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相关论文: EUSO-TA fluorescence detector

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EUSO-TA is a ground-based florescence detector built to validate the design of an ultra-high energy cosmic ray fluorescence detector to be operated in space. EUSO-TA detected the first air shower events with the technology developed within…

EUSO-TA is a ground-based telescope, located at the Black Rock Mesa site of Telescope Array (TA), Utah, USA. The main aim of the instrument is observation of Ultra High Energy Cosmic Rays through detection of ultraviolet light generated by…

高能天体物理现象 · 物理学 2019-09-23 Lech Wiktor Piotrowski

EUSO--TA is a ground-based telescope installed in 2013 in the Black Rock Mesa Telescope Array (BRM-TA) site, operating with 2.5$\mu$s time resolution to observe the night sky in the UV range. The optical system contains two 1m$^2$ Fresnel…

天体物理仪器与方法 · 物理学 2023-09-19 Zbigniew Plebaniak

The EUSO-TA ground-based fluorescence detector of the JEM-EUSO program, which operates at the Telescope Array (TA) site in Utah (USA), is being upgraded. In the previous data acquisition campaigns, it detected the first nine ultra-high…

天体物理仪器与方法 · 物理学 2023-09-22 Francesca Bisconti

EUSO-TA is a ground-based experiment, placed at Black Rock Mesa of the Telescope Array site as a part of the JEM-EUSO (Joint Experiment Missions for the Extreme Universe Space Observatory) program. The UV fluorescence imaging telescope with…

The Extreme Universe Space Observatory-Telescope Array (EUSO-TA) is a ground-based experiment, part of the JEM-EUSO (Joint Experiment Missions -- Extreme Universe Space Observatory) dedicated to the observation of Ultra High Energy Cosmic…

天体物理仪器与方法 · 物理学 2019-09-12 Z. Plebaniak , J. Szabelski , M. Przybylak , L. W. Piotrowski , A. Djakonow , K. Krolik

The origin of Ultra-High Energy Cosmic Rays (UHECRs) remains unsolved in contemporary astroparticle physics. The objective of the JEM-EUSO program is the realization of a space mission devoted to UHECR physics. Several detectors have been…

高能天体物理现象 · 物理学 2019-09-27 Francesco Fenu

The JEM-EUSO program aims at detecting Ultra High Energy Cosmic Rays (UHECRs) by observing the fluorescence light produced by extensive air showers (EAS) in the Earth's atmosphere. Within this program, a new generation of missions is being…

天体物理仪器与方法 · 物理学 2019-09-13 M. Battisti , M. Bertaina , F. Fenu , H. Miyamoto , K. Shinozaki , A. Belov , F. Bisconti , M. Mignone , F. Capel

The JEM-EUSO mission aims to explore the origin of the extreme energy cosmic rays (EECRs) through the observation of air-shower fluorescence light from space. The superwide-field telescope looks down from the International Space Station…

天体物理仪器与方法 · 物理学 2015-09-02 Andreas Haungs , JEM-EUSO Collaboration

JEM-EUSO is an international program for the development of space based Ultra High Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. The instruments…

JEM-EUSO is an international collaboration for the development of space--based Ultra High Energy Cosmic Ray (UHECR) detectors. The instrument consists of a wide Field Of View (FOV) camera for the detection of the UV light emitted by…

高能天体物理现象 · 物理学 2017-03-07 Francesco Fenu

Fluorescence telescopes are among the key instruments used for studying ultra-high energy cosmic rays in all modern experiments. We use model data for a small ground-based telescope EUSO-TA to try some methods of machine learning and neural…

天体物理仪器与方法 · 物理学 2025-07-08 Mikhail Zotov , Pavel Zakharov

JEM--EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. All…

天体物理仪器与方法 · 物理学 2023-11-22 S. Abe , J. H. Adams , D. Allard , P. Alldredge , L. Anchordoqui , A. Anzalone , E. Arnone , B. Baret , D. Barghini , M. Battisti , J. Bayer , R. Bellotti , A. A. Belov , M. Bertaina , P. F. Bertone , M. Bianciotto , P. L. Biermann , F. Bisconti , C. Blaksley , S. Blin-Bondil , P. Bobik , K. Bolmgren , S. Briz , J. Burton , F. Cafagna , G. Cambié , D. Campana , F. Capel , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , K. Černý , M. J. Christl , R. Colalillo , L. Conti , G. Cotto , H. J. Crawford , R. Cremonini , A. Creusot , A. Cummings , A. de Castro Gónzalez , C. de la Taille , L. del Peral , R. Diesing , P. Dinaucourt , A. Di Nola , A. Ebersoldt , T. Ebisuzaki , J. Eser , F. Fenu , S. Ferrarese , G. Filippatos , W. W. Finch , F. Flaminio , C. Fornaro , D. Fuehne , C. Fuglesang , M. Fukushima , D. Gardiol , G. K. Garipov , A. Golzio , P. Gorodetzky , F. Guarino , C. Guépin , A. Guzmán , A. Haungs , T. Heibges , J. Hernández-Carretero , F. Isgrò , E. G. Judd , F. Kajino , I. Kaneko , Y. Kawasaki , M. Kleifges , P. A. Klimov , I. Kreykenbohm , J. F. Krizmanic , V. Kungel , E. Kuznetsov , F. López Martínez , S. Mackovjak , D. Mandát , M. Manfrin , A. Marcelli , L. Marcelli , W. Marszał , J. N. Matthews , A. Menshikov , T. Mernik , M. Mese , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A Morales de los Ríos , S. Nagataki , J. M. Nachtman , D. Naumov , A. Neronov , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , Y. Onel , G. Osteria , A. Pagliaro , B. Panico , E. Parizot , I. H. Park , B. Pastircak , T. Paul , M. Pech , F. Perfetto , P. Picozza , L. W. Piotrowski , Z. Plebaniak , J. Posligua , R. Prevete , G. Prévôt , H. Prieto , M. Przybylak , M. Putis , E. Reali , P. Reardon , M. H. Reno , M. Ricci , M. Rodríguez Frías , G. Romoli , G. Sáez Cano , H. Sagawa , N. Sakaki , A. Santangelo , O. A. Saprykin , F. Sarazin , M. Sato , H. Schieler , P. Schovánek , V. Scotti , S. Selmane , S. A. Sharakin , K. Shinozaki , J. F. Soriano , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , M. Takeda , Y. Takizawa , C. Tenzer , S. B. Thomas , L. G. Tkachev , T. Tomida , S. Toscano , M. Traïche , D. Trofimov , K. Tsuno , P. Vallania , L. Valore , T. M. Venters , C. Vigorito , P. von Ballmoos , M. Vrabel , S. Wada , J. Watts , A. Weindl , L. Wiencke , J. Wilms , D. Winn , H. Wistrand , I. V. Yashin , R. Young , M. Yu. Zotov

The JEM-EUSO program is focused on observations of Ultra High Energy Cosmic Rays (UHECRs) from space. For this purpose, a series of detectors based on multi-anode photomultiplier tubes with a time resolution of the order of $\mu$s have been…

天体物理仪器与方法 · 物理学 2023-09-19 Zbigniew Plebaniak , Marika Przybylak

Since 2007, the Telescope Array (TA) experiment, based in Utah, USA, has been observing ultra high energy cosmic rays to understand their origins. The experiment involves a surface detector (SD) array and three fluorescence detector (FD)…

天体物理仪器与方法 · 物理学 2015-06-03 H. Tokuno , Y. Tameda , M. Takeda , K. Kadota , D. Ikeda , M. Chikawa , T. Fujii , M. Fukushima , K. Honda , N. Inoue , F. Kakimoto , S. Kawana , E. Kido , J. N. Matthews , T. Nonaka , S. Ogio , T. Okuda , S. Ozawa , H. Sagawa , N. Sakurai , T. Shibata , A. Taketa , S. B. Thomas , T. Tomida , Y. Tsunesada , S. Udo , T. Abu-zayyad , R. Aida , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J. W. Belz , D. R. Bergman , S. A. Blake , R. Cady , B. G. Cheon , J. Chiba , E. J. Cho , W. R. Cho , H. Fujii , T. Fukuda , D. Gorbunov , W. Hanlon , K. Hayashi , Y. Hayashi , N. Hayashida , K. Hibino , K. Hiyama , T. Iguchi , K. Ikuta , T. Ishii , R. Ishimori , D. Ivanov , S. Iwamoto , C. C. H. Jui , O. Kalashev , T. Kanbe , K. Kasahara , H. Kawai , S. Kawakami , H. B. Kim , H. K. Kim , J. H. Kim , J. H. Kim , K. Kitamoto , K. Kobayashi , Y. Kobayashi , Y. Kondo , K. Kuramoto , V. Kuzmin , Y. J. Kwon , S. I. Lim , S. Machida , K. Martens , J. Martineau , T. Matsuda , T. Matsuura , T. Matsuyama , I. Myers , M. Minamino , K. Miyata , H. Miyauchi , Y. Murano , T. Nakamura , S. W. Nam , M. Ohnishi , H. Ohoka , K. Oki , D. Oku , A. Oshima , I. H. Park , M. S. Pshirkov , D. Rodriguez , S. Y. Roh , G. Rubtsov , D. Ryu , A. L. Sampson , L. M. Scott , P. D. Shah , F. Shibata , H. Shimodaira , B. K. Shin , J. I. Shin , T. Shirahama , J. D. Smith , P. Sokolsky , T. J. Sonley , R. W. Springer , B. T. Stokes , S. R. Stratton , T. Stroman , S. Suzuki , Y. Takahashi , M. Takita , H. Tanaka , K. Tanaka , M. Tanaka , G. B. Thomson , P. Tinyakov , I. Tkachev , S. Troitsky , K. Tsutsumi , Y. Tsuyuguchi , Y. Uchihori , H. Ukai , G. Vasiloff , Y. Wada , T. Wong , M. Wood , Y. Yamakawa , H. Yamaoka , K. Yamazaki , J. Yang , S. Yoshida , H. Yoshii , R. Zollinger , Z. Zundel

K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of…

Mini-EUSO is a UV telescope that will look downwards to the Earth's atmosphere onboard the International Space Station. With the design of the ultra-high energy cosmic ray fluorescence detectors belonging to the JEM-EUSO program, it will…

K-EUSO (KLYPVE-EUSO) is a planned orbital mission aimed at studying ultra-high energy cosmic rays (UHECRs) by detecting fluorescence and Cherenkov light emitted by extensive air showers in the nocturnal atmosphere of Earth in the…

The JEM-EUSO (Joint Exploratory Missions for Extreme Universe Space Observatory) collaboration is an international initiative studying ultra-high-energy cosmic rays and related phenomena. These particles, with energies exceeding…

天体物理仪器与方法 · 物理学 2025-11-24 Zbigniew Plebaniak

The Telescope Array (TA) observatory, located in midwest Utah, USA, is designed to detect ultra high energy cosmic rays whose energy is greater than 1 EeV. TA mainly consists of two types of detector. The first type is the atmospheric…

天体物理仪器与方法 · 物理学 2014-02-03 Takeshi Okuda
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