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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…

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…

Neural networks as well as other methods of machine learning (ML) are known to be highly efficient in different classification tasks, including classification of images and videos. Mini- EUSO is a wide-field-of-view imaging telescope that…

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…

High Energy Astrophysical Phenomena · Physics 2023-10-05 M. Casolino

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…

Instrumentation and Methods for Astrophysics · Physics 2019-09-10 Mario Bertaina , JEM-EUSO Collaboration

Two types of orbital detectors of extreme energy cosmic rays are being developed nowadays: (i) TUS and KLYPVE with reflecting optical systems (mirrors) and (ii) JEM-EUSO with high-transmittance Fresnel lenses. They will cover much larger…

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 TurLab facility is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located in the Physics Department of the University of Turin. Originally, it was mainly built to study systems of different scales where rotation…

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 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

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 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…

Instrumentation and Methods for Astrophysics · Physics 2023-09-22 Francesca Bisconti

TUS (Tracking Ultraviolet Set-up), the first orbital detector of extreme energy cosmic rays (EECRs), those with energies above 50 EeV, was launched into orbit on April 28, 2016, as a part of the Lomonosov satellite scientific payload. 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…

Instrumentation and Methods for Astrophysics · Physics 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 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.…

The second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) mission is a stratospheric balloon mission developed within the Joint Exploratory Missions for Extreme Universe Space Observatory (JEM-EUSO)…

The latest and most advanced effort towards a space-based optical cosmic ray detector developed within the Joint Experiment Mission for the Extreme Universe Space Observatory (JEM-EUSO) collaboration was the Extreme Universe Space…

Instrumentation and Methods for Astrophysics · Physics 2019-09-27 J. Eser , A. Olinto , L. Wiencke

TUS (Track Ultraviolet Setup) is the first space experiment aimed to check the possibility of registering extreme energy cosmic rays (EECRs) at E>50 EeV by measuring the fluorescence signal of extensive air showers in the atmosphere. The…

The JEM-EUSO Collaboration aims at studying Ultra High Energy Cosmic Rays (UHECR) from space. To reach this goal, a series of pathfinder missions has been developed to prove the observation principle and to raise the technological readiness…

Instrumentation and Methods for Astrophysics · Physics 2020-10-30 Valentina Scotti , Giuseppe Osteria , Francesco Perfetto