Family background, education, and emergence of scientific orientation. Undergraduate years at Wellesley College (1912-1916); description of physics department. Assistant examiner in U.S. Patent Office during World War I. At MIT under E.B. Wilson as graduate student and laboratory assistant, then lab instructor (1920-24). Returned to MIT for doctoral work in 1928. Mathematical physics thesis under Norbert Wiener, while teaching at Wellesley. Depression years brought teaching position at Wilson College (1930-43), used Wellesley as model. Work on Zeeman Pattern earns her Guggenheim Fellowship (1949-50) at MIT and European labs. World War II years as head of OSRD British Report Section. Returned to Wilson (1945-56), worked part-time at National Science Foundation (1953-56). Retirement years including affiliation with U.S. Army and spectroscopic work at Harvard College Observatory. Comments on women in physics in U.S., her own opportunities, and teaching in general.
Extensive interview covering early life and family in New York and Maine; schooling and early interests in astronomy in New York City; observing Halley's comet in 1910; World War I and college years at Harvard University majoring in chemistry; medical degree from Cornell University; contacts with Henry Norris Russell and Harlow Shapley, and decision to move into astronomy; graduate work at Princeton; postdoctoral work and staff position at Mt. Wilson in the 1930s; interests in instrumentation and planetary atmospheres; the role of the Schmidt Camera in spectroscopy; planetary spectroscopy and the nature of the interstellar medium; founding of the FAR (Fund for Astronomical Research); World war II and work in optics for the National Defense Research Committee (NDRC) of the Office of Scientific Research and Development (OSRD); travels to Britian during the war; decision to leave astronomy after the war; move to Rochester for biophysical research; return to astronomy in 1952. The second interview concentrates on his contacts with Henry Norris Russell and activities during World War II.
Extensive interview covering early life and family in New York and Maine; schooling and early interests in astronomy in New York City; observing Halley's comet in 1910; World War I and college years at Harvard University majoring in chemistry; medical degree from Cornell University; contacts with Henry Norris Russell and Harlow Shapley, and decision to move into astronomy; graduate work at Princeton; postdoctoral work and staff position at Mt. Wilson in the 1930s; interests in instrumentation and planetary atmospheres; the role of the Schmidt Camera in spectroscopy; planetary spectroscopy and the nature of the interstellar medium; founding of the FAR (Fund for Astronomical Research); World war II and work in optics for the National Defense Research Committee (NDRC) of the Office of Scientific Research and Development (OSRD); travels to Britian during the war; decision to leave astronomy after the war; move to Rochester for biophysical research; return to astronomy in 1952. The second interview concentrates on his contacts with Henry Norris Russell and activities during World War II.
