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Astronomical data reduction is usually done with processing pipelines that consist of a series of individual processing steps that can be executed stand-alone. These processing steps are then strung together into workflows and fed with data…

The Pierre Auger Observatory is a hybrid detector designed to observe and study ultra-high-energy particles of extraterrestrial origin. With its 27 fluorescence telescopes and over 1600 autonomously operating water-Cherenkov detectors…

天体物理仪器与方法 · 物理学 2025-07-22 Paul Filip

Ultra High Energy Cosmic Rays (UHECRs) offer a unique chance to study the universe at energies inaccessible by man-made accelerators. Observations by ground based observatories have clarified several characteristics of these particles, but…

高能天体物理现象 · 物理学 2023-10-05 M. Casolino

Future detection of Extensive Air Showers (EAS) produced by Ultra High Energy Cosmic Particles (UHECP) by means of space based fluorescence telescopes will open a new window on the universe and allow cosmic ray and neutrino astronomy at a…

天体物理仪器与方法 · 物理学 2010-04-15 C. Berat , S. Bottai , D. De Marco , S. Moreggia , D. Naumov , M. Pallavicini , R. Pesce , A. Petrolini , A. Stutz , E. Taddei , A. Thea

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…

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

Future experiments based on the observation of Earth's atmosphere from sub-orbital and orbital altitudes plan to include optical Cherenkov cameras to observe extensive air showers produced by high-energy cosmic radiation via its interaction…

天体物理仪器与方法 · 物理学 2021-09-22 Austin Cummings , Roberto Aloisio , Johannes Eser , John Krizmanic

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

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 - 400…

天体物理仪器与方法 · 物理学 2018-09-18 Francesca Capel , Alexander Belov , Marco Casolino , Pavel Klimov

The JEM-EUSO observatory on board of the International Space Station (ISS) is a proposed pioneering space mission devoted to the investigation of Ultra High Energy Cosmic Rays (UHECRs). Looking downward at the earth's atmosphere with a…

天体物理仪器与方法 · 物理学 2019-08-14 S. Toscano , A. Neronov , M. D. Rodríguez Frías , S. Wada

The DSN Transient Observatory (DTO) is a signal processing facility that can monitor up to four DSN downlink bands for astronomically interesting signals. The monitoring is done commensally with reception of deep space mission telemetry.…

天体物理仪器与方法 · 物理学 2017-03-03 T. B. H. Kuiper , R. M. Monroe , L. A. White , C. Garcia Miro , S. M. Levin , W. A. Majid , M. Soriano

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…

Mini--EUSO (Multiwavelength Imaging New Instrument for the Extreme Universe Space Observatory, known as \emph{UV atmosphere} in the Russian Space Program) is the first mission of the JEM-EUSO program on board the International Space…

天体物理仪器与方法 · 物理学 2025-11-18 Mario Bertaina , Matteo Battisti , JEM-EUSO collaboration

The TurLab facility is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located in the fourth basement level of the Physics Department of the University of Turin. In the past years, we have used the facility to…

Macroscopic dark matter (or macro) provides a broad class of alternative candidates to particle dark matter. These candidates would transfer energy primarily through elastic scattering, and this linear energy deposition would produce…

高能物理 - 唯象学 · 物理学 2025-10-07 Thomas C. Paul , Sarah T. Reese , Luis A. Anchordoqui , Angela V. Olinto

This paper presents the concept of a community-accessible stratospheric balloon-based observatory that is currently under preparation by a consortium of European research institutes and industry. The planned European Stratospheric Balloon…

The planned JEM-EUSO (Extreme Universe Space Observatory onboard the ISS Japanese Experimental Module) will measure the energy spectra of cosmic rays up to the range of 1000 EeV and will search for direction to their sources. It will…

天体物理仪器与方法 · 物理学 2019-08-14 Blahoslav Pastirčák , Pavol Bobík , Karel Kudela

EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^{th}$ of August 2014 from Timmins, Canada. The flight ended…

天体物理仪器与方法 · 物理学 2018-08-09 G. Abdellaoui , S. Abe , J. H. Adams , A. Ahriche , D. Allard , L. Allen , G. Alonso , L. Anchordoqui , A. Anzalone , Y. Arai , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , S. Bacholle , M. Bakiri , P. Baragatti , P. Barrillon , S. Bartocci , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. Belov , K. Belov , K. Benmessai , M. Bertaina , P. L. Biermann , S. Biktemerova , F. Bisconti , N. Blanc , J. Błȩcki , S. Blin-Bondil , P. Bobik , M. Bogomilov , E. Bozzo , A. Bruno , K. S. Caballero , F. Cafagna , D. Campana , J-N. Capdevielle , F. Capel , A. Caramete , L. Caramete , P. Carlson , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , C. Catalano O. Catalano , A. Cellino , M. Chikawa , G. Chiritoi , M. J. Christl , V. Connaughton , L. Conti , G. Cordero , G. Cotto , H. J. Crawford , R. Cremonini , S. Csorna , A. Cummings , S. Dagoret-Campagne , C. De Donato , C. de la Taille , C. De Santis , L. del Peral , M. Di Martino , A. Diaz Damian , T. Djemil , I. Dutan , A. Ebersoldt , T. Ebisuzaki , R. Engel , J. Eser , F. Fenu , S. Fernández-González , J. Fernández-Soriano , S. Ferrarese , M. Flamini , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , J. Fujimoto , M. Fukushima , P. Galeotti , E. García-Ortega , G. Garipov , E. Gascón , J. Genci , G. Giraudo , C. González Alvarado , P. Gorodetzky , R. Greg , F. Guarino , A. Guzmán , Y. Hachisu , M. Haiduc , B. Harlov , A. Haungs , J. Hernández Carretero , W. Hidber Cruz , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , E. Joven , E. G. Judd , A. Jung , J. Jochum , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , Y. Karadzhov , J. Karczmarczyk , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , D. Kolev , H. Krantz , I. Kreykenbohm , K. Kudela , Y. Kurihara , A. Kusenko , E. Kuznetsov , A. La Barbera , C. Lachaud , H. Lahmar , F. Lakhdari , R. Larson , O. Larsson , J. Lee , J. Licandro , L. López Campano , M. C. Maccarone , S. Mackovjak , M. Mahdi , D. Maravilla , L. Marcelli , J. L. Marcos , A. Marini , W. Marszał , K. Martens , Y. Martín , O. Martinez , M. Martucci , G. Masciantonio , K. Mase , M. Mastafa , R. Matev , J. N. Matthews , N. Mebarki , G. Medina-Tanco , M. A. Mendoza , A. Menshikov , A. Merino , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , C. Moretto S. Nagataki , S. Naitamor , T. Napolitano , W. Naslund , R. Nava , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , P. Orleański , G. Osteria , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , G. Pasqualino , E. Parizot , I. H. Park , B. Pastircak , T. Patzak , T. Paul , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , L. Placidi , Z. Plebaniak , S. Pliego , A. Pollini , Z. Polonski , E. M. Popescu , P. Prat , G. Prévôt , H. Prieto , G. Puehlhofer , M. Putis , J. Rabanal , A. A. Radu , M. Reyes , M. Rezazadeh , M. Ricci , M. D. Rodríguez Frías , M. Rodencal , F. Ronga , G. Roudil , I. Rusinov , M. Rybczyński , M. D. Sabau , G. Sáez Cano , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. C. Sanchez Balanzar , J. L. Sánchez , A. Santangelo , A. Sanz-Andrés , M. Sanz Palomino , O. Saprykin , F. Sarazin , M. Sato , T. Schanz , H. Schieler , V. Scotti , S. Selmane , D. Semikoz , M. Serra , S. Sharakin , H. M. Shimizu , K. Shinozaki , T. Shirahama , B. Spataro , I. Stan , T. Sugiyama , D. Supanitsky , M. Suzuki , B. Szabelska , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , H. Takami , M. Takeda , Y. Takizawa , M. C. Talai , C. Tenzer , S. B. Thomas , O. Tibolla , L. Tkachev , H. Tokuno , T. Tomida , N. Tone , S. Toscano , M. Traïche , R. Tsenov , Y. Tsunesada , K. Tsuno , J. Tubbs , S. Turriziani , Y. Uchihori , O. Vaduvescu , J. F. Valdés-Galicia , P. Vallania , G. Vankova , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts , M. Weber , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , Z. Włodarczyk , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S Zgura , M. Yu. Zotov , A. Zuccaro Marchi

The origin and nature of Ultra-High Energy Cosmic Rays (UHECRs) remain unsolved in contemporary astroparticle physics. To give an answer to these questions is rather challenging because of the extremely low flux of a few per km$^2$ per…

天体物理仪器与方法 · 物理学 2019-09-10 Mario Bertaina , JEM-EUSO Collaboration

Mini-EUSO will observe the Earth in the UV range (300 - 400 nm) offering the opportunity to study a variety of atmospheric events such as Transient Luminous Events (TLEs), meteors and marine bioluminescence. Furthermore it aims to search…