Abstract
In the high-energy region, the spectra of cosmic ray particles are measured using calorimeters and particle charge detectors. Particles flying in the directions opposite to those of the cascade development (backscattered flux) can distort the results of such experiments [1, 2]. In this paper, by the example of the particle charge detector and the PAMELA spectrometer calorimeter, the contribution of the backscattered particle flux when determining the primary particle charge as well as determining its energy in the calorimeter is estimated.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
