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The IceCube Observatory at the South Pole is composed of a cubic kilometer scale neutrino telescope buried beneath the icecap and a square-kilometer surface water Cherenkov tank detector array known as IceTop. The combination of the surface…

High Energy Astrophysical Phenomena · Physics 2012-12-07 Alessio Tamburro

Cosmic rays are charged energetic particles that permeate the interstellar medium. Their sizeable energy share and penetration power makes them essential players in the dynamical and chemical processes that rule Galactic evolution, such as…

High Energy Astrophysical Phenomena · Physics 2026-03-17 Giada Peron , Sarah Recchia , Stefano Menchiari , Alexandre Marcowith , Andrei Bykov , Martin Pohl , Elena Amato

We report progress on applying technologies developed for LHC-era experiments to cosmic ray detection, using scintillating tiles with embedded wavelength-shifting fibers and avalanche photodiode readouts as parts of a robust, inexpensive…

Cosmic ray muon has strong penetrating power and no ionizing radiation hazards, which makes it an ideal probe for detecting special nuclear materials. In this paper, a high spatial resolution muon tomography system based on Micromegas…

Instrumentation and Detectors · Physics 2022-02-16 Yu Wang , Zhiyong Zhang , Shubin Liu , Zhongtao Shen , Changqing Feng , Jianguo Liu , Yulin Liu

In this talk I discuss the use of calorimeter timing both for detector commissioning and in searches for new physics. In particular I present real and simulated cosmic ray muons data results for the ATLAS Tile Calorimeter system. The…

Instrumentation and Detectors · Physics 2010-01-15 Bernhard Meirose

Cosmic rays are energetic charged particles from extraterrestrial sources, with the highest energy events thought to come from extragalactic sources. Their arrival is infrequent, so detection requires instruments with large collecting…

High Energy Astrophysical Phenomena · Physics 2023-11-27 Telescope Array Collaboration

The plasma panel sensor is an ionizing photon and particle radiation detector derived from PDP technology with high gain and nanosecond response. Experimental results in detecting cosmic ray muons and beta particles from radioactive sources…

The CosmicWatch Desktop Muon Detector (v3X) is a compact, low-cost, and portable device designed for detecting ionizing radiation, including cosmic-ray muons. Building on previous iterations, the v3X introduces significant hardware and…

Instrumentation and Detectors · Physics 2025-10-24 Spencer Axani , Masooma Sarfraz , Miles Garcia , Collin Owens , Katarzyna Frankiewicz , Janet M. Conrad

Extensive air showers still are our only access to the highest-energy particles in the universe, namely cosmic-ray nuclei with energies up to several 100 EeV. Studying open questions in cosmic-ray physics, like their yet unknown origin…

High Energy Astrophysical Phenomena · Physics 2017-04-21 Frank G. Schröder

IceCube is a cubic-kilometer Cherenkov detector in the deep ice at the geographic South Pole. The dominant event yield in the deep ice detector consists of penetrating atmospheric muons with energies above approximately 300 GeV, produced in…

High Energy Astrophysical Phenomena · Physics 2022-08-04 Dennis Soldin

Muon component of extensive air showers (EAS) initiated by cosmic ray particles carries information on the primary particle identity. We show that the muon content of EAS could be measured in a broad energy range from 10-100 TeV up to…

Instrumentation and Methods for Astrophysics · Physics 2017-01-05 A. Neronov , D. V. Semikoz , Ie. Vovk , R. Mirzoyan

The Muon Ionization Cooling Experiment (MICE) is a strategic R&D project intended to demonstrate the only practical solution to providing high brilliance beams necessary for a neutrino factory or muon collider. MICE is under development at…

Accelerator Physics · Physics 2013-08-01 U. Bravar , M. Bogomilov , Y. Karadzhov , D. Kolev , I. Russinov , R. Tsenov , L. Wang , F. Y. Xu , S. X. Zheng , R. Bertoni , M. Bonesini , R. Mazza , V. Palladino , G. Cecchet , A. de Bari , M. Capponi , A. Iaciofano , D. Orestano , F. Pastore , L. Tortora , S. Ishimoto , S. Suzuki , K. Yoshimura , Y. Mori , Y. Kuno , H. Sakamoto , A. Sato , T. Yano , M. Yoshida , F. Filthaut , M. Vretenar , S. Ramberger , A. Blondel , F. Cadoux , F. Masciocchi , J. S. Graulich , V. Verguilov , H. Wisting , C. Petitjean , R. Seviour , M. Ellis , P. Kyberd , M. Littlefield , J. J. Nebrensky , D. Forrest , F. J. P. Soler , K. Walaron , P. Cooke , R. Gamet , A. Alecou , M. Apollonio , G. Barber , A. Dobbs , P. Dornan , A. Fish , R. Hare , A. Jamdagni , V. Kasey , M. Khaleeq , K. Long , J. Pasternak , H. Sakamoto , T. Sashalmi , V. Blackmore , J. Cobb , W. Lau , M. Rayner , C. D. Tunnell , H. Witte , S. Yang , J. Alexander , G. Charnley , S. Griffiths , B. Martlew , A. Moss , I. Mullacrane , A. Oats , S. York , R. Apsimon , R. J. Alexander , P. Barclay , D. E. Baynham , T. W. Bradshaw , M. Courthold , R. Edgecock T. Hayler , M. Hills , T. Jones , N. McCubbin , W. J. Murray , C. Nelson , A. Nicholls , P. R. Norton , C. Prior , J. H. Rochford , C. Rogers , W. Spensley , K. Tilley , C. N. Booth , P. Hodgson , R. Nicholson , E. Overton , M. Robinson , P. Smith , D. Adey , J. Back , S. Boyd , P. Harrison , J. Norem , A. D. Bross , S. Geer , A. Moretti , D. Neuffer , M. Popovic , Z. Qian , R. Raja , R. Stefanski , M. A. C. Cummings , T. J. Roberts , A. DeMello , M. A. Green , D. Li , A. M. Sessler , S. Virostek , M. S. Zisman , B. Freemire , P. Hanlet , D. Huang , G. Kafka , D. M. Kaplan , P. Snopok , Y. Torun , Y. Onel , D. Cline , K. Lee , Y. Fukui , X. Yang , R. A. Rimmer , L. M. Cremaldi , T. L. Hart , D. J. Summers , L. Coney , R. Fletcher , G. G. Hanson , C. Heidt , J. Gallardo , S. Kahn , H. Kirk , R. B. Palmer

Cosmic ray studies, in particular UHECR, can be in general supported by a directional, easy deployable, simple and robust detector. The design of this detector is based on the time of flight between two parallel tiles of scintillator, to…

Astrophysics · Physics 2008-11-26 M. Iori , A. Sergi

The gaseous proportional counter is a device that can be used to detect ionizing radiation. These devices can be as simple as a cylindrical cathode and a very thin anode wire centered along its axis. By applying a high voltage, a strong…

We investigate the possibility of detecting light long-lived particle (LLP) produced by high energy cosmic ray colliding with atmosphere. The LLP may penetrate the atmosphere and decay into a pair of muons near/in the neutrino telescope.…

High Energy Physics - Phenomenology · Physics 2015-05-14 Peng-fei Yin , Shou-hua Zhu

The D0 preshower detector consists of scintillator strips with embedded wavelength-shifting fibers, and a readout using Visible Light Photon Counters. The response to minimum ionizing particles has been tested with cosmic ray muons. We…

High Energy Physics - Experiment · Physics 2008-11-26 P. Baringer

A semiconductor tracker for muon scattering tomography is presented. The tracker contains silicon strip sensors with an $80\,\mu$m pitch, precision mechanics and integrated cooling. The electronic readout of the sensors is performed by a…

Instrumentation and Detectors · Physics 2018-10-30 F. Keizer , A. Gorbatch , M. A. Parker , C. Steer , S. A. Wotton

Muography is an innovative imaging technique using naturally produced elementary particles -- atmospheric muons -- like the X-rays of medical imaging. The modification of the particles flux -- by scattering or absorption --, reflects the…

Instrumentation and Detectors · Physics 2024-01-31 Theodore Avgitas , Jean Christophe Ianigro , Jacques Marteau

Primary cosmic rays when interact with our atmosphere, produce a cascade of lighter secondary particles namely pion, kaon, neutrons, muons, electrons, positrons and neutrinos. Muons are one of the most abundant and easily detectable…

Magnetic fields play a critical role in the propagation of charged cosmic rays. Particular field configurations supported by different astrophysical objects may be observable in cosmic ray maps. We consider a simple configuration, a…

High Energy Astrophysical Phenomena · Physics 2015-05-19 E. Battaner , J. Castellano , M. Masip