Degaussing

Interviewed by
David DeVorkin
Interview date
Location
Indiana University Department of Astronomy, Bloomington, Indiana
Abstract

Early life and education in Manchester; World War I; spectroscopy work at Oxford under Frederick A. Lindemann; visits to Gottingen and Berlin in 1920s; ideas on stellar energy source and stellar structure; work and teaching at Rutgers (1929-1937); World War II research on de-Gaussing, ballistics; moves to Greenwich, then Herstmonceaux observatories; their administration and instruments; solar eclipse work; general relativity theory; return to U.S. Also prominently mentioned are: Herbert Jefcoate Atkinson, Irmin von Holton Atkinson, Mary Kathleen Jane Ashe Atkinson, Niels Henrik David Bohr, John Edward Campbell, Arthur Stanley Eddington, George Gamow, I. O. Griffith, Fritz G. Houtermans, Edwin Powell Hubble, James Hopwood Jeans, H. Spencer Jones, Walther Nernst, Henry Norris Russell, Frederick Soddy, Richard van der Riet Woolley; Aberdeen Proving Ground, Balliol College of University of Oxford, Great Britain Admiralty, Indiana University, Royal Astronomical Society, Royal Greenwich Observatory, United States Proving Ground at Aberdeen, MD Ballistics Research Laboratory, and Universitat Gottingen Observatory.

Interviewed by
Robert Smith
Interview date
Location
Flagstaff, Arizona
Abstract

Family background, early life in Brooklyn and Detroit, high school; undergraduate studies at University of Michigan, switch from mathematics to physics. Graduate work at Michigan, 1931-1933; thesis research combines quantum mechanics and infrared spectroscopy. Difficulty finding academic job during Depression; works for Lowell Observatory while at Michigan, 1933-1936; devises long-path absorption cell, research in infrared spectrum of earth's atmosphere. Joins faculty of Johns Hopkins University (Gerhard Dietz), 1935-1936. To Lowell Observatory (Roger Lowell Putnam, V. M. Slipher, E. C. Slipher, C. O. Lampland), 1936; living conditions, constructing the prism spectrometer, studies in earth atmosphere, atmospheric chemistry of Venus, discovery of 20 micron window (Carl Sagan); constructing the grating spectrometer. Adel forced out of Lowell; problems encountered by Adel at Lowell; anti-Semitism. Wartime work in Washington, DC, submarine degaussing (Arthur Bennett), summer 1942. Returns to Michigan, 1941-1945, joins program for training military meteorologists; research to determine causes for failure of lcm radar. Joins McMath-Hulbert Observatory, 1946, discusses staff, autocratic research style. Accepts Air Force contract to build lab at Holloman Air Force Base, Alamagordo, NM to examine effective radiation temperatures of ozone, 1947-1948. Joins faculty of Arizona State College in Flagstaff, 1948; fate of the ozone lab. Air Force funding of Atmospheric Research Observatory at Arizona State College, 1950, establishing a database of ozone research; Yerkes Observatory Symposium, 1947; Gerard Kuiper, Otto Struve. Adel's place in infrared astronomy. Also prominently mentioned are: Ernest F. Barker; Professor Dennison; Edward Epstein; Henry Giclas; Leo Goldberg; Percival Lowell; Ohren Mohler; Henry Norris Russell; Edward Teller; George Uhlenbeck; Harry Wexler