Dumand as muon detector
- 1. Moskovskij Fiziko-Tekhnicheskij Inst. (USSR)
Description
Recent discussions of the DUMAND project have dealt with the programme of neutrino experiments only. At the same time DUMAND gives a unique possibility for the investigations of cosmic ray muons with energies greater than 1013 eV. The size of the detector allows to measure the muon energy spectrum up to 1015 eV, where the change of the muon spectrum connected with the direct muon production and the break in the primary spectrum at about 3x1015 eV should be observed. The large thickness of the detector makes it possible to use the method of the muon energy measurement based on the multiplicative pair production by muons. The accuracy of about 25% may be obtained with the 1 km water thick detector. The large number of muons penetrating a sensitive volume (approximately 109 per year) gives the possibility of the study of the muon arrival direction anisotropy and the time variation of the muor flux. (author)
Additional details
Publishing Information
- Imprint Title
- Fifteenth international cosmic ray conference, v. 6, MN session
- Journal Page Range
- p. 289-294.
- Report number
- INIS-mf--4752
Conference
- Title
- 15. International cosmic ray conference.
- Dates
- 13 - 26 Aug 1977.
- Place
- Plovdiv, Bulgaria.
INIS
- Country of Publication
- Bulgaria
- Country of Input or Organization
- Bulgaria
- INIS RN
- 10439347
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ABSORPTION; ABSORPTION SPECTRA; BACKGROUND RADIATION; COSMIC RAY FLUX; COSMIC SHOWERS; ENERGY SPECTRA; MUON DETECTION; MUONS; NEUTRINOS; PAIR PRODUCTION; PARTICLE DECAY; PRIMARY COSMIC RADIATION; TEV RANGE; UNDERWATER
- Descriptors DEC
- CHARGED PARTICLE DETECTION; COSMIC RADIATION; DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; LEVELS; MASSLESS PARTICLES; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; RADIATION DETECTION; RADIATION FLUX; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS; SPECTRA