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Wide-Field Gamma-Spectrometer BDRG: GRB Monitor On-Board the Lomonosov Mission
Svertilov, S. I.,Panasyuk, M. I.,Bogomolov, V. V.,Amelushkin, A. M.,Barinova, V. O.,Galkin, V. I.,Iyudin, A. F.,Kuznetsova, E. A.,Prokhorov, A. V.,Petrov, V. L.,Rozhkov, G. V.,Yashin, I. V.,Gorbovskoy D. Reidel Pub. Co 2018 Space science reviews Vol.214 No.1
Prompt and Follow-up Multi-wavelength Observations of the GRB 161017A
Sadovnichy, V. A.,Panasyuk, M. I.,Svertilov, S. I.,Lipunov, V. M.,Bogomolov, V. V.,Gorbovskoy, E. S.,Bogomolov, A. V.,Castro-Tirado, A. J.,Gabovich, A.,Hu, Y.,Iyudin, A. F.,Jeong, H. M.,Jeong, S.,Kim, American Astronomical Society 2018 The Astrophysical journal Vol.861 No.1
<P>This paper presents data on the simultaneous and complementary observations of the gamma-ray burst (GRB) GRB 161017A for optical, X-ray, and gamma wavelengths obtained by the Russian multi-messenger Lomonosov space observatory and supplemented by additional data from the Swift satellite as well as the ground-based MASTER Global Robotic Net and the 10 m Gran Telescopio Canarias. Multifrequency spectra of this very powerful explosion indicate that it originated at a distance of 10 billion light years from Earth. Here, we present the results of the prompt, early, and afterglow optical observations. The light curves and spectra suggest that the prompt optical and high-energy emissions occur in the same region near the GRB source.</P>
The TUS Detector of Extreme Energy Cosmic Rays on Board the Lomonosov Satellite
Klimov, P. A.,Panasyuk, M. I.,Khrenov, B. A.,Garipov, G. K.,Kalmykov, N. N.,Petrov, V. L.,Sharakin, S. A.,Shirokov, A. V.,Yashin, I. V.,Zotov, M. Y.,Biktemerova, S. V.,Grinyuk, A. A.,Grebenyuk, V. M. Springer-Verlag 2017 Space science reviews Vol.212 No.3
<P>It will also be able to register slower atmospheric transient events: atmospheric fluorescence in electrical discharges of various types including precipitating electrons escaping the magnetosphere and from the radiation of meteors passing through the atmosphere. We describe the design of the TUS detector and present results of different ground-based tests and simulations.</P>
Slewing mirror telescope of the UFFO-pathfinder: first report on performance in space
Gaikov, G.,Jeong, S.,Agaradahalli, V. G.,Park, I. H.,Budtz-Jørgensen, C.,Castro-Tirado, A. J.,Chen, P.,Jeong, H. M.,Kim, J. E.,Kim, M. B.,Kim, S. W.,Lee, J.,Leonov, V.,Nam, J. W.,Panasyuk, M. I.,Petro The Optical Society 2017 Optics express Vol.25 No.23
UFFO/Lomonosov: The Payload for the Observation of Early Photons from Gamma Ray Bursts
Park, I. H.,Panasyuk, M. I.,Reglero, V.,Chen, P.,Castro-Tirado, A. J.,Jeong, S.,Bogomolov, V.,Brandt, S.,Budtz-Jørgensen, C.,Chang, S.-H.,Chang, Y. Y.,Chen, C.-R.,Chen, C.-W.,Choi, H. S.,Connell, P.,E Springer-Verlag 2018 Space science reviews Vol.214 No.1
UBAT of UFFO/Lomonosov: The X-Ray Space Telescope to Observe Early Photons from Gamma-Ray Bursts
Jeong, S.,Panasyuk, M. I.,Reglero, V.,Connell, P.,Kim, M. B.,Lee, J.,Rodrigo, J. M.,Ripa, J.,Eyles, C.,Lim, H.,Gaikov, G.,Jeong, H.,Leonov, V.,Chen, P.,Castro-Tirado, A. J.,Nam, J. W.,Svertilov, S.,Ya Springer-Verlag 2018 Space science reviews Vol.214 No.1
NEUTRON FIELD OF THE EARTH, ORIGIN AND DYNAMICS
Kuzhevshkij, B.M.,Nechaev, O.Yu.,Panasyuk, M.I.,Sigaeva, E.A.,Volodichev, N.N.,Zakharov, V.A. 대한방사선 방어학회 2001 방사선방어학회지 Vol.26 No.3
It is shown, that both cosmic radiation (external source) and natural radioactive gases (inner source) are sources of neutrons near the Earth crust. Correlation between the Earth crust dynamics and variations of thermal and slow neutron flux near the Earth surface is studied. It is shown, that variations of neutron flux near the Earth crust can be used for short-term predicting of natural hazards.
“Lomonosov” Satellite—Space Observatory to Study Extreme Phenomena in Space
Sadovnichii, V. A.,Panasyuk, M. I.,Amelyushkin, A. M.,Bogomolov, V. V.,Benghin, V. V.,Garipov, G. K.,Kalegaev, V. V.,Klimov, P. A.,Khrenov, B. A.,Petrov, V. L. Springer Science + Business Media 2017 Space science reviews Vol.212 No.3
<P>This paper is directed towards the general description of both scientific goals of the project and scientific equipment on board the satellite. The following papers of this issue are devoted to detailed descriptions of scientific instruments.</P>
Jieun Kim,Jik Lee,A. H. Park,I. H. Park,G. K. Garipov,B. A. Khrenov,P. A. Klimov,M. I. Panasyuk 한국물리학회 2014 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.64 No.5
The TUS (tracking ultraviolet setup) experiment is intended for the observation from space of ultraviolet(UV) fluorescence induced both by ultra-high-energy cosmic rays (UHECRs) with energiesabove 5 × 1019 eV and by transient luminous events (TLEs) occurring in the upper atmosphere. These two types of events are very different in terms of duration, lateral shape, and intensity; thus,each behaves as a background for the other. The TUS is equipped with two conventional pinholecameras as auxiliary instrumentation to detect and efficiently distinguish TLEs from UHECRs. Each pinhole camera contains a MAPMT (multi-anode photo-multiplier tube) and its associatedanalog and digital electronics. The R11265-03-M64 MAPMT has been custom-made for space applicationsby Hamamatsu Photonics, particularly for the future EUSO (Extreme Universe SpaceObservatory) UHECR space mission. Thus, the TUS pinhole system will be the test bench for thedeployment in space of a large number, 5000, of MAPMTs. In this study, we present the designand fabrication of the pinhole cameras, and we estimate the detectability of TLEs with respect toatmospheric light background.