Speaker
Mrs
Saba Mortazavi Moghaddam
(Semnan University)
Description
The first phase of the Alborz Observatory Array (Alborz-I) is designed to have 20 scintillation detectors to study the cosmic ray spectrum in the energy range of $10^{12}$ eV to $10^{16}$ eV. In order to collect data under stable environmental conditions, a sub-array consists of 5 plastic scintillation detectors on a pentagon with side of 5 m similar to the central cluster of the Alborz-I have been operational since February 2014. This paper studies angular distribution of detected showers and the angular resolution of the sub-array with comparing to the simulated results.
| Collaboration | -- not specified -- |
|---|---|
| Registration number following "ICRC2015-I/" | 158 |
Primary author
Mrs
Saba Mortazavi Moghaddam
(Semnan University)
Co-authors
Dr
Gohar Rastegarzadeh
(Semnan University)
Dr
Mahmud Bahmanabadi
(Sharif University of Technology, Alborz Observatory)
Ms
Soheila Abdollahi
(Alborz Observatory, Sharif University of Technology)
