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Biographical Memoirs Volume 75 (1998) / Chapter Skim
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Robert B. Leighton
Pages 164-189

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From page 165...
... by himself. Bob Leighton built, improved, en c!
From page 166...
... en c! built inexpensive lO-meter radio telescopes of the highest quality for work at submillimeter wavelengths.
From page 167...
... At eight, Leighton won a movie-theater game involving Baby Ruth en c! Abba Zabba c ancly bars, reasoning that the smaller bars shouIc!
From page 168...
... en c! testecI.4 Leighton registered at Los Angeles City College in engineering, where he fount!
From page 169...
... Smythe. Smythe5 gave the clifficult course on classical electricity and magnetism, while Epstein taught theoretical thermoclynamics.
From page 170...
... from the course on nuclear physics of Fowler, Leighton incluclec! his elegant lecture notes in his own later text Principles of Modern Physics.
From page 171...
... only wait for an extremely energetic cosmic ray to collicle.
From page 172...
... Two odd tracks from high-energy cosmic rays in cloud chambers had been ascribed to V-particles and were cIassified as hooks and forks at Manchester University. The Caltech cloud chamber studies of many higher energy cosmic rays yielded similar complex events, some are illustrated in Leighton's textbook.
From page 173...
... In 1906 George Ellery Hale starter! astronomical observations on Mount Wilson en c!
From page 174...
... Wilson en c! the two scientists who later became directors, Ira Bowen en c!
From page 175...
... A long-slit, high-resolution spectrogram covers many picture elements simultaneously, making absorption lines wiggle.
From page 176...
... clie after a few minutes. Between the granules cooler falling darker material is founcI.
From page 177...
... Big Bear Solar Observatory just as Leighton's interests were changing. His last paper on the Sun, "A Magneto-Kinematic Moclel of the Solar Atmosphere," gave a partial explanation in 1968 of some of the Tong-term cycles of magnetic phenomena that Hale hac!
From page 178...
... The telescope vibrates! twenty times per second, so as to "chop" alternately between the sky plus object (i.e., signal plus noise)
From page 179...
... The experiment, built by the Jet Propulsion Laboratory, was lightweight, but its telemetry was seriously limited by the low rate at which information conic! be transmitter!
From page 180...
... who knew more about how everything in the universe worked than anyone else on Earth at that moment." Leighton en c! Feynman were close personal friends, enjoying talk about physics, Leighton's son Ralph entertained them musically en c!
From page 181...
... by raclio astronomers partly because their longer wavelengths clemanclec! only looser tolerances on surface accuracy.
From page 182...
... in peculiar active external galaxies. The molecular lines present gave information on the compositions, on the chemical processes in interstellar matter, en c!
From page 183...
... the NASA Exceptional Scientific Achievement Mecial in 1971. The six-component millimeter-wave radio telescopes at the Owens Valley Radio
From page 184...
... " I sympathized with my new astronomy graduate students who sometimes had to repeat some undergraduate physics courses. Yet, when I worked with former Caltech student Leverett Davis, Tr., in 1951 on the light scattered by spinning, elongated interstellar dust grains, Leverett remembered and found one of his Smythe problems, which gave the polarizability of an ellipsoid.
From page 185...
... 9. See the profusely illustrated book by Harold Zirin (who directed the Big Bear Solar Observatory)
From page 186...
... 104:1703-10. 1959 Observations of solar magnetic fields in plage regions.
From page 187...
... 140:1120-47. Transport of magnetic fields on the Sun.
From page 188...
... 188 BIOGRAPHICAL MEMOIRS 1979 With P


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