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The Effects of High-Energy Carbon Co-Doping on IMB-CNM LGAD Fabrication and Performance. [PDF]
Sensors (Basel)Villegas J +5 more
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Atmospheric Cosmic Ray Detectors
2011This document is part of Part 2 'Principles and Methods' of Subvolume B 'Detectors for Particles and Radiation' of Volume 21 'Elementary Particles' of Landolt-Bornstein - Group I 'Elementary Particles, Nuclei and Atoms'. It contains the Section '6.1 Atmospheric Cosmic Ray Detectors' of Chapter '6 Detectors for Special Applications' with the content:
J. Blümer, J. Engler
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Applications of cosmic-ray muons
Progress in Particle and Nuclear Physics, 2020Applications of cosmic-ray muons have grown in numbers in the last decades. This was possible thanks to the development of detectors and techniques employed in particle and nuclear physics.
G. Bonomi +4 more
semanticscholar +3 more sources
2010
This document is part of Subvolume A 'Instruments and Methods' of Volume 4 'Astronomy, Astrophysics, and Cosmology' of Landolt-Bornstein - Group VI 'Astronomy and Astrophysics'.
D. Müller
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This document is part of Subvolume A 'Instruments and Methods' of Volume 4 'Astronomy, Astrophysics, and Cosmology' of Landolt-Bornstein - Group VI 'Astronomy and Astrophysics'.
D. Müller
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SVIRCO contribution to the world-wide network of cosmic ray detectors
Advances in Space Research, 2009M. Storini, F. Signoretti
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Astronomical & Astrophysical Transactions, 2003
In this paper a compact large solid-angle photodetection system is proposed. This system was designed to measure spectrum of the gamma-ray bursts in the range from 20 MeV to 10 GeV with a resolution from 2 to 150 MeV.
E. S. Konobeevski +2 more
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In this paper a compact large solid-angle photodetection system is proposed. This system was designed to measure spectrum of the gamma-ray bursts in the range from 20 MeV to 10 GeV with a resolution from 2 to 150 MeV.
E. S. Konobeevski +2 more
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European Physical Journal A, 2019
.The relevant interaction energies for astrophysical radiative capture reactions are very low, much below the repulsive Coulomb barrier. This leads to low cross sections, low counting rates in γ-ray detectors, and therefore the need to perform such ...
T. Szücs +9 more
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.The relevant interaction energies for astrophysical radiative capture reactions are very low, much below the repulsive Coulomb barrier. This leads to low cross sections, low counting rates in γ-ray detectors, and therefore the need to perform such ...
T. Szücs +9 more
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Introduction to Ultrahigh Energy Cosmic Ray Physics
, 2020Cosmic ray physics has recently attracted a great deal of attention from the high energy physics community because of the discovery of new sources and the advent of new techniques.
P. Sokolsky
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