Energetic delayed hadrons in large air showers observed at 5200m above sea level
| dc.contributor.author | T. Kaneko | |
| dc.contributor.author | K. Hagiwara | |
| dc.contributor.author | H. Yoshii | |
| dc.contributor.author | N. Martinić | |
| dc.contributor.author | L. Siles | |
| dc.contributor.author | P. Miranda | |
| dc.contributor.author | F. Kakimoto | |
| dc.contributor.author | I. Tsuchimoto | |
| dc.contributor.author | N. Inoue | |
| dc.contributor.author | K. Suga | |
| dc.coverage.spatial | Bolivia | |
| dc.date.accessioned | 2026-03-22T17:00:48Z | |
| dc.date.available | 2026-03-22T17:00:48Z | |
| dc.date.issued | 1985 | |
| dc.description.abstract | Energetic delayed hadrons in air showers with electron sizes in the range 10 to the 6th power to 10 to the 9th power were studied by observing the delayed bursts produced in the shield of nine square meter scintillation detectors in the Chacaltaya air-shower array. The frequency of such delayed burst is presented as a function of electron size, core distance and sec theta. | |
| dc.identifier.uri | https://andeanlibrary.org/handle/123456789/61647 | |
| dc.language.iso | en | |
| dc.source | Okayama University | |
| dc.subject | Physics | |
| dc.subject | Nuclear physics | |
| dc.subject | Hadron | |
| dc.subject | Range (aeronautics) | |
| dc.subject | Air shower | |
| dc.subject | Electron | |
| dc.subject | Scintillation | |
| dc.subject | Astrophysics | |
| dc.subject | Environmental science | |
| dc.subject | Cosmic ray | |
| dc.title | Energetic delayed hadrons in large air showers observed at 5200m above sea level | |
| dc.type | article |