Underground measurements on secondary cosmic rays

Details Underground measurements on secondary cosmic rays Underground measurements on secondary cosmic rays

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8..175w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 175-178 (SEE N85-36066 24-93)

Computer Science

1

Anisotropy, Cosmic Rays, Detection, Secondary Emission, Computer Techniques, Distribution (Property), Particle Interactions, Resolution

Scientific paper

Measurements made at the Poatina cosmic ray station (41.8 S 149.9 E, 347 m.w.e.) from August 1983 to July 1984 are summarized. The cosmic ray primary particles responsible for events detected at the station have a median primary energy of 1.2 TeV. The motivation for part of this work came from the reported detection of narrow angle anisotropies in the arrival direction of cosmic rays.

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