A System for Generating the Trigger Signals of the Spaceborne GAMMA-400 Telescope


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Аннотация

The GAMMA-400 space project is one of the new generation of space observatories designed to search for signs of dark matter in the cosmic gamma emission, and to measure the characteristics of diffuse gamma-ray emission and gamma-rays from the Sun during periods of solar activity; gamma-ray bursts; extended and point gamma-ray sources; and electron, positron, and cosmic-ray nuclei fluxes with energies in the TeV ranges. The GAMMA-400 γ-ray telescope constitutes the core of the scientific instrumentation. The nature of the intended experiments imposes stringent requirements on the gamma telescope’s system of trigger signal formation, now being developed using the state-of-the-art logic devices and fast data links. The design concept of the system is discussed, along with the chosen engineering solutions and some experimental results obtained during the operation of the system prototype using a positron beam with energies of 100–300 MeV from the PAKHRA S-25R synchrotron at the Lebedev Physical Institute.

Авторлар туралы

A. Arkhangelskiy

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Хат алмасуға жауапты Автор.
Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991; Moscow, 115409

A. Galper

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991; Moscow, 115409

I. Arkhangelskaja

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 115409

A. Bakaldin

Lebedev Physical Institute, Russian Academy of Sciences; Scientific Research Institute of System Analysis, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991; Moscow, 117218

Yu. Gusakov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

O. Dalkarov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

A. Egorov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

V. Zverev

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

A. Leonov

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991; Moscow, 115409

N. Pappe

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

M. Runtso

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 115409

Yu. Stozhkov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

S. Suchkov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

N. Topchiev

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991

M. Kheymits

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 115409

E. Chasovikov

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 115409

I. Chernysheva

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 119991; Moscow, 115409

Yu. Yurkin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Ресей, Moscow, 115409

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