Radio detection of cosmic-ray air showers and high-energy neutrinos
FG Schröder - Progress in Particle and Nuclear Physics, 2017 - Elsevier
In the last fifteen years radio detection made it back to the list of promising techniques for
extensive air showers, firstly, due to the installation and successful operation of digital radio …
extensive air showers, firstly, due to the installation and successful operation of digital radio …
Radio detection of cosmic ray air showers in the digital era
T Huege - Physics Reports, 2016 - Elsevier
In 1965 it was discovered that cosmic ray air showers emit impulsive radio signals at
frequencies below 100 MHz. After a period of intense research in the 1960s and 1970s …
frequencies below 100 MHz. After a period of intense research in the 1960s and 1970s …
Design and sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
This article presents the design of the Radio Neutrino Observatory Greenland (RNO-G) and
discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure …
discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure …
The Pierre Auger cosmic ray observatory
Pierre Auger Collaboration - … and Methods in Physics Research Section …, 2015 - Elsevier
Abstract The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is
the world׳ s largest cosmic ray observatory. The objectives of the Observatory are to probe …
the world׳ s largest cosmic ray observatory. The objectives of the Observatory are to probe …
The pierre auger observatory upgrade-preliminary design report
A Aab, P Abreu, M Aglietta, EJ Ahn, IA Samarai… - arXiv preprint arXiv …, 2016 - arxiv.org
The Pierre Auger Observatory has begun a major Upgrade of its already impressive
capabilities, with an emphasis on improved mass composition determination using the …
capabilities, with an emphasis on improved mass composition determination using the …
A large light-mass component of cosmic rays at 1017–1017.5 electronvolts from radio observations
Cosmic rays are the highest-energy particles found in nature. Measurements of the mass
composition of cosmic rays with energies of 1017–1018 electronvolts are essential to …
composition of cosmic rays with energies of 1017–1018 electronvolts are essential to …
Method for high precision reconstruction of air shower using two-dimensional radio intensity profiles
S Buitink, A Corstanje, JE Enriquez, H Falcke… - Physical Review D, 2014 - APS
The mass composition of cosmic rays contains important clues about their origin. Accurate
measurements are needed to resolve longstanding issues such as the transition from …
measurements are needed to resolve longstanding issues such as the transition from …
NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector
C Glaser, D García-Fernández, A Nelles… - The European Physical …, 2020 - Springer
Abstract NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy
neutrino detectors that rely on the radio detection method. This method exploits the radio …
neutrino detectors that rely on the radio detection method. This method exploits the radio …
[图书][B] Introduction to ultrahigh energy cosmic ray physics
P Sokolsky, G Thomson - 2020 - taylorfrancis.com
This revised edition provides an up-to-date summary of the field of ultra-high energy cosmic
rays, dealing with their origin, propagation, and composition,. The authors reflect the …
rays, dealing with their origin, propagation, and composition,. The authors reflect the …
Constraints on the diffuse flux of ultrahigh energy neutrinos from four years of Askaryan Radio Array data in two stations
P Allison, S Archambault, JJ Beatty, M Beheler-Amass… - Physical Review D, 2020 - APS
The Askaryan Radio Array (ARA) is an ultrahigh energy (UHE,> 10 17 eV) neutrino detector
designed to observe neutrinos by searching for the radio waves emitted by the relativistic …
designed to observe neutrinos by searching for the radio waves emitted by the relativistic …