Abstract
We discuss the feasibility of a telescope consisting in a sampling array for extensive air showers measure combined with a muon tracking device. The sampling array will extend over a surface of ≥107 m2 while the muon tracking device will cover ≥104 m2. The telescope should be done with resistive plates counters and would become a very powerful device to study high-energy neutrinos and gamma-ray astronomy as well as cosmicray physics up to the highest energy (≥1019 eV) region.
Original language | English |
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Pages (from-to) | 321-336 |
Number of pages | 16 |
Journal | Nuovo Cimento della Societa Italiana di Fisica C |
Volume | 13 |
Issue number | 2 |
DOIs | |
Publication status | Published - Mar 1990 |
Externally published | Yes |
Keywords
- Muons and neutrinos