Abstract
Ultra high energy cosmic rays are detected via extensive air shower produced in the atmosphere which is measured by various techniques. In case of the geometric arrangement of the ground detectors, it is important to reconstruct the core location of the air shower, for accurate measurement of the energy of the primary cosmic ray particle. In this presentation, we report a new method to find the shower core position in a large-scale ground detector array.
Original language | English |
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Pages | 125-128 |
Number of pages | 4 |
DOIs | |
Publication status | Published - 2011 |
Event | 32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: 2011 Aug 11 → 2011 Aug 18 |
Other
Other | 32nd International Cosmic Ray Conference, ICRC 2011 |
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Country/Territory | China |
City | Beijing |
Period | 11/8/11 → 11/8/18 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics