Displaying 1 - 10 of total 149 results:
Reviews Aarons' (b. October 3, 1921) career at AFCRL as a research physicist (1946-55), Chief of Radio Astronomy Branch (1955-72), and at AFGL as Chief of the Trans-ionospheric Propagation Branch and Senior Scientist at the Space Physics Lab (1972-81). Topics discussed include significant aspects of his role in the use of V-2s by Marcus O'Day for upper atmosphere research; his contact with O'Day and Menzel and the establishment of Sac Peak; the research mission of AFCRL; AFCRL's early interest in solar studies; and a comparison of present day research activities at AFGL and NRL.
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 super-clusters and cosmology.
Abt discusses his childhood and youth in Germany and then the United States; his student days at Northwestern University and his graduate work at Caltech; use of the Mt. Wilson 100-inch telescope; research topics include W Virginis stars and Zeta Auriga; his work at Lick Observatory and later at Yerkes; use of the McDonald 82-inch telescope for postdoc research; site survey for the building of Kitt Peak in 1959; life at Kitt Peak in its early years including building and design of new instruments; his work as editor of The Astrophysical Journal and the changes that took place over the years; and the final part discusses his personal life and public service efforts.
Childhood; early interest in science (astronomy). Member of Astronomical Society of the Pacific, 1928. Special student at University of California at Berkeley, 1931, with Donald H. Menzel’s help. Regular student from 1932; comments on teachers and fellow students at Berkeley Student Observatory. Summer assistantship at Lick Observatory (Nicholas Mayall, Arthur B. Wyse), life at Lick Observatory. To Harvard University in 1937 for graduate studies; comparison between Harvard and Berkeley/Lick; teaching assistant at Radcliffe; 3-year membership in Harvard Society of Fellows, from 1939, of enormous importance for his development; works with Menzel and James G. Baker on the Theory of Physical Processes in Gaseous Nebulae, 1937; Analysis of the Atmospheres of the A-type Dwarfs Gamma Geminorum and Sirius based on data from Louis Berman; Jesse Greenstein. Comments on Harvard Summer Schools, Harlow Shapley’ s Square.” Volunteer teacher of elementary physics courses from 1942 at Harvard. Lawrence Radiation Laboratory, 1943-1945; work involved evaluation of the chemists and the Counting Group’s output from the electromagnetic separation process. Job offer from University of Indiana (Frank Edmunson) accepted due to cutback at Radiation Laboratory. Indiana years, 1945-1948, very productive (drafts for two astrophysics books); problems getting telescope time at Yerkes Observatory and unsatisfactory living conditions leads to acceptance of a promising tenured position at Michigan, a center with very active research due to Leo Goldberg; Robert McMath’s influence in the department; Keith Pierce and Aller’s work on infrared solar spectrum. Work performed at Mt. Wilson Observatory and Dominion Astrophysical Observatory. Goldberg resigns in 1959; comments on Aller’s decision to leave Michigan; discussions of funding; “over-head” (Aller’s talk at an AAS Meeting); comparison of Lick Observatory and Kitt Peak Observatory policies. Work at Mt. Stromio Observatory, Australia on sabbatical visits, 1960, 1968-1969, 1977-1978. Overview of opinions of the present state of astronomy. Comments on personal life, wife and children.
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. Ambartsumian at the 1957 Solvay Conference; Fritz Zwicky; Atlas of Peculiar Galaxies; comments on published papers: Distribution of Quasars compared to Maarten Schmidt’s work with similar title; Edoard Stephan’s quintet; work on discrepant red shift with respect to the Friedman universe; future research interest, non-professional interests. Also prominently mentioned are: Basch, Bart Jan Bok, Subrahmanyan Chandrasekhar, William Alfred Fowler, Jesse Leonard Greenstein, Edwin Powell Hubble, Milton Lasell Humason, Bernard Lovell, Rudolph Leo Bernhard Minkowski, Jan Hendrik Oort, Edison Petit, Robert Richardson, Allan Sandage, Maarten Schmidt, Harlow Shapley, Dick Stoy, Vanderlaan, Gerard Henri de Vaucouleurs; Atlas of Peculiar Galaxies, Institut de Physique at Solvay, and United States Navy.
Dr. Eugene Avrett (1933 - ) is an astrophysicist at the Harvard-Smithsonian Center for Astrophysics. This interview reviews his personal and professional life and was conducted as part of a study of the history of the SAO during the tenure of Fred Whipple, 1955-1972. The interview covers his family life in a suburb of Atlanta, Georgia, public schooling and development of interests, influential teachers, and matriculation at Georgia Tech in electrical engineering in 1952. Facility in conceptual subjects like physics, but no special interests. Knowledge of WWII. Summer employment at Glenn L. Martin Aircraft on Matador program. Decision to switch to physics. Graduation in 1957 and entrance to Harvard for graduate study in physics. Advisors included Gerald Holton, Max Krook, George Carrier. Growth of interest in astrophysics slow, due to Krook and exposure to, first research in, and publications in stellar atmospheres. Teaching assistant for Bill Liller. Thesis with Max Krook. Collaboration with Owen Gingerich. Marriage in 1961 to Judith Reno Brett. Ph.D. in 1962, conferences attended that solidified his interests in stellar atmospheres and spectral line formation and non-LTE processes. Hired by Charles Whitney into the “Stellar Theory Division” at SAO. Organization of SAO under Whipple and his managers, including Harris Rosenthal, Charles Lundquist and Paul Tillinghast. Impressions of joint program between Harvard and Smithsonian. Teaching activities. Backup theoretical group for Celescope; extended discussion of Celescope, calibration issues, and the challenge of analyzing the data and the production of the catalogue of UV stellar colors. Nature of the data, methods of post-hoc calibration of the fields. Continued refinement of stellar atmospheres techniques and changing state of knowledge of theoretical energy distributions mitigate value of Celescope data. Role of Celescope staff, mainly Robert Davis, in the processing. History of OAO program; failed launches. Nancy Roman’s role in OAO and suggestion to close down Celescope. Work with student Steve Strom to prepare for Celescope reductions. NASA conference on OAO results. Relations between HCO and SAO and between Leon Goldberg and Fred Whipple. Teaching and thesis direction by SAO staff. Strom and early development of optical astronomy at SAO -- the MMT. SAO collaboration with Arizona rather than with Harvard. Use of OSO data for solar atmospheres research. Layoffs at SAO, deteriorating relations between Harvard and SAO and the formation of the Center for Astrophysics.
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. Whitford; Gerald Kron; Allan Sandage; Martin Schwarzschild; spectrographs; radio astronomy; x-ray astronomy; galactic evolution; stellar material; Robert McMath; societies; American Astronomical Society; International Astronomical Union; Jan Oort; Theodore Dunham Jr.; Alexander Pogo.
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. Wilson-Palomar diffraction gratings; discovery of magnetic stars and studies of variations; work on solar magnetic fields (with father) and theory of solar cycle; comments on cosmology; discussion of Mt. Wilson and Palomar Observatories since the 1920s, especially under Ira Bowen's and Babcock's directorship (1963); internal administration; staff relations; dealings with Carnegie Institution and Caltech; discussion of Hale Observatories, 1930-1977; role of government funding in astronomy; guest investigators; allocation of telescope time; planning, funding, and construction of the Carnegie Southern Observatory at Las Campanas, 1963-1977. Also prominently mentioned are: Philip Abelson, Ed Ackerman, Carl David Anderson, Wilhelm Heinrich Walter Baade, Patrick Maynard Stuart Blackett, Vannevar Bush, Subrahmanyan Chandrasekhar, Crawford Greenewalt, Jesse Leonard Greenstein, George Ellery Hale, Caryl Haskins, Louis Henyey, Armin O. Leuschner, Nicholas Ulrich Mayall, Charles Edward Kenneth Mees, Paul Merrill, Rudolph Leo Bernhard Minkowski, Edgar Nichols, Elmer Prall, Bruce Rule, Frederick H. Seares, Sinclair Smith, Otto Struve, Charles Hard Townes, George van Biesbroeck, H. A. Wood, Fritz Zwicky; Astronomical Society of the Pacific, Astrophysical Journal, Bausch and Lomb Co., Eastman Kodak Co., Ford Foundation, Hale Observatories, Hale Solar Laboratory, Inyokern Project, Kitt Peak National Observatory, Las Campanas Observatory, Lick Observatory Bulletin, McDonald Observatory, Mount Wilson and Palomar Observatories, National Science Foundation (U.S.), 48-inch Schmidt Telescope, 100-inch Telescope, 120-inch Telescope, 200-inch Telescope, and University of California at Berkeley, CA.
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. Aspects of his experience in experimentation with V-2s and Aerobees, and his thesis research on rockets at CALTECH (PhD, 1950, physics) are also explored. Additional topics discussed include: Optics Division, NRL; White Sands Proving Ground (NM); relationships with, and costs and descriptions of Baird Atomic; V-2 missile experiments, development and launch; meetings with Werner Von Braun; and contacts with R.W. Wood, J. Strong, Lyman, Stockbarger, and Tousey.
This interview reviews Bergstralh's childhood and early impressions of manned space exploration; his years as a graduate student at the University of Texas; his experience as a National Research Council fellow, and his time at the Jet Propulsion Laboratory as a senior scientist and member of the technical staff. He speaks at some length of his student-teacher relationship with G.H. Vaucouleurs. Other topics discussed include: NASA's Planetary Astronomy Program Office (now the Solar System Exploration Division, part of the Office of Space Science), activities at the University of Texas McDonald Observatory, and the Jet Propulsion Laboratory Table Mountain Observatory. With Bergstralh's employment history, most of his recollections involve NASA and a history of the research and administration of NASA headquarter and branches during the 1960s and 1970s.