A large area cosmic muon detector located at Ohya stone mine

Details A large area cosmic muon detector located at Ohya stone mine A large area cosmic muon detector located at Ohya stone mine

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8...16n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 16-19 (SEE N85-36066 24-93)

Computer Science

Chemical Composition, Cosmic Ray Showers, Muons, Point Sources, Angular Resolution, Gamma Ray Telescopes, Scintillation Counters

Scientific paper

The chemical composition of the primary cosmic rays between 10 to the 15th power eV and 10 to the 18th power eV were determined by a Large Area Cosmic Muon Detector located at Ohya stone mine. The experimental aims of Ohya project are; (1) search for the ultra high-energy gamma-rays; (2) search for the GUT monopole created by Big Bang; and (3) search for the muon bundle. A large number of muon chambers were installed at the shallow underground near Nikko (approx. 100 Km north of Tokyo, situated at Ohya-town, Utsunomiya-city). At the surface of the mine, very fast 100 channel scintillation counters were equipped in order to measure the direction of air showers. These air shower arrays were operated at the same time, together with the underground muon chamber.

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