An approach to study the cosmic ray 'knee' composition from underground multimuon events at a shallower depth.

Details An approach to study the cosmic ray 'knee' composition from underground multimuon events at a shallower depth. An approach to study the cosmic ray 'knee' composition from underground multimuon events at a shallower depth.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hepnp..23..584d&link_type=abstract

High Energ. Phys. Nucl. Phys., Vol. 23, No. 6, p. 584 - 588

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Cosmic Rays: Composition, Cosmic Rays: Muons

Scientific paper

The observation of underground multimuon phenomena is an important way for the study of the cosmic ray composition in the 'knee' region (1015 - 1016eV). It is noticed that the existing underground detectors are not very ideal for the composition study because they were originally designed mainly for other aims. A new approach having higher sensitivity for this study by observing multimuon events using a detector array in a shallower depth underground is presented.

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