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MILLIKAN, R. A. Nobel Laureate In Physics (1923) And Others. Listings

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1 MILLIKAN, R. A. Nobel Laureate in Physics (1923) and Others. ELEVEN OFFPRINTS FROM VARIOUS JOURNALS 1921-1927.
1921. Paperback 
Eleven Very Good+ to Fine offprints in original printed wrappers as follows: "The Further Extension of the Ultra-Violet-Spectrum and the Progression with Atomic Number of the Spectra of Light Elements" (1921); "The Vacum-Spark Spectra in the Extreme Ultra-Violet of Carbon, Iron, and Nickel" (1921); "The Fine Structure of the Nitrogen Oxygen, and Fluorine Lines in the Extreme Ultra-Violet" (1924); "The Series Spectra of the Stripped Boron Atom" (1924); "Extreme Ultra-Violet Spectra" (1924); "The Series Spectra of Three-Valence-Electron Atoms of Phosphorus, Sulphur, and Chlorine" (1925); "The Seies Spectra of the Stripped Atoms of Phosphorus, Sulphur, and Chlorine" (1925); '"The Series Spectra of Two-Valence-Electron Atoms of Phosphorus, Sulphur, and Chlorine" (1925); "Stripped Oxygen, OVI, The PP' Group ion OV, and New Aluminum Lines in the Extreme Ultra-Violet" (1926); "Recent Developments in Spectroscopy" (1927).

The Nobel Prize in Physics 1923 was awarded to Robert A. Millikan "for his work on the elementary charge of electricity and on the photoelectric effect". 
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2 MILLIKAN, R. A. Nobel Laureate in Physics (1923) and Others. TEN OFFPRINTS FROM VARIOUS JOURNALS AND TWO ISSUES OF NATURE AND ON ISSUE OF THE PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES 1926-1930.
1926. Paperback 
Offered are ten offprints, two entire issues of Nature, and one entire issue of the Proceedings of the National Academy of Sciences in Very Good+ to Near Fine condition in self or original printed wrappers as follows: "High Frequency Rays of Cosmic Origin" (1926); "High Frequency Rays of Cosmic Origin. I. Sounding Balloon Observations at Extreme Altitudes" (1926); "High Frequency Rays of Cosmic Origin II. Mountain Peak and Airplane Observations" (1926); High Frequency Rays of Cosmic Origin III. Measurements in Snow-Fed Lakes at High Altitudes" (1926); "The Significance of Recent Cosmic-Ray Experiments" In the Proceedings of the National Academy of Sciences, Vol. 16, No. 6, June, 1930, pp. 421-425; "New Results on Cosmic Rays" (1928); "On the Question of the Constancy of the Cosmic Radiation and the Relation of These Rays to Meteorology' (1930); "The Significance of Recent Cosmic-Ray Experiments" (1930); "Further Experiments on the Uniformity of Distribution of the Cosmic Radiation" (1932); "Cosmic-Rays Energies and Their Bearing on the Photon and Neutron Hypotheses" (1932); "Cosmic-Ray Intensities in the Stratosphere" (1933); "New Results on Cosmic Rays" and "New and Views" In Supplement to Nature, No. 3036, Vol. 121, Jan. 7, 1928 pp. 19-26 and 29-30; "History of Research in Cosmic Rays" In Nature, No. 3166, Vol. 126, Saturday, July 5, 1930, pp. 14-16.

In the 1920's Millikan also began an increasingly intensive program of research into the penetrating radiation which in mid-decade he would name "cosmic rays." In 1912 the Austrian-born physicist Victor Hess had found that atmospheric ionization increased with altitude up to 12,000 feet. But although Hess had argued that some kind of radiation was coming from the heavens, most physicists still attributed the phenomenon to some terrestrial cause, such as electrical discharges from thunderstorms or radioactivity. Millikan's initial experiments in the field, done with an unmanned sounding balloon in 1922 to a height of fifteen kilometers and with lead-schielded electroscopes atop Pike's Peak in 1923, failed to decide in favor of either interpretation. In the summer of 1925 Millikan proposed to settle the question by measuring the variation of ionization with depth in Muir Lake and Lake Arrowhead in the mountains of California. Snow-fed and separated by many miles, as well as 6,675 feet of atmosphere, each was likely to be free of both local radioactive disturbances and whatever atmospheric peculiarities might affect the ionization in the other. Millikan's electroscopic measurements showed that the intensity of ionization at any given depth in lake Arrowhead was the same as the intensity six feet lower in Muir Lake. Since the layer of atmosphere between in surfaces of the two lakes had precisely the absorptive power of six feet of water, the results decisively confirmed that the radiation was coming from cosmos. Moreover, since the intensity of the ionization showed no diurnal variation, the radiation was uniformly distributed over all directions in space. And, Finally, since Millikan detected ionization as far below the top of the atmosphere as the combined air and water equivalent of six feet of lead, it was evident that cosmic rays were a good deal more energetic than even the hardest known gamma rays. (DSB Vol. 9, pp. 397-398). The Nobel Prize in Physics 1923 was awarded to Robert A. Millikan "for his work on the elementary charge of electricity and on the photoelectric effect". 
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