Abstract
Both the penetrating power of the cosmic rays through material absorbers and their ability to reach the earth in spite of its magnetic field, make it certain that the energy of many of the primary particles must reach at least 10
11
e-volts. However, the energy measurements by Kunze, and by Anderson, using cloud chambers in strong magnetic fields, have extended only to about 5 x 10
9
e-volts. Particles of greater energy were reported, but the curvature of their tracks was too small to be measured with certainty. We have extended these energy measurements to somewhat higher energies, using a large electro-magnet specially built for the purpose and described in Part I. As used in these experiments, the magnet allowed the photography of tracks 17 cm long in a field of about 14,000 gauss. The magnet weighed about 11,000 kilos and used a power of 25 kilowatts.
Cited by
27 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. References;Radioactivity;2016
2. References;Radioactivity;2007
3. The “Magnet House” and the Muon;Early History of Cosmic Ray Studies;1985
4. Theoretische Gesichtspunkte zur Deutung der kosmischen Strahlung;Scientific Review Papers, Talks, and Books Wissenschaftliche Übersichtsartikel, Vorträge und Bücher;1984
5. Interactions of FastμMesons in Lead with Small-Energy Transfer;Physical Review;1960-06-01