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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.
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.
Family background and early education, motivation and funding for college; math program at Stanford University, from 1928; physics studies at California Institute of Technology; graduate study at Princeton University, beginning 1932, atmosphere of the department, faculty (Lou Turner, Eugene Wigner, John Von Neumann); colloquia, Edward Condon. Development of applications of group theory, work in solid state with Linus Pauling, Hillard B. Huntington, Albert Sherman, William Hansen, William Shockley, Robert R. Brattain, R. Bowling Barnes. Betty Seitz; work with her on the text Modern Theory of Solids. Sodium band theory work with Wigner. To University of Rochester with Lee DuBridge. Centers for solid state work including University of Michigan, University of Wisconsin, Harvard University (John Van Vleck). Work at General Electric, 1935-1936, studies of luminescence; atmosphere in industrial labs following Depression, contacts with other industrial labs; association with DuPont. State of physics in 1930s, trends at solid state centers. Work on crystal defects, pigments, leading to work on germanium and, particularly, silicon; history of study of semiconductors and influences on its development such as World War II; work on dislocations and creep; work at Westinghouse Company. World War II work with Frankford Arsenal, Dahlgren Proving Ground, and Massachusetts Institute of Technology Radiation Laboratory; University of Pennsylvania, 1938; Carnegie-Mellon University, 1942, on dark trace tubes, leading to color center papers; University of Chicago work on reactors and neutron diffraction, 1943; Oak Ridge National Laboratory with Wigner; Argonne National Laboratory, solid state group. With Field Intelligence Agency Technical (FIAT), visit to Gottingen, 1945; state of solid state physics in international centers and U.S. Return to Carnegie- Mellon; diffusion theory. Pugwash Conferences; trips to Japan, 1953 and 1962, conditions and theoretical solid state work in postwar Japan. To University of Illinois, 1949 (Wheeler Loomis); John Bardeen's work, visits by Nevill Mott and Heinz Pick; McCarthyism. Development of Seitz's bibliography, changes in the study of solid state during the 1950s.
Family background and early education, motivation and funding for college; math program at Stanford University, from 1928; physics studies at California Institute of Technology; graduate study at Princeton University, beginning 1932, atmosphere of the department, faculty (Lou Turner, Eugene Wigner, John Von Neumann); colloquia, Edward Condon. Development of applications of group theory, work in solid state with Linus Pauling, Hillard B. Huntington, Albert Sherman, William Hansen, William Shockley, Robert R. Brattain, R. Bowling Barnes. Betty Seitz; work with her on the text Modern Theory of Solids. Sodium band theory work with Wigner. To University of Rochester with Lee DuBridge. Centers for solid state work including University of Michigan, University of Wisconsin, Harvard University (John Van Vleck). Work at General Electric, 1935-1936, studies of luminescence; atmosphere in industrial labs following Depression, contacts with other industrial labs; association with DuPont. State of physics in 1930s, trends at solid state centers. Work on crystal defects, pigments, leading to work on germanium and, particularly, silicon; history of study of semiconductors and influences on its development such as World War II; work on dislocations and creep; work at Westinghouse Company. World War II work with Frankford Arsenal, Dahlgren Proving Ground, and Massachusetts Institute of Technology Radiation Laboratory; University of Pennsylvania, 1938; Carnegie-Mellon University, 1942, on dark trace tubes, leading to color center papers; University of Chicago work on reactors and neutron diffraction, 1943; Oak Ridge National Laboratory with Wigner; Argonne National Laboratory, solid state group. With Field Intelligence Agency Technical (FIAT), visit to Gottingen, 1945; state of solid state physics in international centers and U.S. Return to Carnegie- Mellon; diffusion theory. Pugwash Conferences; trips to Japan, 1953 and 1962, conditions and theoretical solid state work in postwar Japan. To University of Illinois, 1949 (Wheeler Loomis); John Bardeen's work, visits by Nevill Mott and Heinz Pick; McCarthyism. Development of Seitz's bibliography, changes in the study of solid state during the 1950s.
Family background and early education, motivation and funding for college; math program at Stanford University, from 1928; physics studies at California Institute of Technology; graduate study at Princeton University, beginning 1932, atmosphere of the department, faculty (Lou Turner, Eugene Wigner, John Von Neumann); colloquia, Edward Condon. Development of applications of group theory, work in solid state with Linus Pauling, Hillard B. Huntington, Albert Sherman, William Hansen, William Shockley, Robert R. Brattain, R. Bowling Barnes. Betty Seitz; work with her on the text Modern Theory of Solids. Sodium band theory work with Wigner. To University of Rochester with Lee DuBridge. Centers for solid state work including University of Michigan, University of Wisconsin, Harvard University (John Van Vleck). Work at General Electric, 1935-1936, studies of luminescence; atmosphere in industrial labs following Depression, contacts with other industrial labs; association with DuPont. State of physics in 1930s, trends at solid state centers. Work on crystal defects, pigments, leading to work on germanium and, particularly, silicon; history of study of semiconductors and influences on its development such as World War II; work on dislocations and creep; work at Westinghouse Company. World War II work with Frankford Arsenal, Dahlgren Proving Ground, and Massachusetts Institute of Technology Radiation Laboratory; University of Pennsylvania, 1938; Carnegie-Mellon University, 1942, on dark trace tubes, leading to color center papers; University of Chicago work on reactors and neutron diffraction, 1943; Oak Ridge National Laboratory with Wigner; Argonne National Laboratory, solid state group. With Field Intelligence Agency Technical (FIAT), visit to Gottingen, 1945; state of solid state physics in international centers and U.S. Return to Carnegie- Mellon; diffusion theory. Pugwash Conferences; trips to Japan, 1953 and 1962, conditions and theoretical solid state work in postwar Japan. To University of Illinois, 1949 (Wheeler Loomis); John Bardeen's work, visits by Nevill Mott and Heinz Pick; McCarthyism. Development of Seitz's bibliography, changes in the study of solid state during the 1950s.
Family background and early education, motivation and funding for college; math program at Stanford University, from 1928; physics studies at California Institute of Technology; graduate study at Princeton University, beginning 1932, atmosphere of the department, faculty (Lou Turner, Eugene Wigner, John Von Neumann); colloquia, Edward Condon. Development of applications of group theory, work in solid state with Linus Pauling, Hillard B. Huntington, Albert Sherman, William Hansen, William Shockley, Robert R. Brattain, R. Bowling Barnes. Betty Seitz; work with her on the text Modern Theory of Solids. Sodium band theory work with Wigner. To University of Rochester with Lee DuBridge. Centers for solid state work including University of Michigan, University of Wisconsin, Harvard University (John Van Vleck). Work at General Electric, 1935-1936, studies of luminescence; atmosphere in industrial labs following Depression, contacts with other industrial labs; association with DuPont. State of physics in 1930s, trends at solid state centers. Work on crystal defects, pigments, leading to work on germanium and, particularly, silicon; history of study of semiconductors and influences on its development such as World War II; work on dislocations and creep; work at Westinghouse Company. World War II work with Frankford Arsenal, Dahlgren Proving Ground, and Massachusetts Institute of Technology Radiation Laboratory; University of Pennsylvania, 1938; Carnegie-Mellon University, 1942, on dark trace tubes, leading to color center papers; University of Chicago work on reactors and neutron diffraction, 1943; Oak Ridge National Laboratory with Wigner; Argonne National Laboratory, solid state group. With Field Intelligence Agency Technical (FIAT), visit to Gottingen, 1945; state of solid state physics in international centers and U.S. Return to Carnegie- Mellon; diffusion theory. Pugwash Conferences; trips to Japan, 1953 and 1962, conditions and theoretical solid state work in postwar Japan. To University of Illinois, 1949 (Wheeler Loomis); John Bardeen's work, visits by Nevill Mott and Heinz Pick; McCarthyism. Development of Seitz's bibliography, changes in the study of solid state during the 1950s.