Published online by Cambridge University Press: 24 October 2008
During the course of a cloud chamber investigation of the occurrence of rare events accompanying the passage of fast β-particles through matter, it was found* that existing methods of introducing high-energy electrons into the chamber were unsatisfactory. Electrons of sufficiently high energy could only be obtained from sources which emit, in addition, a large amount of γ-radiation. Absorption of this γ-radiation in the walls and gas of the chamber resulted in the ejection of numbers of stray electrons, whose presence rendered the observation of the fast β-ray tracks a matter of some difficulty.
* By one of us (W. T. D.) with the collaboration of M. A. Fromageot.
† Ho, P. C., Proc. Camb. Phil. Soc. 31 (1934), 119.CrossRefGoogle Scholar
‡ Terroux, and Alexander, , Proc. Camb. Phil. Soc. 28 (1931), 115.CrossRefGoogle Scholar
§ While this work was in progress a description was given by Staub (Helv. Phys. Acta, 9 (1936), 306–16Google Scholar) of a solenoidal electron lens used in conjunction with a Wilson chamber. Many of the considerations studied hereafter do not apply to his arrangement.
∥ Klemperer, , Phil. Mag. 20 (1936), 545.CrossRefGoogle Scholar
* Busch, , Arch. Elektrotechnik, 18 (1927), 583CrossRefGoogle Scholar; Henriot, , Revue, d'optique, 14 (1935), 146.Google Scholar
* The focused electrons were assumed to have energies distributed between 1 and 2·5 M.V. An energy equivalent to Hp = 7000 is a rough mean value.
* Since the beam of electrons has a width of several cm. φ will vary appreciably (~ 20°) from one edge of the beam to the other.
* The focal length could not be decreased sufficiently, and it was inconvenient to lengthen the tube. A larger object distance would result in the permissible divergence being exceeded.