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Displaying 1 - 10 of total 18 results:
Family background; father’s education; early education and musical interest; Amherst College with graduate fellowship; graduate school at Harvard University; influence of Elmer Kohler’s course on early research problems, bromination of ketones. Comments on staff, fellow students and influential faculty at Harvard (James B. Conant); teaching policies at Harvard. Postdoctoral work at Rockefeller Institute and Columbia University; wife’s contribution to career; University of Minnesota position, comments on Charles Frederick Koelsch’s work and on the facilities at Minnesota.
Childhood and major influences; college education at Harvard University; position at Edward C. Worden Co., position at Columbia University's chemistry department as a graduate student and instructor, as a professor, and as the department chairman; history of chemistry department's administration. Major emphasis on his research results and papers spanning his entire career; Hammett equation and acidity theory; his contact with students Henry P. Treffers, Martin Paul, Lois Zucker.
Childhood and major influences; college education at Harvard University; position at Edward C. Worden Co., position at Columbia University's chemistry department as a graduate student and instructor, as a professor, and as the department chairman; history of chemistry department's administration. Major emphasis on his research results and papers spanning his entire career; Hammett equation and acidity theory; his contact with students Henry P. Treffers, Martin Paul, Lois Zucker.
Harvard University to Bell Laboratories in 1925 seeking job as chemist, ending up in the General Methods and Audits Department for five years; Publications Department, 1930; editor of Bell Laboratories Record. Depression lay-offs at Bell Labs. Holden to Chemistry Department (under Girard T. Kohman), 1936; W. Edgerton. Informal groups studying Mott and Jones Theory of Metals, Tolman's Statistical Mechanics. Comments on numerous other scientists including William Shockley, Foster Nix, James Fisk, Bancroft Gherardi. Solid state group formed in 1945.
Harvard University to Bell Laboratories in 1925 seeking job as chemist, ending up in the General Methods and Audits Department for five years; Publications Department, 1930; editor of Bell Laboratories Record. Depression lay-offs at Bell Labs. Holden to Chemistry Department (under Girard T. Kohman), 1936; W. Edgerton. Informal groups studying Mott and Jones Theory of Metals, Tolman's Statistical Mechanics. Comments on numerous other scientists including William Shockley, Foster Nix, James Fisk, Bancroft Gherardi. Solid state group formed in 1945.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Childhood in New York City; studying astronomy and literature at Harvard (1925-1929, M.A. 1930); work during the Depression in real estate and at Columbia; graduate-education in the new astrophysics at Harvard (1934-1937), contacts with H. Shapley, C. Payne, H.N. Russell; work at Yerkes from 1937: nebula spectroscopy, stellar composition, stellar atmospheres; contacts with 0. Struve, S. Chandrasekhar, B. Stromgren; optical design work during World War II. Move to Cal Tech, 1947, contacts with W. Baade, I. Bowen, F. Zwicky, N. Schmidt, L.
Family background; freshman course instructors at the University of Chicago; war-time training program; living next door to Manhattan Project people; Radio Research Laboratory at Harvard University; work on jamming tools (radar counter-measures) and antennas; work and graduate study at the Institute for the Study of Metals the University of Chicago (with Clarence Zener); work with Andy Lawson; E. R.