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Ch. 1. Introduction -- ch. 2. Historical background. 2.1. The early history of accelerators. 2.2. Accelerator physics in the Midwest. 2.3. The coming of strong focusing. 2.4. The desire for a new accelerator laboratory in the Midwest -- ch. 3. The early MURA years, 1953-1956. 3.1. The beginnings of MURA. 3.2. The invention of FFAG. 3.3. MURA studies. 3.4. Theory of radio frequency acceleration. 3.5. Nonlinear dynamics. 3.6. The radial sector model. 3.7. The spiral sector model. 3.8. MURA computing. 3.9. Colliding beams. 3.10. Collective instabilities. 3.11. Conferences -- ch. 4. The Madison years, 1956-1963. 4.1. Formation of the MURA organization. 4.2. The move to Madison. 4.3. Space charge...
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A thin magnetic lens spectrometer for the investigation of gamma-ray spectra is described. The effect of the thickness of the radiator used for the production of photoelectrons and the influence of the earth's magnetic field are reported. Based on a calibration of the instrument by means of annihilation radiation and the F line of ThB, energy values of 1.106 Mev for the gamma-ray of Zn(65), and 1.155 and 1.317 MeV for the two lines of Co(60) are obtained. The probable error is estimated as 0.5 per cent.
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