John Alexander Simpson

John Alexander Simpson
File:Jsimpson.JPG
Born	(1916-11-03)November 3, 1916 Portland, Oregon
Died
Citizenship	United States
Fields	physics
Institutions	Chicago University Laboratory for Astrophysics and Space Research (LASR) Washington D.C.
Alma mater	Reed College New York University
Doctoral students	Sam Treiman
Known for	Cosmic Ray Nuclear physics high-energy astrophysics Space Exploration
Notable awards	Gagarin Medal (1986) Bruno Rossi Prize (1991) Arctowski Medal (1993) Leo Szilard Lectureship Award (1999) William Bowie Medal (2000)

John Alexander Simpson (November 3, 1916 – August 31, 2000) worked as an experimental nuclear, and cosmic ray physicist who was deeply committed to educating the public and political leaders about science and its implications. The year he died, his instruments in space had been sending data back for nearly 40 years. Simpson spent his career as an instructor and researcher for the University of Chicago Physics department. His research continued up until a few weeks prior to his death on August 31 of 2000.

He is known for inventions such as the gas flow a-particle proportional counter for measuring plutonium yields in the presence of high intensity fission products, and the neutron monitor. And also for having several of the instruments he created launched into space.

John A. Simpson died at age 83. His death was caused from a case of Pneumonia in which he contracted in the hospital following a successful heart surgery, and he is survived by his wife Elizabeth, and by his two children Mary Ann and Simpson from his first marriage.

Early life

Born in Portland, Oregon, Simpson was an accomplished clarinetist and saxophonist in his early years, receiving recognition in high school with an award for his virtuosity. He received an AB degree from Reed College in 1940, where he became interested in the history of science and technology spanning from the Greeks and Romans to the Middle Ages, to the most recent discoveries in astronomy and physics. He obtained an MS from New York University in 1943, and a Ph.D a year later. It was at New York University in 1943 when Simpson first got his invitation to become employed at Chicago University. Volney Wilson, an administrator at the Metallurgical Laboratory of the university had asked him to come help invent instruments for measuring high levels of radioactivity. It took much convincing, but Simpson finally agreed to help.

Research

Simpson began his professional career as a physicist in 1943 where he acted as a group leader on the Manhattan Project. The Manhattan Project was the codename for a United States project with the United Kingdom and Canada conducted during World War II to develop the first atomic bombs. It was common for government to recruit physicists during World War II for such tasks. Simpson had taken up the offer after recognizing the social and human implications of nuclear energy and wanted to partake in its development. Because of this, Simpson became a founding member and first chairman of the Atomic Scientists of Chicago, founded two years after the start of his career in August 1945, a day after the United States dropped the atomic bomb on Hiroshima. He was also a co-founder that same year of the Bulletin of the Atomic Scientists. This bulletin's aim was to spell out the implications of the atomic bomb, as well as to provide rational courses of action in response to the implications. In the October 29, 1945 issue of Life, Simpson, along with Eugene Rabinowitch spoke about their involvement with nuclear energy, and said that scientists for the first time had recognized a moral responsibility to carry the warning of the danger of any further use of nuclear weapons. He felt that scientists and engineers could no longer remain aloof from the consequences of their work.

This same year Simpson began his tenure as a faculty member at the University of Chicago as a physics instructor, and remained there throughout his career partaking in research as well until shortly before his death in August 2000. In 1945 also he was able to work as an unofficial adviser to Connecticut Senator Brien McMahon after taking a leave of absence from the university. As part of the university faculty, Simpson was able to invent and patent a gas flow a-particle proportional counter for measuring plutonium yields in the presence of high intensity fission products. He had come up with the idea to pipe the plutonium-bearing gas through the counter itself.

Simpson has 15 patents under his name which include the multiwire proportional counter, a device that assists in improving reading speed and accuracy, and the Neutron monitor. Nancy Farley Wood worked with Simpson and is credited with the development and production of the radiation detectors for the laboratory.

In 1946 Simpson developed a special interest in cosmic rays, which very little was known about at the time as the field which was still in the process of being established, including their origin. Beginning with investigations pertaining to the cosmic ray neutrons in the lower atmosphere, Simpson was there from the beginning developmental phases of the field, and contributed significantly throughout the years to its development with his scientific investigations. Simpson's contributions were unique in that he somehow accomplished his work in a way which boosted the accomplishments and careers of others around him such as graduate students, research associates and other faculty. In 1955 he gave Eugene N. Parker a job as a research associate in the Enrico Fermi Institute of the University of Chicago, and his progress was largely a consequence of Simpson's continued support. His research on cosmic ray neutrons in the lower atmosphere was developed upon its founding by Serge Korff before World War II. Simpson in his research contributed the discovery that the latitude effect seen with neutrons is around 20 times greater than with ionization chambers in 1949. In 1951 he found that the time variations are much greater as well. He had recognized the potential of the neutrons and the lower energy cosmic ray particles for exploring the causes of the time variations. That year he also invented the neutron monitor to fulfill the need for a stable ground-based neutron detector. In doing so, he established neutron monitor stations at various locations including Peru, Huancayo, Mexico, Mexico City, New Mexico, Sacramento Peak, Colorado, Climax, and Chicago Illinois.

In 1954 and 1955, Simpson explored the global and time variations of cosmic rays around the world at these neutron monitor stations. In 1956, the giant cosmic ray flare provided for Simpson the first direct glimpse of the state of things in interplanetary space. At this point the scientific community surrounding cosmic rays and solar activity had grown largely, and for the International Geophysical Year (1957–58) Simpson was one of 12 other scientists responsible for organizing and coordinating the international program, helping to make it a huge success.

At the end of 1957 after the launch of Sputnik by the Soviet Union, Simpson, realizing the necessity for the U.S. to send instruments into space, outlined the scientific situation and his plans for such activity to University chancellor Lawrence Kimpton. Kimpton granted Simpson $5000 to get the project off the ground, and partnered with Peter Meyer to develop small lightweight particle detectors suited for the space environment. Simpson's first particle detector was launched in 1958 on spacecraft Pioneer 2.

In 1962 Simpson and Professor Peter Meyer established the Laboratory for Astrophysics and Space Research (LASR) which was built within the Enrico Fermi Institute at the University of Chicago. NASA contributed towards the laboratory and funded a building for LASR which was completed in 1964. In the laboratory instrument development and space research were consolidated under one roof, along with theoretical research connected with the results of the ongoing research and space experiments.

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John A. Simpson and James Van Allen, Pioneer 10/11 press conference on magnetic field and radiation belts at Jupiter, January 27, 1973.

In 1965 Simpson, along with his students and co-workers, built the first cosmic ray (energy particle) detectors to visit Mars. In 1973 it was the first to visit Jupiter, in 1974 Mercury, and in 1979 Saturn. Jupiter's mission detected the relativistic (3-30 MeV) electron population for the first time which the planet was emitting. This first recognized the electrons contained within the Jovian magnetosphere and then the escaping electrons at distances of at least 1 AU. Simpson's detection in 1974 is what first established that the magnetic fields being observed at Mercury were not being carried from the Sun by the impacting solar wind, but in fact belonged to the planet itself. Simpson had been helping to develop the mission from concept since 1959. Also, in 1980, his detection of a tiny gap in the distribution of energetic particles trapped in the magnetic field of Saturn indicated to them the presence of a previously undetected small moon there orbiting at that position in space and absorbing particles which would otherwise be found there were there no disruption. Subsequently, scientists became able to identify Saturn's moon optically. In 1976 and 1982 Simpson also detected bursts of energetic particles associated with the passage of shock waves in the solar wind, and provided evidence that the transition serves as an efficient accelerator of particles, and provided a basis for further studies.

In 1970 Simpson, William Dietrich and John David Anglin discovered that some impulsive sun flares produce energetic particles among which Helium-3, a light non-radioactive isotope of helium with two protons and one neutron, is at least ten times more abundant than Helium-4, a non-radioactive and light isotope of helium. On Earth, Helium-4 is what makes up about 99.986% of the helium here. In 1973 his instruments on Pioneer 10 and 11 indicated a cosmic ray intensity increase of about 1 percent per AU. In 1975 he found that during the low point of activity three years prior, the abundance of cosmic ray helium was strangely enhanced at these very low energies, as opposed to it dropping off with declining energies like the protons do, toward zero energy.

In the 1975s and 1977s Simpson discovered the fact that Beryllium-10 nuclei are scarce in cosmic rays, and that that scarcity indicates that they have been around for about 2 x 10⁷ years. This led him to conclude that cosmic rays pass freely between the gaseous disk and the extended magnetic halo portion of the galaxy, where the ambient gas density is more like 10⁻² atoms/cm³ or less.

In the 1980s Simpson Simpson and A. J. Tuzzolino developed the dust flux monitor instrument which involved a thin sheet of plastic which was polymerized in the presence of a strong electric field perpendicular to the plane of the plastic, and then electrically polarized carrying a positive electric charge on one of its surfaces and a negative charge on the other. The way it operated was such that a dust particle or heavy nucleus penetrating through the sheet first vaporizes in a small area releasing the charges, then the electrical signal indicates the location and size of the hole in the plastic which is then calibrated to give information on its speed and size. These calibrations took place from 1985 until 1989. Simpson's device was used on spacecraft Vega 1 and Vega 2 to Halley's comet in 1986, and earned him the Gagarin Medal for Space Exploration that year for his contribution towards the success of the Vega mission, as his instruments had been the only ones from the United States to encounter the comet.

Accomplishments

John Alexander Simpson is known for inventions such as the gas flow α-particle proportional counter for measuring plutonium yields in the presence of high intensity fission products, and a neutron monitor. His obituary in The Guardian noted that he was one of the most prolific inventors of scientific instruments for space exploration. In 1958 his first created instrument was launched into space, and the last two were launched in 1999. One on board the Stardust, met up with Comet Wild-2, a frozen snowball one and a half miles in diameter in 2004.

In 1959 Simpson was elected to the National Academy of Sciences, in 1968 he held the first Ryerson Chair and was made Distinguished Service Professor at his university, in 1974 was the first to be appointed to the Compton Chair, and in 1986 he became Emeritus. Simpson is the recipient of the 1986 Gagarin Medal for Space Exploration for his contribution towards the success of the Vega mission, which sent satellites to Halley's comet earlier that year. In 1991 he was awarded the Bruno Rossi Prize by the American Astronomical Society for his contributions towards high-energy astrophysics, and in 1993 was awarded the Arctowski Medal of the National Academy of Sciences. In 1999 he was awarded the Leo Szilard Lectureship Award for his role in educating scientists, members of the United States Congress and the public on the importance of civilian control of nuclear policy and his critical efforts in planning and execution of the International Geophysical Year. In 2000 he was also additionally awarded the William Bowie Medal which is the highest award given by the American Geophysical Union, for his extensive explorations of the cosmic rays and other energetic particles that our planet is continually bombarded by. He is known as having been an outstanding professor, having throughout the course of his academic career supervised the research of 34 doctoral students, many who are now leaders in the space sciences. Simpson has also provided lectures to the public using funds in 1974 which came from his Compton Chair in an attempt to reach a larger audience with his research. In 1982 he also established and became the first chairman of the Universities Space Science Working Group located in Washington, D.C. in order to represent the space science laboratories in their dealings with congress and NASA