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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
Interview focusses on early life in Vienna, family and religion; atmosphere in Vienna in early 1930s; growth of interest in mathematical physics; anti-Semitism in Vienna; influence of history teacher and rejection of religion; influence of reading Eddington and Jeans in the mid-1930s; further study in England and contact with Eddington; Trinity College, 1937-1940; study with Besicovitch; collapse of plebiscite and family in Vienna; internment during World WarII; graduate study with Harold Jeffreys; naval radar, 1942; associates during war and circle at Cambridge; development of radar research team with Gold and Hoyle; developing astronomical interests, 1943; early research on accretion and evolution; cosmology; general relativity; contact with Dyson, Lighthill and W.H. McCrae; work in theoretical stellar structure; the problem of red giants; Hoyle's theory of stellar evolution; Hoyle-Lyttleton red giant models; growing interests in cosmology and discussion of Tolman and Hubble; the Steady State Cosmology; reactions to Steady State theory; gravitational theory and relativity circa 1955.
Deals with the career of Herbert Friedman, an experimentalist who used space-borne instruments from the 1940s through 1970s to examine the upper atmosphere and astronomical phenomena. Pioneer in the fields of solar and non-solar x-ray astronomy. His role in development of Naval Research Laboratory (NRL) research programs. Discussed are: childhood and youth; his family's Jewish tradition; physics education at Brooklyn College and Johns Hopkins University during the Depression; anti-semitism in job-hiring; to the National Research Laboratory (NRL), 1940; war work on radio crystal oscillators using x-ray techniques; his atomic bomb detection work after the war; introduction to rocket research at NRL immediately after the war; Navy funding of rocket work; early solar x-ray work, 1949-1958; impressions of colleagues Edward O. Hulbert, Richard Tousey, T. Robert Burnight, Homer E. Newell; impact of Sputnik and creation of the National Aeronautics and Space Administration (NASA) in 1958; pioneering work in ultraviolet astronomy and non-solar x-ray astronomy; x-ray astronomy work in the 1960s; trying to detect neutron stars in 1964; x-ray astronomy in the 1970s; High Energy Astronomy Observatory program; possible evidence for a closed universe; administration of NRL; his work on various committees (including the President's Science Advisory Committee); future programs such as the Space Shuttle and Space Telescope. Also prominently mentioned are: William W. Beeman, C. Stuart Bowyer, Werner von Braun, Gunter Bruckner, Edward T. Byram, George Carruthers, Talbot Chubb, James Franck, Riccardo Giacconi, Leo Goldberg, John Charles Hubbard, Neil Johnson, Jim Kurfess, James Van Allen; American Science and Engineering, Inc., High Energy Astronomy Observatory, Johns Hopkins University Applied Physics Laboratory, National Academy of Sciences (U.S.), Naval Research Laboratory (U.S.), Phillips Petroleum Co., United States Office of Naval Research, V-2 (Rocket), and Washington Navy Yard.
After surveying Martin Harwit's family background and early education, the interview concentrates on: his graduate education at Massachusetts Institute of Technology; his career in physics at Cambridge Unviersity as a NATO Fellow; his time at the Naval Research Laboratory (NRL) as a National Science Foundation Fellow; and, principally, his work at Cornell as assistant and associate professor of astronomoy, professor, and chairman of the Physics department. While discussing his childhood and education, Harwit addresses the antisemitism he and his family faced in German and in the United States. This interview covers a broad range of his scientific interest: galaxy and star formations; comets; infrared optics, especially relating to detector technology; infrared astronomy; rocketry; history of philosophy in science; use of balloons in observation; and astronomy education. Some affliliations discussed include: John Decker, Herbert Friedman, Thomas Gold, and Fred Hoyle.
After surveying Martin Harwit's family background and early education, the interview concentrates on: his graduate education at Massachusetts Institute of Technology; his career in physics at Cambridge Unviersity as a NATO Fellow; his time at the Naval Research Laboratory (NRL) as a National Science Foundation Fellow; and, principally, his work at Cornell as assistant and associate professor of astronomoy, professor, and chairman of the Physics department. While discussing his childhood and education, Harwit addresses the antisemitism he and his family faced in German and in the United States. This interview covers a broad range of his scientific interest: galaxy and star formations; comets; infrared optics, especially relating to detector technology; infrared astronomy; rocketry; history of philosophy in science; use of balloons in observation; and astronomy education. Some affliliations discussed include: John Decker, Herbert Friedman, Thomas Gold, and Fred Hoyle.
After surveying Martin Harwit's family background and early education, the interview concentrates on: his graduate education at Massachusetts Institute of Technology; his career in physics at Cambridge Unviersity as a NATO Fellow; his time at the Naval Research Laboratory (NRL) as a National Science Foundation Fellow; and, principally, his work at Cornell as assistant and associate professor of astronomoy, professor, and chairman of the Physics department. While discussing his childhood and education, Harwit addresses the antisemitism he and his family faced in German and in the United States. This interview covers a broad range of his scientific interest: galaxy and star formations; comets; infrared optics, especially relating to detector technology; infrared astronomy; rocketry; history of philosophy in science; use of balloons in observation; and astronomy education. Some affliliations discussed include: John Decker, Herbert Friedman, Thomas Gold, and Fred Hoyle.
Discusses his work in solid state physics, band theory, research relating anit-submarine warfare during World War II, physics in the Soviet Union, working at Bell Laboratories in the late 1940s; antisemitism in the field of physics; working with William Shockley. Persons prominently mentioned include: John C. Slater, Albert Gordon Hill, John Bardeen.
Born February 13, 1923 in Berlin, Germany; discusses life in Germany and Belgium under Hitler’s rule. Recalls his transition to America and his high school and undergraduate education in New York; discusses his transfer to the University of Michigan and being hired at MIT’s Radiation Lab. Discusses his graduate education at Columbia in physics and his interest in geophysics from Maurice Ewing; Jean Katz discusses her background and how she came to be Ewing’s personal secretary. Recalls his first cruise on the Albatross in 1952; describes his interactions with the individuals active at Lamont. Recalls the poor reception of the novelty of his dissertation; being forced to change his new layer theory to accommodate a two layer model. Discusses his decision to leave Lamont for Stanford and later RPI, only to return to Lamont. Contemplates the reasons for Lamont’s success; describes his awareness of the Heezen-Ewing controversy and its effect on Lamont.
Life of his father, Karl Schwarzschild; father's scientific relationships in Göttingen (Felix Klein, David Hilbert); move to Potsdam, 1909; relations with Potsdam and Berlin scientists (Albert Einstein, Karl Sommerfeld); father's Jewish background concealed. M. Schwarzschild's youth in Göttingen and Berlin; early education, interest in astronomy and mathematics. Undergraduate at Göttingen Universität (Hans Kienle, Richard Courant, Neugebauer), 1930-1933; graduate work at Gottingen Observatory, 1933-1935; his reaction to Nazism. Introduction to astrophysics (Arthur Eddington), interest in stellar interiors and stellar evolution; contacts with other astronomers from Gottingen Observatory (Otto Heckmann, Kienle, Rupert Wildt); comments on general relativity; interest in pulsating stars; leaves Göttingen, 1936. Postdoctorate at Oslo (Svein Rosseland); Jan Oort, Ejnar Hertzsprung; mechanical analog computer for computations in astrophysics and celestial mechanics; comments on development of theory of stellar interiors, 1939-1950. To Harvard College Observatory (Harlow Shapley), 1938; C. Payne-Gaposchkin, Bart Bok; comparison of European and American observational style, social scene; Barbara Schwarzschild's difficulties as female astronomer; contacts with S. Chandrasekhar and other astronomers. Tour of the United States; visits Mt. Wilson Observatory (Wilhelm Baade, Rudolph Minkowski, Edwin Hubble, Milton Humason), 1940; Shapley's relationship with Mt. Wilson staff. Harvard (Fred Whipple), 1938-1941; Shapley as a leader; astronomy summer school at Harvard; work on Cepheid variables in M3 (Bok, Chandrasekhar); overall impact on Schwarzschild of Harvard period. Columbia University (Jan Schildt, I. I. Rabi), 1940-1942; difficulties there; origin and funding of Thomas Watson Astronomical Computing Center; discussion of cosmology in the late 1930s; contacts with physicists (Enrico Fermi). In U.S. Army, 1941-1945; enters as private, teaches math to recruits; refuses invitation to Los Alamos; transferred to Aberdeen Proving Ground, dissatisfaction there; to officers training school, does bombing analysis for Italian campaign. Work relating to stellar interiors and evolution, 1938-1946; nuclear energy source ideas (Hans Bethe, Fermi); Eddington, Gerard Kuiper, Chandrasekhar, G. Keller; German astronomers during World War II (Ludwig Biermann). Discussion of wife's career and her role in his career. Early ideas about red giants (Öpik, Herman Bondi, Fred Hoyle), 1946-1950. Work on acoustic wave energy transport (R. Richardson, Gold); work on chemical composition differences in stellar populations. To Princeton University (Spitzer, H. N. Russell), 1947; Project Matterhorn (start of bomb and fusion projects); relationship with Russell. Stellar evolution work in the 1950s; computer work (John Von Neumann, Richard Härm), mid-1950s; collaboration with Allan Sandage evolving a stellar model, 1952; computing towards red giants; observational cluster work, 1951; ages, metallicity, and the Big Bang; beginnings of "astrophysical" cosmology. Evolution theory after late 1950s; effect of computers on theoretical progress; relation of evolution theory to cosmology; general comments on his work in stellar evolution; interactions with Robert Dicke; views on cosmology, general relativity. Need for better solar convection work leads to use of balloons (James Van Allen); post-Sputnik funding; on cooperation with industry and engineers; Stratoscope II (Bob Danielson, Spitzer). Years advising the National Science Foundation, President's Science Advisory Committee, 1959-1976, and National Aeronautics and Space Administration (Von Neumann), to 1969; The International Astronomical Union, 1964-1970; American Asronomical Society, 1967-1973. Informal advisor to various observatories: Kitt Peak National Observatory, Mt. Wilson-Palomar Observatories, Carnegie Southern Observatory. Recent work on galactic structure. Reflects on importance of ethical standards; his feelings about religion and nature.
Life of his father, Karl Schwarzschild; father's scientific relationships in Göttingen (Felix Klein, David Hilbert); move to Potsdam, 1909; relations with Potsdam and Berlin scientists (Albert Einstein, Karl Sommerfeld); father's Jewish background concealed. M. Schwarzschild's youth in Göttingen and Berlin; early education, interest in astronomy and mathematics. Undergraduate at Göttingen Universität (Hans Kienle, Richard Courant, Neugebauer), 1930-1933; graduate work at Gottingen Observatory, 1933-1935; his reaction to Nazism. Introduction to astrophysics (Arthur Eddington), interest in stellar interiors and stellar evolution; contacts with other astronomers from Gottingen Observatory (Otto Heckmann, Kienle, Rupert Wildt); comments on general relativity; interest in pulsating stars; leaves Göttingen, 1936. Postdoctorate at Oslo (Svein Rosseland); Jan Oort, Ejnar Hertzsprung; mechanical analog computer for computations in astrophysics and celestial mechanics; comments on development of theory of stellar interiors, 1939-1950. To Harvard College Observatory (Harlow Shapley), 1938; C. Payne-Gaposchkin, Bart Bok; comparison of European and American observational style, social scene; Barbara Schwarzschild's difficulties as female astronomer; contacts with S. Chandrasekhar and other astronomers. Tour of the United States; visits Mt. Wilson Observatory (Wilhelm Baade, Rudolph Minkowski, Edwin Hubble, Milton Humason), 1940; Shapley's relationship with Mt. Wilson staff. Harvard (Fred Whipple), 1938-1941; Shapley as a leader; astronomy summer school at Harvard; work on Cepheid variables in M3 (Bok, Chandrasekhar); overall impact on Schwarzschild of Harvard period. Columbia University (Jan Schildt, I. I. Rabi), 1940-1942; difficulties there; origin and funding of Thomas Watson Astronomical Computing Center; discussion of cosmology in the late 1930s; contacts with physicists (Enrico Fermi). In U.S. Army, 1941-1945; enters as private, teaches math to recruits; refuses invitation to Los Alamos; transferred to Aberdeen Proving Ground, dissatisfaction there; to officers training school, does bombing analysis for Italian campaign. Work relating to stellar interiors and evolution, 1938-1946; nuclear energy source ideas (Hans Bethe, Fermi); Eddington, Gerard Kuiper, Chandrasekhar, G. Keller; German astronomers during World War II (Ludwig Biermann). Discussion of wife's career and her role in his career. Early ideas about red giants (Öpik, Herman Bondi, Fred Hoyle), 1946-1950. Work on acoustic wave energy transport (R. Richardson, Gold); work on chemical composition differences in stellar populations. To Princeton University (Spitzer, H. N. Russell), 1947; Project Matterhorn (start of bomb and fusion projects); relationship with Russell. Stellar evolution work in the 1950s; computer work (John Von Neumann, Richard Härm), mid-1950s; collaboration with Allan Sandage evolving a stellar model, 1952; computing towards red giants; observational cluster work, 1951; ages, metallicity, and the Big Bang; beginnings of "astrophysical" cosmology. Evolution theory after late 1950s; effect of computers on theoretical progress; relation of evolution theory to cosmology; general comments on his work in stellar evolution; interactions with Robert Dicke; views on cosmology, general relativity. Need for better solar convection work leads to use of balloons (James Van Allen); post-Sputnik funding; on cooperation with industry and engineers; Stratoscope II (Bob Danielson, Spitzer). Years advising the National Science Foundation, President's Science Advisory Committee, 1959-1976, and National Aeronautics and Space Administration (Von Neumann), to 1969; The International Astronomical Union, 1964-1970; American Asronomical Society, 1967-1973. Informal advisor to various observatories: Kitt Peak National Observatory, Mt. Wilson-Palomar Observatories, Carnegie Southern Observatory. Recent work on galactic structure. Reflects on importance of ethical standards; his feelings about religion and nature.