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Study of cosmic rays above 0.3 EeV using Fly’s Eye‐muon array coincidence
dc.contributor.authorGreen, K. D.en_US
dc.date.accessioned2011-11-15T16:00:55Z
dc.date.available2011-11-15T16:00:55Z
dc.date.issued1991-04-05en_US
dc.identifier.citationGreen, K. D. (1991). "Study of cosmic rays above 0.3 EeV using Fly’s Eye‐muon array coincidence." AIP Conference Proceedings 220(1): 184-188. <http://hdl.handle.net/2027.42/87434>en_US
dc.identifier.otherAPCPCS-220-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87434
dc.description.abstractThe Fly’s Eye (FE) and the Michigan Muon Array (MA) simultaneously detect Extensive Air Showers (EAS) from EeV Enrgy primaries. Combining data from both experiments during analysis yields a reliable measurement of Depth of Shower Maximum (Xmax), and gives a measurement of the Muon Lateral Distribution (MLD)<1km from the Shower core. The MLD densities agree with previously measured values.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleStudy of cosmic rays above 0.3 EeV using Fly’s Eye‐muon array coincidenceen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUMC Collaboration University of Michigan, Ann Arbor, Michigan 48109en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87434/2/184_1.pdf
dc.identifier.doi10.1063/1.40290en_US
dc.identifier.sourceHigh Energy Gamma−Ray Astronomyen_US
dc.owningcollnamePhysics, Department of


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