Solar Physicist Art Walker Dies at 64
A memorial service is scheduled for Thursday, May 3, from 3:00
to 4:00 p.m. in Stanford Memorial Church.
Arthur
Bertram Cuthbert Walker II, professor of physics and applied physics at Stanford
since 1974 and pioneer in the use of X-rays and thin films to study the solar
corona, died April 29 at his home on campus after a long battle with cancer. He
was 64.
A memorial service is scheduled for Thursday,
May 3, from 3:00 to 4:00 p.m. in Stanford Memorial Church. A reception will
follow at the Stanford Faculty Club.
"Walker
was best known for developing, with [materials scientist] Troy Barbee, a whole
new set of X-ray optics with which the two of them formed some wonderful and
scientifically important images of the sun, "said Malcolm Beasley, dean of
the School of Humanities and Sciences and a colleague of Walker's in the Applied
Physics Department. "Art
was also a leader of the community of African-American physicists, and a very,
very respected conscience of us all in diversifying the academy - not to mention
a role model to many students."
Largely due to Walker's efforts, Stanford led
the nation's major research universities in educating graduate students from
underrepresented groups in physics. Astronaut Sally Ride, America's first woman
in space, was among Walker's graduate students. The month before his death, he
presided over the National Conference of Black Physics Students, hosted this
year at Stanford.
Walker's recommendations to Congress were
instrumental in creating a national solar observatory. In 1986, President Ronald
Reagan appointed him to serve on the commission that investigated the space
shuttle Challenger explosion and ultimately concluded that the disaster was
preventable.
Walker was born in Cleveland on Aug. 24, 1936.
He received a baccalaureate degree in physics with honors from Cleveland's Case
Institute of Technology in 1957. He earned a master's degree in 1958 and
doctorate in 1962 from the University of Illinois with a dissertation on the use
of radiation to produce the particles that bind protons and neutrons together in
the atomic nucleus.
Walker joined the U.S. Air Force in 1962 as a
first lieutenant and was assigned to the Air Force Weapons Laboratory, where he
developed instrumentation for an experiment that involved rocket launch of a
satellite to measure Van Allen belt radiation in the Earth's magnetic field.
Upon completing his military duty in 1965, he
joined the Space Physics Laboratory of the Aerospace Corporation, where for nine
years he conducted pioneering physics experiments to study the sun and upper
atmosphere of the Earth.
After arriving at Stanford, Walker directed the
student observatory and taught astronomy courses including the popular Applied
Physics 15 ("The
Nature of the Universe") and Physics 50 ("Observational
Astronomy").
In the 1980s, senior research associate Troy
Barbee at Stanford's Center for Materials Research created multi-layered thin
films that could capture images produced by hot solar gas so energetic that it
spewed radiation in the extreme ultraviolet end of the spectrum. In 1987, Walker
used these materials to develop telescopes and complex instrumentation, which he
mounted on rockets and launched into space to capture the first detailed
pictures of the sun's outermost atmosphere, or corona. Images from the first
flight of Walker's solar telescope appeared on the cover of Science magazine on
Sept. 30, 1988.
"Art
Walker obtained the first soft X-ray images of the sun,"
recalled Bob Byer, chair of the Department of Applied Physics. "The
images showed spectacular surface details of the sun, including flares, bubbles
and gas jets. Art was just thrilled with these images. I will never forget his
face when he showed us the first images."
Walker launched 14 telescopes in NASA's first
Multi-Spectral Solar Telescope Array (MSSTA) flight in 1991 and 19 telescopes in
the second flight. Since a telescope's flight filter only lets in one wavelength
of light at a time - and each wavelength represents a different temperature -
arrays of telescopes allow researchers to look at different temperatures
throughout the sun and gain a greater understanding of solar activity. Walker's
technique has since been used in NASA's Chandra X-ray Observatory, to study the
nighttime sky, and in a worldwide chain of ground stations called the Global
Oscillation Network Group (GONG), to study solar activity.
On Sept. 15, 2000, the departments of Physics
and Applied Physics and the African and Afro-American Studies Program hosted a
celebration to honor Walker's "innovative
research and inspiring teaching in physics, particularly in solar physics, as
well as his exemplary contributions to the black community at Stanford,"
said psychology Professor Ewart Thomas. At the celebration, NASA officials
surprised Walker with a Distinguished Public Service Medal in recognition of
four decades of distinguished scholarship, achievements in experimental space
sciences and extensive service to NASA and the nation on many advisory and
review boards.
Walker is survived by his wife, Victoria T.
Walker, of Stanford; daughter Heather M. M. Walker of Los Altos Hills; stepsons
Nigel D. Gibbs of Los Angeles and Eric D. Gibbs of Temecula; and four
grandchildren. He was also beloved by many cousins, other relatives and friends,
and members of the Sigma Pi Phi fraternity (Gamma Chi Boule), of which he was a
member of long standing.
In lieu of flowers, donations may be sent to the
A.B.C. Walker II Memorial Fund for the greater inclusion of ethnic minorities
and women in the sciences. Checks should be made payable to Stanford University
and sent to:
Department of Physics
C/O
Jenifer Conan-Tice
Stanford University
Stanford, CA 94305-4060.
Profile on Art Walker at: http://www.stanford.edu/dept/news/pr/00/walkerprofile1011.html
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