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So far, cosmic ray air showers have been detected using scintillation counter arrays on the ground widely. And also air Cherenkov detection method, which is limited its observation period in moonless nights, has been adopted. The detection…

Instrumentation and Methods for Astrophysics · Physics 2019-07-23 Yoshitaka Kawashima

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

We present the development and performance of a newly built recoil ion momentum spectrometer to study the fragmentation dynamics of ionized molecules. The spectrometer is based on the two-stage Wiley-McLaren geometry and satisfies both time…

Atomic Physics · Physics 2022-11-23 Avijit Duley , Rohit Tyagi , Sandeep B. Bari , A. H. Kelkar

Proportional scintillation counters (PSCs), both single- and dual-phase, can measure the scintillation (S1) and ionization (S2) channels from particle interactions within the detector volume. The signal obtained from these detectors depends…

Instrumentation and Detectors · Physics 2016-03-23 Kareem Kazkaz , Tenzing Henry Yatish Joshi

We present results demonstrating the time resolution and $\mu$/e separation capabilities with a new concept of an EAS detector capable for measurements of cosmic rays arriving with large zenith angles. This kind of detector has been…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 M. Iori , H. Denizli , A. Yilmaz , F. Ferrarotto , J. Russ

This article presents a few selected developments and future ideas related to the measurement of $(n,\gamma)$ data of astrophysical interest at CERN n_TOF. The MC-aided analysis methodology for the use of low-efficiency radiation detectors…

Nuclear Experiment · Physics 2023-02-07 C. Domingo-Pardo , V. Babiano-Suarez , J. Balibrea-Correa , L. Caballero , I. Ladarescu , J. Lerendegui-Marco , J. L. Tain , A. Tarifeño-Saldivia , O. Aberle , V. Alcayne , S. Altieri , S. Amaducci , J. Andrzejewski , M. Bacak , C. Beltrami , S. Bennett , A. P. Bernardes , E. Berthoumieux , M. Boromiza , D. Bosnar , M. Caamaño , F. Calviño , M. Calviani , D. Cano-Ott , A. Casanovas , F. Cerutti , G. Cescutti , S. Chasapoglou , E. Chiaveri , N. M. Chiera , P. Colombetti , N. Colonna , P. Console Camprini , G. Cortés , M. A. Cortés-Giraldo , L. Cosentino , S. Cristallo , S. Dellmann , M. Di Castro , S. Di Maria , M. Diakaki , M. Dietz , R. Dressler , E. Dupont , I. Durán , Z. Eleme , S. Fargier , B. Fernández , B. Fernández-Domínguez , P. Finocchiaro , S. Fiore , V. Furman , F. García-Infantes , A. Gawlik-Ramiega , G. Gervino , S. Gilardoni , E. González-Romero , C. Guerrero , F. Gunsing , C. Gustavino0 , J. Heyse , W. Hillman , D. G. Jenkins , E. Jericha , A. Junghans , Y. Kadi , K. Kaperoni , F. Käppeler , G. Kaur , A. Kimura , I. Knapová , U. Koester , M. Kokkoris , Y. Kopatch , M. Krtička , N. Kyritsis , C. Lederer-Woods , G. Lerner , A. Manna , T. Martínez , A. Masi , C. Massimi , P. Mastinu , M. Mastromarco , E. A. Maugeri , A. Mazzone , E. Mendoza , A. Mengoni , P. M. Milazzo , I. Mönch , R. Mucciola , F. Murtas , E. Musacchio-Gonzalez , A. Musumarra , A. Negret , A. Pérez de Rada , P. Pérez-Maroto , N. Patronis , J. A. Pavón-Rodríguez , M. G. Pellegriti , J. Perkowski , C. Petrone , E. Pirovano , J. Plaza , S. Pomp , I. Porras , J. Praena , J. M. Quesada , R. Reifarth , D. Rochman , Y. Romanets , C. Rubbia , A. Sánchez , M. Sabaté-Gilarte , P. Schillebeeckx , D. Schumann , A. Sekhar , A. G. Smith , N. V. Sosnin , M. Stamati , A. Sturniolo , G. Tagliente , D. Tarrío , P. Torres-Sánchez , J. Turko , S. Urlass , E. Vagena , S. Valenta , V. Variale , P. Vaz , G. Vecchio , D. Vescovi , V. Vlachoudis , R. Vlastou , T. Wallner , P. J. Woods , T. Wright , R. Zarrella , P. Žugec

The detectors in mass spectrometers are precise enough to count ion events. In practice, the statistics of chemical noise are affected by large quantization errors and overdispersion because of amplification in the detector. The detector…

Discrete Mathematics · Computer Science 2009-06-02 Sébastien Li-Thiao-Té

The Pierre Auger Cosmic-Ray Observatory uses the earth's atmosphere as a calorimeter to measure extensive air-showers created by particles of astrophysical origin. Some of these particles carry joules of energy. At these extreme energies,…

Astrophysics · Physics 2019-08-13 L. Wiencke

Very high energy gamma-ray astronomy based on the measurement of air shower particles at ground-level has only recently been established as a viable approach, complementing the well established air Cherenkov technique. This approach…

High Energy Astrophysical Phenomena · Physics 2019-06-26 Harm Schoorlemmer , Jim Hinton , Rubén López-Coto

This article describes the design, assembly and characterization of a portable cosmic ray detector, developed by the INSULAB group and suitable for teaching activities aimed at high school students. It consists of a compact aluminum…

This article describes a radon emanation measurement technique using liquid scintillator counting. A model for radon loading and transport is described, along with its calibration. Detector background and blank have been studied and…

Instrumentation and Detectors · Physics 2025-01-30 A. B. M. R. Sazzad , P. Acharya , P. Back , J. Busenitz , D. Chernyak , Y. Meng , A. Piepke , C. A. Rhyne , R. Tsang

For a long time, the cloud chamber was the only educational tool available for measuring radiation. In recent years, simple radiation detectors combining scintillators with silicon photomultipliers have become increasingly common for these…

Physics Education · Physics 2026-05-12 Yuzuka Sasaki , Yuuki Wada , Kazuo S. Tanaka

Aerial source detection systems have the capability to rapidly provide radiological data over a large area of land. Sodium Iodine (NaI) scintillator based aerial radiation detection systems of compact physical sizes have the potential aid…

Instrumentation and Detectors · Physics 2021-11-16 Sebastian Ritter

Changes in the sky noise spectrum are used to characterize perturbations in the ionosphere. Observations were made at the same sidereal time on multiple days using a calibrated broadband dipole and radio spectrometer covering 80 to 185 MHz.…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 Alan E. E. Rogers , Judd D. Bowman , Juha Vierinen , Raul Monsalve , Thomas Mozdzen

We present a study of scintillation induced by the mid-latitude ionosphere. By implementing methods currently used in Interplanetary Scintillation studies to measure amplitude scintillation at low frequencies, we have proven it is possible…

Instrumentation and Methods for Astrophysics · Physics 2022-09-14 A. Waszewski , J. Morgan , C. H. Jordan

START, a high-efficiency and low-noise scintillation detector for ionizing particles, was developed for the purpose of creating a high-granular system for triggering cosmic muons. Scintillation light in START is detected by MRS APDs…

Coherent scattering is a flavor-blind, high-rate, as yet undetected neutrino interaction predicted by the Standard Model. We propose to use a compact (kg-scale), two-phase (liquid-gas) argon ionization detector to measure coherent neutrino…

Nuclear Experiment · Physics 2009-11-10 Chris Hagmann , Adam Bernstein

Ground-based gamma-ray astronomy is a powerful tool to study cosmic-ray physics, providing a diagnostic of the high-energy processes at work in the most extreme astrophysical accelerators of the universe. Ground-based gamma-ray detectors…

Instrumentation and Methods for Astrophysics · Physics 2023-07-07 Ulisses Barres de Almeida , Martin Tluczykont

In the context of particle therapy monitoring, we are developing a gamma-ray detector to determine the ion range in vivo from the measurement of particle time-of-flight. For this application, a beam monitor capable to tag in time the…

Ultra-high energy cosmic rays impinging onto the atmosphere induce huge cascades of secondary particles. The measurement of the energy radiated by these air showers in form of radio waves enables an accurate measurement of the cosmic-ray…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Christian Glaser
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