Abstract
The Tunka-13 EAS array has operated two winter seasons since 1996 until 1998 years. It consists of 13 Cherenkov light detectors based upon the QUASAR-370 phototubes. The array covers the area 240 x240 m2 and measures the primary energy, derived from Cherenkov light flux, and individual lateral distribution functions (LDF). Good energy and angular resolution of the array permits to study the irregularities in energy spectrum following the classic “knee”.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.