Sydney Chapman
Sydney Chapman 1888–1970
Born	(1888-01-29)29 January 1888 Eccles, Greater Manchester, England
Died	16 June 1970(1970-06-16) (aged 82) Boulder, Colorado, U.S.
Alma mater	University of Manchester University of Cambridge
Known for	Chapman cycle Chapman function Chapman–Kolmogorov equation Chapman–Enskog theory
Awards	Fellow of the Royal Society (1919)[1] Smith's Prize (1913) Adams Prize (1928) Royal Medal (1934) Chree Medal and Prize (1941) De Morgan Medal (1944) William Bowie Medal (1962) Copley Medal (1964) Symons Gold Medal (1965)
Scientific career
Institutions	University of Manchester University of Cambridge Imperial College London University of Oxford The Queen's College, Oxford Royal Observatory, Greenwich, University of Colorado
Academic advisors	G. H. Hardy[2]
Doctoral students	Franz Kahn[3] George Frederick James Temple[2] Syun-Ichi Akasofu

Sydney Chapman FRS (29 January 1888 – 16 June 1970)^[1] was a British mathematician and geophysicist.^[4] His work on the kinetic theory of gases, solar-terrestrial physics, and the Earth's ozone layer has inspired a broad range of research over many decades.^{[2][5][6][7][8]}

Education and early life

Chapman was born in Eccles, near Salford in England and began his advanced studies at a technical institute, now the University of Salford, in 1902.^[9] In 1904 at age 16, Chapman entered the University of Manchester. He competed for a scholarship to the university offered by his home county, and was the last student selected. Chapman later reflected, "I sometimes wonder what would have happened if I'd hit one place lower."^[5] He initially studied engineering in the department headed by Osborne Reynolds. Chapman was taught mathematics by Horace Lamb, the Beyer professor of mathematics, and J. E. Littlewood, who came from Cambridge in Chapman's final year at Manchester. Although he graduated with an engineering degree, Chapman had become so enthusiastic for mathematics that he stayed for one further year to take a mathematics degree. Following Lamb's suggestion, Chapman applied for a scholarship to Trinity College, Cambridge. He was at first awarded only a partial scholarship as a sizar (meaning that he obtained financial support by acting as a servant to other students), but from his second year onwards he received a full scholarship. He graduated as a wrangler in 1910.^[6] He began his research in pure mathematics under G. H. Hardy, but later that year was asked by Sir Frank Dyson to be his chief assistant at the Royal Greenwich Observatory.

Career and research

From 1914 to 1919, Chapman returned to Cambridge as a lecturer in mathematics and a fellow of Trinity. He held the Beyer Chair of Applied Mathematics at Manchester from 1919 to 1924, the same position as had been held by Lamb, and then moved to Imperial College London. During the Second World War he was Deputy Scientific Advisor to the Army Council.^[6]

In 1946, Chapman was elected to the Sedleian Chair of Natural Philosophy at Oxford, and was appointed fellow of The Queen's College, Oxford. In 1953, on his retirement from Oxford, Chapman took research and teaching opportunities all over the world,^[4] including at the University of Alaska and the University of Colorado, but also as far afield as Istanbul, Cairo, Prague, and Tokyo. As the Advisory Scientific Director of the University of Alaska Geophysical Institute from 1951 to 1970, he spent three months of the year in Alaska, usually during winter for research into auroras.^[10] Much of the remainder of the year he spent at the High Altitude Observatory in Boulder, Colorado.^[11]

Chapman's most noted mathematical accomplishments were in the field of stochastic processes (random processes), especially Markov processes. In his study of Markovian stochastic processes and their generalizations, Chapman and the Russian Andrey Kolmogorov independently developed the pivotal set of equations in the field, the Chapman–Kolmogorov equations. Chapman is credited with working out, in 1930, the photochemical mechanisms that give rise to the ozone layer.^[11]

Chapman is recognised as one of the pioneers of solar-terrestrial physics.^[4] This interest stemmed from his early work on the kinetic theory of gases. Chapman studied magnetic storms and aurorae, developing theories to explain their relation to the interaction of the Earth's magnetic field with the solar wind. He disputed and ridiculed the work of Kristian Birkeland and Hannes Alfvén, later adopting Birkeland's theories as his own.^[12][13] Chapman and his first graduate student, V. C. A. Ferraro, predicted the presence of the magnetosphere in the early 1930s. They also predicted characteristics of the magnetosphere that were confirmed 30 years later by the Explorer 12 satellite.^[5]

In 1940, Chapman and a German colleague Julius Bartels published a book in two volumes^[14][15] on geomagnetism, which was to become the standard text book for the next two decades.^[5] In 1946 Chapman coined the term: Aeronomy, which is used today to describe the scientific field of high-altitude research into atmosphere/space interaction.

From 1951 to 1954, Chapman was president of the International Union of Geodesy and Geophysics (IUGG).

Chapman was President of the Special Committee for the International Geophysical Year (IGY). The idea of the IGY stemmed from a discussion in 1950 between Chapman and scientists including James Van Allen. The IGY was held in 1957–58, and resulted in great progress in fields including Earth and space sciences, as well as leading to the first satellite launches.

Personal life

In 1970, Chapman died in Boulder, Colorado, at the age of 82.^[6]

References