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 |
|---|---|
| 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