ENERGY SPECTRUM AND STRUCTURE OF LARGE AIR SHOWERS

摘要: Nineteen 3.3-m/sup 2/ plastic scintillation detectors in a hexagonal array covering 2 km/sup were used this study. Methods of recording and analyzing data are discussed, results presented on the following: lateral distribution particle density, proportion penetrating particles, variation shower intensity size with atmospheric depth, primary cosmic ray energy spectrum, isotropy radiation, largest recorded. (A.G.W.)