Cosmic ray showers at large zenith angles
A large vertical array of muon detectors, of sensitive area 34 square metres, has been constructed and used to determine the frequency of observation of groups of coincident muons in E.A.S. as a function of the zenith angle and of the number of muons in the group. These observations are compared wit...
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Durham University
1969
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.585895 |