Adams JH, Ahmad S, Albert JN, Allard D, Anchordoqui L, Andreev V, Anzalone A, Arai Y, Asano K, Ave Pernas M, Baragatti P, Barrillon P, Batsch T, Bayer J, Bechini R, Belenguer T, Bellotti R, Belov K, Berlind AA, Bertaina M, Biermann PL, Biktemerova S, Blaksley C, Blanc N, Blecki J, Blin-Bondil S, Bluemer J, Bobik P, Bogomilov M, Bonamente M, Briggs MS, Briz S, Bruno A, Cafagna F, Campana D, Capdevielle JN, Caruso R, Casolino M, Cassardo C, Castellini G, Catalano C, Catalano O, Cellino A, Chikawa M, Christl MJ, Cline D, Connaughton V, Conti L, Cordero G, Crawford HJ, Cremonini R, Csorna S, Dagoret-Campagne S, De Castro AJ, De Donato C, De La Taille C, De Santis C, Del Peral L, Dell'Oro A, De Simone N, Di Martino M, Distratis G, Dulucq F, Dupieux M, Ebersoldt A, Ebisuzaki T, Engel R, Falk S, Fang K, Fenu F, Fernandez-Gomez I, Ferrarese S, Finco D, Flamini M, Fornaro C, Franceschi A, Fujimoto J, Fukushima M, Galeotti P, Garipov G, Geary J, Gelmini G, Giraudo G, Gonchar M, Gonzalez Alvarado C, Gorodetzky P, Guarino F, Guzman A, Hachisu Y, Harlov B, Haungs A, Hernandez Carretero J, Higashide K, Ikeda D, Ikeda H, Inoue N, Inoue S, Insolia A, Isgro F, Itow Y, Joven E, Judd EG, Jung A, Kajino F, Kajino T, Kaneko I, Karadzhov Y, Karczmarczyk J, Karus M, Katahira K, Kawai K, Kawasaki Y, Keilhauer B, Khrenov BA, Kim JS, Kim SW, Kim SW, Kleifges M, Klimov PA, Kolev D, Kreykenbohm I, Kudela K, Kurihara Y, Kusenko A, Kuznetsov E, Lacombe M, Lachaud C, Lee J, Licandro J, Lim H, Lopez F, Maccarone MC, Mannheim K, Maravilla D, Marcelli L, Marini A, Martinez O, Masciantonio G, Mase K, Matev R, Medina-Tanco G, Mernik T, Miyamoto H, Miyazaki Y, Mizumoto Y, Modestino G, Monaco A, Monnier-Ragaigne D, Morales De Los Rios JA, Moretto C, Morozenko VS, Mot B, Murakami T, Nagano M, Nagata M, Nagataki S, Nakamura T, Napolitano T, Naumov D, Nava R, Neronov A, Nomoto K, Nonaka T, Ogawa T, Ogio S, Ohmori H, Olinto AV, Orleanski P, Osteria G, Panasyuk MI, Parizot E, Park IH, Park HW, Pastircak B, Patzak T, Paul T, Pennypacker C, Perez Cano S, Peter T, Picozza P, Pierog T, Piotrowski LW, Piraino S, Plebaniak Z, Pollini A, Prat P, Prevot G, Prieto H, Putis M, Reardon P, Reyes M, Ricci M, Rodriguez I, Rodriguez Frias MD, Ronga F, Roth M, Rothkaehl H, Roudil G, Rusinov I, Rybczynski M, Sabau MD, Saez Cano G, Sagawa H, Saito A, Sakaki N, Sakata M, Salazar H, Sanchez S, Santangelo A, Santiago Cruz L, Sanz Palomino M, Saprykin O, Sarazin F, Sato H, Sato M, Schanz T, Schieler H, Scotti V, Segreto A, Selmane S, Semikoz D, Serra M, Sharakin S, Shibata T, Shimizu HM, Shinozaki K, Shirahama T, Siemieniec-Ozieblo G, Silva Lopez HH, Sledd J, Slominska K, Sobey A, Sugiyama T, Supanitsky D, Suzuki M, Szabelska B, Szabelski J, Tajima F, Tajima N, Tajima T, Takahashi Y, Takami H, Takeda M, Takizawa Y, Tenzer C, Tibolla O, Tkachev L, Tokuno H, Tomida T, Tone N, Toscano S, Trillaud F, Tsenov R, Tsunesada Y, Tsuno K, Tymieniecka T, Uchihori Y, Unger M, Vaduvescu O, Valdes-Galiciaga JF, Vallania P, Valore L, Vankova G, Vigorito C, Villasenor L, Von Ballmoos P, Wada S, Watanabe J, Watanabe S, Watts J, Weber M, Weiler TJ, Wibig T, Wiencke L, Wille M, Wilms J, Wlodarczyk Z, Yamamoto T, Yamamoto Y, Yang J, Yano H, Yashin IV, Yonetoku D, Yoshida K, Yoshida S, Young R, Zotov MY, Marchi AZ (2015)
Publication Status: Published
Publication Type: Journal article
Publication year: 2015
Publisher: SPRINGER
Book Volume: 40
Pages Range: 239-251
Journal Issue: 1
DOI: 10.1007/s10686-014-9431-0
The main goal of the JEM-EUSO experiment is the study of Ultra High Energy Cosmic Rays (UHECR, 10(19)-10(21) e V), but the method which will be used (detection of the secondary light emissions induced by cosmic rays in the atmosphere) allows to study other luminous phenomena. The UHECRs will be detected through the measurement of the emission in the range between 290 and 430 m, where some part of Transient Luminous Events (TLEs) emission also appears. This work discusses the possibility of using the JEM-EUSO Telescope to get new scientific results on TLEs. The high time resolution of this instrument allows to observe the evolution of TLEs with great precision just at the moment of their origin. The paper consists of four parts: review of the present knowledge on the TLE, presentation of the results of the simulations of the TLE images in the JEM-EUSO telescope, results of the Russian experiment Tatiana-2 and discussion of the possible progress achievable in this field with JEM-EUSO as well as possible cooperation with other space projects devoted to the study of TLE - TARANIS and ASIM. In atmospheric physics, the study of TLEs became one of the main physical subjects of interest after their discovery in 1989. In the years 1992 - 1994 detection was performed from satellite, aircraft and space shuttle and recently from the International Space Station. These events have short duration (milliseconds) and small scales (km to tens of km) and appear at altitudes 50 - 100 km. Their nature is still not clear and each new experimental data can be useful for a better understanding of these mysterious phenomena.
APA:
Adams, J.H., Ahmad, S., Albert, J.-N., Allard, D., Anchordoqui, L., Andreev, V.,... Marchi, A.Z. (2015). Science of atmospheric phenomena with JEM-EUSO. Experimental Astronomy, 40(1), 239-251. https://dx.doi.org/10.1007/s10686-014-9431-0
MLA:
Adams, J. H., et al. "Science of atmospheric phenomena with JEM-EUSO." Experimental Astronomy 40.1 (2015): 239-251.
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