Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....8...47k&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 8 p 47-49 (SEE N85-36066 24-93)
Physics
Background Radiation, Cosmic Rays, Flux (Rate), Muons, Time Of Flight Spectrometers, Electron Photon Cascades, Scintillation Counters, Zenith
Scientific paper
There are some discrepancies among the data of absolute muon intensities at large zenth angles. Through the analysis of the data obtained in the previous measurement by Nagoya Cosmic Ray Spectrometer, one of the sources of these discrepancies has been found to be the ambiguity induced by the selection criteria with which genuine muons are distinguished from the backgrounds. To remove the ambiguity of this kind, it is necessary to know the amount of the backgrounds and their characteristics in detail. Some features of the background events were reported from the observations by using this triggering system of Nagoya Cosmic Ray Spectrometer. In this paper, the results of extended observations using track detector together with this system are reported.
Iida Sanae
Iijima Kazuto
Kamiya Yasuomi
Shibata Shinpei
No associations
LandOfFree
The Nagoya cosmic-ray muon spectrometer 3, part 1: Preliminary observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Nagoya cosmic-ray muon spectrometer 3, part 1: Preliminary observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Nagoya cosmic-ray muon spectrometer 3, part 1: Preliminary observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-759304