Case Institute of Technology

In this interview, Jack Mowry, former owner of Sound & Vibration, discusses his career. He speaks about his time at the Case Institute of Technology where he received a degree in Engineering Administration. He details being a member of the Acoustical Society of America (ASA) and notes how he began publishing Sound & Vibration to replace the ASA magazine, Noise Control. He speaks to the strength of the staff of his magazine and talks about their first editor, Lou Goodfriend. Mowry discusses his time working with B&K Instruments. Lastly, he discusses launching NoiseExpo, a venue for presentations and training courses on noise and vibration control.

In this interview, David Zierler, Oral Historian for AIP interviews Siegfried Hecker, Professor Emeritus with the Department of Management Science and Engineering, and Senior Fellow, Freeman Spogli Institute for International Security and Cooperation, at Stanford University. Hecker recounts his family background as the child of ethnic Austrian and German parents who lived in Bosnia at the outbreak of World War II. He describes his family’s ordeal during the war and the circumstances surrounding his mother’s decision to move the family to the United States. Hecker recounts his experiences growing up in Cleveland and his decision to attend Case Tech for his undergraduate education. He explains his decision to switch his focus from physics to metallurgy, his formative summer at Los Alamos Lab before returning to Case for his Ph.D. work, and his decision to return to Los Alamos for postdoctoral research in metallurgy and elastic to plastic transitions. He describes his work at the General Motors Research Lab and his decision to return once again to Los Alamos, where he was assured he could focus on science and not management issues. Hecker explains how he became more involved in plutonium research and the various national security implications of this work. He describes his rise in the ranks at Los Alamos and how he became involved in national policy decisions in Washington. Hecker recounts the circumstances leading to being named director of Los Alamos, and he reflects on the challenges and opportunities he saw to improve the lab in this position. He provides an overview of nuclear weapons policy at the end of the Cold War and the renaissance in plutonium research in the 1990s. Hecker reflects on his decision to join the faculty at Stanford, and why he wanted to pursue matters of international security studies, and he describes his record of advisory work on nuclear verification in North Korea and elsewhere. At the end of the interview, Hecker describes his ongoing interest and research in metallurgy, and he reflects on how these interests bring him back full circle to the origins of his career. 

In this interview Richard Garwin discusses topics such as: his parents, growing up in Cleveland, education, Case Institute of Technology (Case Western Reserve University), Leon Lederman, muons, cyclotron,  University of Chicago, Enrico Fermi, nuclear reactors, coincidence circuits.This interview is part of a collection of interviews on the life and work of Richard Garwin. To see all associated interviews, click here.

Family background, early schooling; undergraduate studies at Case Institute of Technology (B.S. 1917); assistant physicist at National Bureau of Standards (1917-19); research on piezoelectricity of sodium chlorate and bromate; World War I work in pyrometry and optical glass manufacture; graduate studies at University of Minnesota (MA. 1920, teaching assistant 1919-20, Ph.D. 1921, instructor of physics, 1920-21), member of physics faculty; research on ferroelectricity of Rochelle Salt Crystals and location of Curie Points; X-ray spectroscopy research at University of Upsala, Sweden 1928-29; comments on nuclear physics at University of Minnesota.

This interview describes Fraser's work as an engineer and instrumentation specialist at the Department of Terrestrial Magnetism (DTM) during WWII, and then more significantly, at Applied Physics Laboratory (APL) following World War II.  His work at DTM was on proximity fuse research.  He tranferred from DTM to APL during the war and concentrated on radar research and control systems for guided missiles.  After the war, he participated in the used of V-2s for upper atmostphere research with James Van Allen's High Altitude Group, developing instrumentation for telemtetry and cosmic ray research.  Other affiliations and contacts discussed include:  Luis Alvarez, William Fowler, Allen Hynek, Richard Roberts, Philip Rudnick, Robert Shankland, Merle Tuve, James Van Allen, John Victoreen and the Victoreen Instrument Company, White Sands Missile Range.  Topics discussed include metallurgy, nuclear fission, proximity fuzes, rocket development and radio transmission.

Born July 19, 1915 in Cleveland, OH; family background and early childhood growing up in Cleveland; early interest in acoustics, the flute, electronics, and radio; graduated from high school in 1933; attended Case Institute of Technology, graduating with a B.S. in physics in 1937; moved to University of Illinois for graduate school, specialized in nuclear physics research (also maintained abiding interest in acoustics); thesis research on nuclear cross sections classified by wartime Manhattan Project; completed Ph.D. in 1941; awarded Westinghouse Research Fellowship in 1941 to work on wartime microwave electronics at corporate laboratories in Pittsburgh; collaborated with researchers at MIT Radiation Laboratory; concentrated on development of magnetrons and other high-power electron tubes; accepted full time position at Westinghouse in 1944; developed x-ray image amplifier, major innovation for medical fluoroscopy; transitioned into management positions initially overseeing electronics projects (and some nuclear physics work); graduatlly moved into senior management positions focusing on research strategy and policy; retired in 1980; continued work in acoustics field.

This interview traces Brunk's career in engineering with the National Advisory Committee for Aeronautics (NACA), Lewis Research Center (formerly Lewis Flight Propulsion Laboratory), NASA and NASA Headquarters.  The discussion begins with an overview of his family background and his education at Case Institute of Technology, followed by his work in supersonic aerodynamics for NACA.  The interview primarily examines Brunk's role in and perceptions of the development of planetary ground-based astronomy during his tenure at NASA Headquarters, as Program Chief of Planetary Astronomy.  Topics discussed include: telescope innovations at different observatories; problems and techniques in ground-based observation; exploration of Mars; the Planetary Patrol program at Lowell Observatory; his membership to the American Astronomical Society; and general perceptions of NASA's role in ground-based astronomy.  Other affiliations and contacts discussed include: Jason Nassau, Nancy Roman, Urner Liddel, and Gerard Kuiper.

This interview traces Brunk's career in engineering with the National Advisory Committee for Aeronautics (NACA), Lewis Research Center (formerly Lewis Flight Propulsion Laboratory), NASA and NASA Headquarters.  The discussion begins with an overview of his family background and his education at Case Institute of Technology, followed by his work in supersonic aerodynamics for NACA.  The interview primarily examines Brunk's role in and perceptions of the development of planetary ground-based astronomy during his tenure at NASA Headquarters, as Program Chief of Planetary Astronomy.  Topics discussed include: telescope innovations at different observatories; problems and techniques in ground-based observation; exploration of Mars; the Planetary Patrol program at Lowell Observatory; his membership to the American Astronomical Society; and general perceptions of NASA's role in ground-based astronomy.  Other affiliations and contacts discussed include: Jason Nassau, Nancy Roman, Urner Liddel, and Gerard Kuiper.

Interview discusses, not in chronological order: early home life and schooling; undergraduate at Leiden, influence of Paul Ehrenfest, Jan H. Oort, Jacobus C. Kapteyn, Gerard Kuiper, Antonie Pannekoek, Ejnar Hertzsprung. Recollections of work of Georg Uhlenbeck and Samuel Goudsmit. Assistant to Peter van Rhijn at Groningen ca. 1928, work on various stellar and galactic topics. Move to Harvard, 1929, and atmosphere there under Harlow Shapley. Marriage to Priscilla Fairfield Bok; her contacts with William W. Campbell. Search for and interpretation of spiral auras of our galaxy; studies of stellar density distribution. Activities during World War II. Harvard astronomy group's difficult postwar transition; McCarthyism. Work on nebulae and globules. Comments on astronomy at Mt. Wilson, Tonantziutla, and South Africa. Origins of Harvard radio astronomy and National Radio Astronomy Observatory, and their funding. Move to Australia, 1956, and conditions there. Move to Steward Observatory of University of Arizona, 1964, and conditions there. Location of national observatory at Kitt Peak; management of Kitt Peak. Discussions of astronomy, education, popularization, employment, and organization. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, McGeorge Bundy, Edwin F. Carpenter, Tom Cherry, James Bryant Conant, Arthur Stanley Eddington, Sergei Gaposchkin, Jesse Leonard Greenstein, Haro, David Heeschen, Ejnar Hertzsprung, James Jeans, Ivan Robert King, Bertil Lindblad, Antonia Maury, Nicholas Ulrich Mayall, Joseph McCarthy, Sidney McCuskey, Aden Meinel, Donald Howard Menzel, Robert Menzies, James E. Miller, Edward Arthur Milne, William Wilson Morgan, Edward Charles Pickering, Harry Hemley Plaskett, Nathan Pusey, Martin Schwarzschild, Willem de Sitter, Otto Struve; American Astronomical Society, Associated Universities for Research in Astronomy, Associated Universities, Inc., Boyden Observatory, Case Institute of Technology, Harvard College Observatory, Harvard Series on Astronomy, Indiana University, Mount Stromlo Observatory, National Science Foundation (U.S.), Ohio State University, Princeton University, Rijksuniversiteit te Groningen, Rijksuniversiteit te Leiden, University of Arizona, University of Illinois, University of Michigan, and University of Texas.

Interview discusses, not in chronological order: early home life and schooling; undergraduate at Leiden, influence of Paul Ehrenfest, Jan H. Oort, Jacobus C. Kapteyn, Gerard Kuiper, Antonie Pannekoek, Ejnar Hertzsprung. Recollections of work of Georg Uhlenbeck and Samuel Goudsmit. Assistant to Peter van Rhijn at Groningen ca. 1928, work on various stellar and galactic topics. Move to Harvard, 1929, and atmosphere there under Harlow Shapley. Marriage to Priscilla Fairfield Bok; her contacts with William W. Campbell. Search for and interpretation of spiral auras of our galaxy; studies of stellar density distribution. Activities during World War II. Harvard astronomy group's difficult postwar transition; McCarthyism. Work on nebulae and globules. Comments on astronomy at Mt. Wilson, Tonantziutla, and South Africa. Origins of Harvard radio astronomy and National Radio Astronomy Observatory, and their funding. Move to Australia, 1956, and conditions there. Move to Steward Observatory of University of Arizona, 1964, and conditions there. Location of national observatory at Kitt Peak; management of Kitt Peak. Discussions of astronomy, education, popularization, employment, and organization. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, McGeorge Bundy, Edwin F. Carpenter, Tom Cherry, James Bryant Conant, Arthur Stanley Eddington, Sergei Gaposchkin, Jesse Leonard Greenstein, Haro, David Heeschen, Ejnar Hertzsprung, James Jeans, Ivan Robert King, Bertil Lindblad, Antonia Maury, Nicholas Ulrich Mayall, Joseph McCarthy, Sidney McCuskey, Aden Meinel, Donald Howard Menzel, Robert Menzies, James E. Miller, Edward Arthur Milne, William Wilson Morgan, Edward Charles Pickering, Harry Hemley Plaskett, Nathan Pusey, Martin Schwarzschild, Willem de Sitter, Otto Struve; American Astronomical Society, Associated Universities for Research in Astronomy, Associated Universities, Inc., Boyden Observatory, Case Institute of Technology, Harvard College Observatory, Harvard Series on Astronomy, Indiana University, Mount Stromlo Observatory, National Science Foundation (U.S.), Ohio State University, Princeton University, Rijksuniversiteit te Groningen, Rijksuniversiteit te Leiden, University of Arizona, University of Illinois, University of Michigan, and University of Texas.