Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T11:53:30.382Z Has data issue: false hasContentIssue false

Features of the High Energy Electron Spectrum

Published online by Cambridge University Press:  14 August 2015

J. Nishimura*
Affiliation:
Institute of Space and Aeronautical Science, University of Tokyo, Tokyo, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent studies of the spectrum of high energy primary electrons using emulsion chambers have been made with an exposure factor some 10 to 100 times larger than those obtained by other experimental devices. The total exposure is now almost 6 m2-day-str., including the recent exposure at Palestine, Texas in May 1980, and it is now quite possible to extend observations of the electron spectrum into the TeV region with reliable accuracy in the next few years.

Type
Research Article
Copyright
Copyright © Reidel 1981 

References

Giler, M., Wdowczyk, J., and Wolfendale, A.W.: 1978, J. Phys., G. 4, 269 1979, Proc. Int. Cosmic Ray Conf., Kyoto, 507.CrossRefGoogle Scholar
Nishimura, J., Fujii, M., and Taira, T.: 1979, Proc. Int. Cosmic Ray Conf. Kyoto, 488, (referred to as Ref. I).Google Scholar
Nishimura, J., et al.: 1980 Ap. J. (in press).Google Scholar
Taira, T., et al.,: 1979, Proc. Int. Cosmic Ray Conf., Kyoto, 478.Google Scholar
Webber, W.R., Goeman, R.A., and Tushak, S.M., 1979, Proc. Int. Cosmic Ray Conf. Kyoto, 495.Google Scholar