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The origin of cosmic rays have remained a mistery for more than a century. JEM-EUSO is a pioneer space-based telescope that will be located at the International Space Station (ISS) and its aim is to detect Ultra High Energy Cosmic Rays…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 G. Sáez-Cano , J. A. Morales de los Ríos , L. del Peral , A. Neronov , S. Wada , M. D. Rodríguez Frías

Observing ultra-high energy cosmic rays (UHECR) and very high energy (VHE) neutrinos from space is a promising way to measure their extremely low fluxes by significantly increasing the observed volume. The Extreme Universe Space Observatory…

High Energy Astrophysical Phenomena · Physics 2023-09-01 Johannes Eser , Angela V. Olinto , Lawrence Wiencke

We present a concept for large-area, low-cost detection of ultra-high energy cosmic rays (UHECRs) with a Fluorescence detector Array of Single-pixel Telescopes (FAST), addressing the requirements for the next generation of UHECR…

Mini-EUSO is a telescope launched on board the International Space Station in 2019 and currently located in the Russian section of the station. Main scientific objectives of the mission are the search for nuclearites and Strange Quark…

The detection of Cerenkov light from EAS in a delayed coincidence with fluorescence light gives a strong signature to discriminate protons and neutrinos in cosmic rays. For this purpose, the ULTRA experiment has been designed with 2…

The Extreme Universe Space Observatory on a Super Pressure Balloon II Mission (EUSO-SPB2) is a precursor for a next generation space observatory for multi-messenger astrophysics. The EUSO-SPB2 instrument will measure PeV and EeV-scale…

Instrumentation and Methods for Astrophysics · Physics 2019-10-01 L. Wiencke , A. Olinto

The ultra high energy cosmic neutrinos are powerful astrophysical probes for both astrophysical mechanisms of particle acceleration and fundamental interactions. They open a window into the very distant and high-energy Universe that is…

Instrumentation and Methods for Astrophysics · Physics 2015-11-24 Galina Vankova , Stefan Mladenov , Marian Bogomilov , Roumen Tsenov , Mario Bertaina , Andrea Santangelo

H.E.S.S. -- The High Energy Stereoscopic System-- is a new system of large atmospheric Cherenkov telescopes for GeV/TeV Gamma-ray astronomy. This paper describes the trigger system of H.E.S.S. with emphasis on the multi-telescope array…

Astrophysics · Physics 2009-11-10 S. Funk , G. Hermann , J. Hinton , D. Berge , K. Bernloehr , W. Hofmann , P. Nayman , F. Toussenel , P. Vincent

In this thesis, an introduction to the Ultra-High Energy Cosmic Ray (UHECR) field is given, including air shower physics, UHECR astrophysics, and experimental techniques. The current questions in UHECR physics are mentioned, along with the…

Instrumentation and Methods for Astrophysics · Physics 2014-06-24 Carl Blaksley

We present the data acquisition and control software for the operation of the Mini-Extreme Universe Space Observatory (EUSO), a space-based fluorescence telescope for the observation of extensive air showers and atmospheric phenomena. This…

Instrumentation and Methods for Astrophysics · Physics 2019-12-12 F. Capel , A. Belov , G. Cambiè , M. Casolino , C. Fornaro , P. Klimov , L. Marcelli , L. W. Piotrowski , S. Turriziani

The Japanese Experiment Module (JEM) Extreme Universe Space Observatory (EUSO) will be launched and attached to the Japanese module of the International Space Station (ISS). Its aim is to observe UV photon tracks produced by ultra-high…

The High Energy Cosmic-Radiation Detection (HERD) facility has been proposed as a leading experiment on China's Space Station (CSS). Scheduled for installation around 2027, HERD is expected to operate for at least a decade. The main…

High Energy Astrophysical Phenomena · Physics 2025-04-18 Keerthana Rajan Lathika

TUS (Tracking Ultraviolet Set-up) is the world's first orbital detector of ultra-high-energy cosmic rays (UHECRs). It was launched into orbit on 28th April 2016 as a part of the scientific payload of the Lomonosov satellite. The main aim of…

The second generation of the Extreme Universe Space Observatory on a Super Pressure Balloon (EUSO-SPB2) is a balloon instrument for the detection of ultra high energy cosmic rays (UHECRs) with energies above 1 EeV and very high energy…

Instrumentation and Methods for Astrophysics · Physics 2021-12-22 Rebecca Diesing , Alexa Bukowski , Noah Friedlander , Alex Miller , Stephan Meyer , Angela V. Olinto

JEM-EUSO, on board of the Japanese Exploration Module of the International Space Station, is being proposed as the first space observatory devoted to UHECR. Its privileged position at 430 km above the Earth surface, combined with a large…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Gustavo Medina-Tanco , K. Asano , D. Cline , T. Ebisuzaki , S. Inoue , P. Lipari , E. Parizot , A. Santangelo , G. Sigl , Y. Takahashi , H. Takami , M. Teshima , T. J. Weiler

The TUS detector was the first space-based mission aimed for ultra-high-energy cosmic ray (UHECR) measurements. The detector was designed to register the fluorescent signal of extensive air showers (EAS) developing in the night atmosphere…

High Energy Astrophysical Phenomena · Physics 2021-08-23 Pavel Klimov , Sergei Sharakin , Mikhail Zotov , Mario Bertaina , Francesco Fenu

The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2), successfully launched from Wanaka, New Zealand on May 13, 2022, is a precursor for a space-based astroparticle observatory such as the Probe Of Extreme…

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…

Instrumentation and Methods for Astrophysics · Physics 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 extreme energy cosmic rays (EECRs), which have energies above the 50 EeV, the Greisen-Zatsepin-Kuzmin (GZK) energy limit, is one of the most interesting and complicated problems in modern cosmic-ray physics.…

Mini-EUSO (Multiwavelength Imaging New Instrument for the Extreme Universe Space Observatory) is a telescope observing the Earth in the ultraviolet band (290-430 nm) from the Russian Zvezda module of the International Space Station since…

Instrumentation and Methods for Astrophysics · Physics 2023-10-05 Giulia Romoli