A. Belov
Moscow State University
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Featured researches published by A. Belov.
Advances in Space Research | 2017
A. Belov; Mario E. Bertaina; Francesca Capel; Federico Fausti; Francesco Fenu; P. A. Klimov; Marco Mignone; Hiroko Miyamoto
Abstract The Mini-EUSO telescope is designed by the JEM-EUSO Collaboration to observe the UV emission of the Earth from the vantage point of the International Space Station (ISS) in low Earth orbit. The main goal of the mission is to map the Earth in the UV, thus increasing the technological readiness level of future EUSO experiments and to lay the groundwork for the detection of Extreme Energy Cosmic Rays (EECRs) from space (Ebisuzaki et al., 2014). Due to its high time resolution of 2.5u202fμs, Mini-EUSO is capable of detecting a wide range of UV phenomena in the Earth’s atmosphere. In order to maximise the scientific return of the mission, it is necessary to implement a multi-level trigger logic for data selection over different timescales. This logic is key to the success of the mission and thus must be thoroughly tested and carefully integrated into the data processing system prior to the launch. This article introduces the motivation behind the trigger design and details the integration and testing of the logic.
Advances in Space Research | 2017
Francesca Capel; A. Belov; M. Casolino; P. A. Klimov
Abstract The Mini-EUSO instrument is a UV telescope to be placed inside the International Space Station (ISS), looking down on the Earth from a nadir-facing window in the Russian Zvezda module. Mini-EUSO will map the earth in the UV range (300–400xa0nm) with a spatial resolution of 6.11xa0km and a temporal resolution of 2.5xa0μs, offering the opportunity to study a variety of atmospheric events such as transient luminous events (TLEs) and meteors, as well as searching for strange quark matter and bioluminescence. Furthermore, Mini-EUSO will be used to detect space debris to verify the possibility of using a EUSO-class telescope in combination with a high energy laser for space debris remediation. The high-resolution mapping of the UV emissions from Earth orbit allows Mini-EUSO to serve as a pathfinder for the study of Extreme Energy Cosmic Rays (EECRs) from space by the JEM-EUSO collaboration.
Proceedings of Topical Workshop on Electronics for Particle Physics — PoS(TWEPP-17) | 2018
Federico Fausti; Mario E. Bertaina; Hiroko Miyamoto; Francesco Fenu; Marco Mignone; Stefano Durando; Daniele D'ago; Francesca Capel; A. Belov; P. A. Klimov
As a pathfinder for the JEM-EUSO mission, Mini-EUSO is a 25cm diameter telescope which is going to be launched and positioned inside the International Space Station (ISS) in 2018. The main scientific goal of this mission is the achievement of a state-of-the-art UV map of the Earth from a 400 Km altitude, with
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
M. Casolino; M. Bertaina; A. Belov; Tosikazu Ebisuzaki; Masaki Fukushima; P. A. Klimov; M. I. Panasyuk; Piergiorgio Picozza; H. Sagawa; Kenji Shinozaki
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Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Francesca Capel; A. Belov; Mario E. Bertaina; Federico Fausti; Hiroko Miyamoto
km of pixel spatial resolution, collecting data though a multi-level triggering system. The signal is collected with Multi-Anode Photo Multiplier Tubes (MAPMTs) and digitized by means of custom chips. The raw data moves then to a central system, the Zynq Board, where the trigger operates a data selection dividing different classes of events characterized by specific time scales. The acquired UV map will be used as discrimination threshold for the Extreme Energy Cosmic-Ray detection.
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
M. Casolino; A. Belov; M. Bertaina; G. Cambie; Francesca Capel; Tosikazu Ebisuzaki; P. A. Klimov; M. I. Panasyuk; Piergiorgio Picozza; M. Ricci
The study of Ultra High Energy Cosmic Rays (UHECRs) offers unique possibilities to probe the energies currently inaccessible by man-made accelerators. The last years have shed light on several characteristics of these particles, but - due to their extremely low flux - their origin, nature and acceleration mechanisms are still unclear. K-EUSO will be the detector to perform measurement of the flux of UHECR from space, covering and comparing the spectra of both northern and southern hemispheres. In this work we will discuss the science capabilities of the detector.
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
P. A. Klimov; A. Belov; Francesca Capel; Mario E. Bertaina; Federico Fausti; Marco Mignone
The Mini-EUSO telescope is designed by the JEM-EUSO Collaboration to observe the UV emission of the Earth from the vantage point of the International Space Station in low Earth orbit. The main goal ...
Physics Letters A | 2012
A. Belov; V. V. Eremin
The Mini-EUSO space experiment (``UV atmosphere in Russian Space Program) is a telescope designed to perform observations of night-time Earth in the UV spectrum. The instrument comprises a compact telescope with a large field of view (44 degrees), based on an optical system employing two 25 cm diameter Fresnel lenses (focal length