particle, but do depend on the depth of observation Aa#39; and on the depth Xm of shower maximum. ... to the arrival time of the shower core reflect the pathlength distribution of the muon travel from locus of production (near the axis) to the observation locus. ... Here X is slant depth at the observation level Xv (the vertical atmospheric thickness Xv) dT/dlog1QEv\x = DedT/dXm\x The change of T with the energyanbsp;...
|Author||:||International Union of Pure and Applied Physics, Dublin Institute for Advanced Studies|