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Intensities of high-energy cosmic rays at Mount KanbalaThe energy spectra of atmospheric cosmic rays at Mt. Kanbala (520 g/sq cm.) are measured with emulsion chambers. The power indexes of the spectra are values of about 2.0 for both gamma-rays and hadrons. Those fluxes are consistent with the ones expected from the model of primary cosmic rays with heavy nuclei of high content in the energy around 10 to the 15th power eV.
Document ID
19850027589
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ren, J. R. (Academia Sinica Beijing, China)
Kuang, H. H. (Academia Sinica Beijing, China)
Huo, A. X. (Academia Sinica Beijing, China)
Lu, S. L. (Academia Sinica Beijing, China)
Su, S. (Academia Sinica Beijing, China)
Wang, Y. X. (Academia Sinica Beijing, China)
Xue, Y. G. (Academia Sinica Beijing, China)
Wang, C. R. (Shangdong Univ. Jinan, China)
He, M. (Shangdong Univ. Jinan, China)
Zhang, N. J. (Shangdong Univ. Jinan, China)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 6
Subject Category
Space Radiation
Report/Patent Number
HE-3.1-2
Accession Number
85N35902
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850027535Collected WorksNineteenth International Cosmic Ray Conference. HE Sessions, Volume 6
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