10-14 October 2016
Milan Hotel
Europe/Moscow timezone

Gamma-quanta and charged particles recognition by the counting and triggers signals formation system of GAMMA-400 space gamma-telescope

13 Oct 2016, 17:30
15m
Verdi (Milan Hotel)

Verdi

Milan Hotel

Shipilovskaya Street, 28A, Moscow, Russia, 115563
Plenary/section talk Cosmic rays Cosmic rays - parallel VI

Speaker

Mrs. Irene ARKHANGELSKAJA (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute))

Description

GAMMA-400 (Gamma Astronomical Multifunctional Modular Apparatus) parameters are optimized for detection of gamma-quanta with the energy $\sim~100$~GeV in the main aperture. Also there are opportunities to detect particles in additional and lateral apertures. Registered events identification procedures details are discussed in the presented article for gammas, electrons/positrons and protons both in low and high energy bands of 0.2 - 10~MeV in additional and lateral apertures and from ~20~MeV to several TeV in all three ones. It allows providing energy resolution $8\% - 2\%$ for gamma-quanta in low energy region and $~2\%$ for gammas and electrons/positrons in high one.

Primary author

Mrs. Irene ARKHANGELSKAJA (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute))

Co-authors

Mr. Andrey Arkhangelskiy (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)) Prof. Arkady Galper (NRNU MEPhI) Mr. Evgeniy Chasovikov (National Research Nuclear University "MEPhI" (Moscow Engineering Physics Institute)) Mr. Maxim Kheymits (NRNU MEPhI) Dr. Nikolay Topchiev (Lebedev Physical Institute) Dr. Sergey SUCHKOV (LPU) Dr. Yury YURKIN (MEPhI)

Presentation Materials

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