Experimental results obtained from Pamir emulsion chamber by the Lodz University Group

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Cosmic Rays

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The experimental results obtained by the Lodz group of Pamir Colloboration are presented here. The gamma-quantum and hadron energy spectra and qγ-distribution are compared with calculations of cascade development in the atmosphere. The gamma-energy spectrum and halo intensity can be interpreted as no change of interaction in the fragmentation region. In the central region the change of interaction is observed. The possibility of explaining experimental data by the two-component model is also considered.

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