spin. Complicated, fluctuating fluid motions,
which can be compared to giant breaking waves,
conspire to push air westward. When air is pushed
westward, the Coriolis effect from the Earth’s spin
tends to deflect it poleward. A movie of the gyro-
scopic pump in action in the real stratosphere
can be viewed at www.atm.damtp.cam.ac.uk/
people/mem/.
The instrument that produced the movie in
this case uses a set of highly sensitive infrared
spectroscopes that are cooled with liquid helium.
McIntyre, Michael Edgeworth 113