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MEMS space Telescope for the observation of Extreme Lightening (MTEL)
Park, Jae-Hyoung,Garipov, Garik,Jeon, Jin-A,Jin, Joo-Young,Jung, Ae-Ra,Kim, Ji-Eun,Kim, Min-Soo,Kim, Yong-Kweon,Klimov, Pavel,Khrenov, Boris,Lee, Chang-Hwan,Lee, Jik,Na, Go-Woon,Nam, Ji-Woo,Nam, Shin- 한국우주과학회 2009 한국우주과학회보 Vol.18 No.1
MEMS space Telescope for the observation of Extreme Lightening (MTEL)
Jae-Hyoung Park,Garik Garipov,Jin-A Jeon,Joo-Young Jin,Aera Jung,Ji-Eun Kim,Minsoo Kim,Yong-Kweon Kim,Pavel Klimov,Boris Khrenov,Chang-Hwan Lee,Jik Lee,Go-Woon Na,Jiwoo Nam,Shinwoo Nam,Il-Heung Park,Y 한국천문학회 2009 天文學會報 Vol.34 No.1
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>
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.
Kim, Ji Eun,Lee, Jik,Park, A. H.,Park, I. H.,Garipov, G. K.,Khrenov, B. A.,Klimov, P. A.,Panasyuk, M. I. 한국물리학회 2014 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol. No.
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 energies above 5 x 10(19) 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 pinhole cameras as auxiliary instrumentation to detect and efficiently distinguish TLEs from UHECRs. Each pinhole camera contains a MAPMT (multi-anode photo-multiplier tube) and its associated analog and digital electronics. The R11265-03-M64 MAPMT has been custom-made for space applications by Hamamatsu Photonics, particularly for the future EUSO (Extreme Universe Space Observatory) UHECR space mission. Thus, the TUS pinhole system will be the test bench for the deployment in space of a large number, similar to 5000, of MAPMTs. In this study, we present the design and fabrication of the pinhole cameras, and we estimate the detectability of TLEs with respect to atmospheric light background.
“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>
A New Type of Space Telescope for Observation of Extreme Lightning Phenomena in the Upper Atmosphere
Lee, J.,Kim, J. E.,Na, G. W.,Jeon, J. A.,Jeong, S.,Jung, A.,Lee, H. Y.,Nam, J. W.,Suh, J. E.,Garipov, G.,Klimov, P.,Khrenov, B. A.,Panasyuk, M. I.,Vedenkin, N. N.,Park, I. H. IEEE 2012 IEEE transactions on geoscience and remote sensing Vol.50 No.10
<P>A new type of space telescope with a 3 mm × 3 mm Micro-Electro-Mechanical System (MEMS) micromirror array has been fabricated and launched into space. This telescope has unique features: a wide field of surveillance view, and fast zoom-in and tracking capabilities. Although the micromirror array area is small, the space telescope was capable of observing the space-time development of extreme lightning in the upper atmosphere. It fulfilled its purpose by proving the principles of a space telescope. The concept and technologies used in this telescope can be extended to large MEMS space telescopes for future missions for earth and space science, including gamma ray bursts and ultra high energy cosmic rays. The performance of the space telescope during the ground test before launch as well as its performance in space are here presented to demonstrate the fast zoom-in and tracking capabilities of the telescope.</P>