The Washington Large Area Time Coincidence Array
| dc.creator | Cramer, J. G. | |
| dc.creator | Elliott, S. R. | |
| dc.creator | Wilkerson, J. F. | |
| dc.creator | Wilkes, R. J. | |
| dc.creator | Zager, E. | |
| dc.date | 1999-09-15 | |
| dc.date.accessioned | 2026-07-07T02:33:18Z | |
| dc.date.available | 2026-07-07T02:33:18Z | |
| dc.description | The number and density of schools in the Seattle area is convenient for the study of distributed particle showers produced at the top of the atmosphere by ultra-high energy (about $10^{20}$ eV) cosmic rays. We are forming a collaboration for the development of a distributed detector network to study air showers from such ultra-high energy cosmic rays. We call the cosmic ray measurement component WALTA (WAshington Large-area Time-coincidence Array). WALTA aims to provide teachers and students the opportunity to become active participants in forefront scientific projects. A cornerstone of the program will be to install a measurement module at each participating school. | |
| dc.description | 4 pages, 1 figure | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9909268 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9909268 | |
| dc.identifier | Proc 26th ICRC (Salt Lake City, 1999) 4, 341 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14787 | |
| dc.subject | Astrophysics | |
| dc.title | The Washington Large Area Time Coincidence Array | |
| dc.type | text |