Displaying 1 - 10 of total 125 results:
Early life in California, undergraduate work at Caltech (1947-51), graduate work at Caltech in physics and astronomy, including work at Mt Wilson-Palomar (1951-54), Accounts of Palomar sky survey (1953-56) and work on galaxies Impressions of instructors, among them Rubble, Zwicky, Baade, Minkowski Abell joined UCLA astronomy department in 1956 and describes its history, faculty, and expansion Discussion of Abell’s professional interest in popularization of astronomy since 1960’s (textbook, BBC-Open University work, campaign against astrology, summer science program) and technical work on su
Anderson talks almost exclusively about his work during the thirties with particles of high energy involved in nuclear reactions. He covers in detail his discovery of the positive electron, his pair production work with gamma rays, his expedition to Pike’s Peak with Neddermeyer and their discovery of the mesotron. He mentions that it was in his speech accepting the Nobel Prize in 1936 that he first mentioned the possibility of negative and positive particles of intermediate mass.
The interview focuses on Archambeau's geophysical training at the California Institute of Technology and his career as a seismologist, covering the period before 1970. Major emphasis lies on his involvement in issues related to the seismic detection of underground nuclear explosions and his advocacy for a nuclear test ban treaty. He discusses the Department of Defense's "Project Vela Uniform," which aimed at improving seismic detection capabilities, and he describes Vela's impact on his career on seismology in general.
Childhood and unconventional early education; Harvard University: impressions of courses and social climate; Caltech, Mt. Wilson, comments on Walter Baade and background of Baade’s theory; differences between astronomy and astrophysics; early professional career work on Magellanic clouds; interest in peculiar galaxies, Viktor A.
In this interview, Horace Babcock discusses how the field of astrophysics has changed over the course of his career. Topics discussed include: research administration; Mount Wilson Observatory; Ira S. Bowen; National Science Foundation; California Institute of Technology; stellar evolution; photomultiplier tubes; Joel Stebbins; Albert E.
This interview begins with a discussion of Babcock's childhood and youth around Mt. Wilson Observatory, with comments on father (Harold D. Babcock), Walter S. Adams, and Edwin P. Hubble. Also discussed in this interview: education at Caltech, University of California at Berkeley and Lick Observatory (1934-1939), and at Yerkes and MacDonald Observatories; work at MIT and Caltech on World War II hardware; astronomical instrumentation work, especially postwar Mt.
Discusses youth, college and graduate studies at Michigan (to 1930); work with Goudsmit, NRC Fellowships at Caltech (1930-1931) and MIT (1931-1932); Lloyd Fellowship at Michigan (1932-1933); work with Sawyer (1933-1934). Influence of Michigan summer sessions. Teaching and research at Columbia (1934-1935), move to Cornell (1935-1940); work with Bethe on REVIEW articles; involvement in nuclear physics; with Baker measures shape of neutron resonance by time-of-flight method, comparison with Fermi's results.
In this interview Robert Bacher discusses science policy and physicists' involvement in it after World War II through 1970. Topics discussed include: General Leslie Groves; international control of atomic energy; Chauncey Star; Manson Benedict; Report on the International Control of Atomic Energy (Acheson–Lilienthal Report); Dean Acheson; David Lilienthal; J.
This interview surveys Baum's career as a physicist at the Naval Research Laboratory (NRL) and astronomer at Mt. Wilson and Palomar Observatories. After sketching Baum's early life, the discussion concentrates on Baum's role in the development of spectroscopy research at NRL, specifically his work on the UV spectrum of the sun - including the first successful UV spectra of the sun.
Relation of the individual to the whole; California Institute of Technology (1939-1940); negative experience at Caltech; interest in Chinese and Japanese culture; Thesis – calculate scattering of light from a nebular gas cloud; University of California Berkeley (1941-1943); political interests and activity including Marxism, socialism, communism; better social, educational and natural environment at Berkeley; compute scattering of protons from deutrons [sic]; Lawrence Radiation Laboratory (1943-1946); electrostatic focusing, electric arc, nature of plasma, particle spin; effects of the atom