NEVOD — An experimental complex for multi-component investigations of cosmic rays and their interactions in the energy range 1–1010 GeV

2021 ◽  
Vol 16 (08) ◽  
pp. T08014
Author(s):  
I.I. Yashin ◽  
M.B. Amelchakov ◽  
I.I. Astapov ◽  
N.S. Barbashina ◽  
A.G. Bogdanov ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Experimental Complex

scholarly journals THE FERMI BUBBLE AS A SOURCE OF COSMIC RAYS IN THE ENERGY RANGE >1015eV

2012 ◽  
Vol 746 (2) ◽  
pp. 116 ◽  
Author(s):  
K.-S. Cheng ◽  
D. O. Chernyshov ◽  
V. A. Dogiel ◽  
C.-M. Ko ◽  
W.-H. Ip ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Range

scholarly journals Radio detection of cosmic rays with the Auger Engineering Radio Array

2019 ◽  
Vol 210 ◽  
pp. 05011 ◽  
Author(s):  
Tim Huege ◽  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Cosmic Ray ◽  
Energy Scale ◽  
Pierre Auger Observatory ◽  
Mass Composition ◽  
Frequency Range ◽  
Radio Detection ◽  
Composition Measurements

The Auger Engineering Radio Array (AERA) complements the Pierre Auger Observatory with 150 radio-antenna stations measuring in the frequency range from 30 to 80 MHz. With an instrumented area of 17 km2, the array constitutes the largest cosmic-ray radio detector built to date, allowing us to do multi-hybrid measurements of cosmic rays in the energy range of 1017 eV up to several 1018 eV. We give an overview of AERA results and discuss the significance of radio detection for the validation of the energy scale of cosmicray detectors as well as for mass-composition measurements.

RECENT RESULTS FROM SUPER-KAMIOKANDE

2002 ◽  
Vol 17 (24) ◽  
pp. 3353-3363 ◽  
Author(s):  
◽  
J. A. GOODMAN
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Solar Neutrinos ◽  
Recent Analysis ◽  
The Sun

Super-Kamiokande is a 50 Kiloton water-Cherenkov that detects neutrinos in the MeV energy range that are produced in the Sun and neutrinos in the GeV energy range produced in the atmosphere by cosmic rays. The detector has been operational since April of 1996. In this paper results of our most recent analysis will be presented on both atmospheric and solar neutrinos.

ASTROPARTICLE PHYSICS FROM 1016 TO 1020 eV

2007 ◽  
Vol 16 (09) ◽  
pp. 2775-2788
Author(s):  
VITOR DE SOUZA
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Particle Interactions ◽  
Astroparticle Physics ◽  
Near Future

Cosmic rays have always been an important tool to study particle interactions and astrophysics. In this article, we are going to review the main results from this field in the energy range from 1016 to 1020 eV. Important results from the KASCADE and Pierre Auger Experiments are going to be shown and discussed. Some perspectives for the near future concerning new measurements are going to be presented.

scholarly journals Underground investigation of extensive air showers spectra at high energy range of cosmic rays and other research in the Pyhäsalmi mine

2020 ◽  
Vol 72 (1) ◽  
pp. 19-26
Author(s):  
N. Yerezhep ◽  
W.H. Trzaska ◽  
L. Bezrukov ◽  
T. Enqvist ◽  
P. Kuusiniemi ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
High Energy ◽  
Extensive Air Showers ◽  
Air Showers

scholarly journals The HiSCORE Project

2014 ◽  
Vol 1 (1) ◽  
pp. 283-287 ◽  
Author(s):  
M. Tluczykont ◽  
M. Brückner ◽  
N. Budnev ◽  
O. Chvalaev ◽  
A. Dyachok ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Cosmic Ray ◽  
Central Question ◽  
Large Area ◽  
Particle Detectors ◽  
Air Shower ◽  
The Status ◽  
Hybrid Detector ◽  
Cosmic Origin

A central question of Astroparticle Physics, the origin of cosmic rays, still remains unsolved. HiSCORE (Hundred*i Square-km Cosmic ORigin Explorer) is a concept for a large-area wide-angle non-imaging air shower detector, addressing this question by searching for cosmic ray pevatrons in the energy range from 10TeV to few PeV and cosmic rays in the energy range above 100TeV. In the framework of the Tunka-HiSCORE project, first prototypes have been deployed on the site of the Tunka-133 experiment, where we plan to install an engineering array covering an area of the order of 1km<sup>2</sup>. On the same site, also imaging and particle detectors are planned, potentially allowing a future hybrid detector system. Here we present the HiSCORE detector principle, its potential for cosmic ray origin search and the status of ongoing activities in the framework of the Tunka-HiSCORE experiment.

scholarly journals Investigation of the energy spectrum and chemical composition of primary cosmic rays in 1–100 PeV energy range with a UAV-borne detector

2020 ◽  
Vol 15 (09) ◽  
pp. C09061-C09061
Author(s):  
D. Chernov ◽  
E. Bonvech ◽  
M. Finger Jr. ◽  
M. Finger ◽  
V. Galkin ◽  
...  
Keyword(s):  
Chemical Composition ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Primary Cosmic Rays

scholarly journals Cosmic Ray Energy Spectrum derived from the Data of EAS Cherenkov Light Arrays in the Tunka Valley

2019 ◽  
Vol 210 ◽  
pp. 01003
Author(s):  
V. Prosin ◽  
I. Astapov ◽  
P. Bezyazeekov ◽  
A. Borodin ◽  
M. Brückner ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Cosmic Ray ◽  
Cherenkov Light ◽  
Differential Energy Spectrum ◽  
Extensive Air Shower ◽  
Air Shower

The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from 2009 to 2017. From 2175 hours of data taking, we derived the differential energy spectrum of cosmic rays in the energy range 6 · 1015 2 · 1018 eV. The TAIGA-HiSCORE array is in the process of continuous expansion and modernization. Here we present the results obtained with 28 stations of the first HiSCORE stage from 35 clear moonless nights in the winter of 2017-2018. The combined spectrum of two arrays covers a range of 2 · 1014 – 2 · 1018 eV.

scholarly journals Summary of the main results of the KASCADE and KASCADE-Grande experiments

2019 ◽  
Vol 208 ◽  
pp. 03002 ◽  
Author(s):  
A. Chiavassa ◽  
W.D. Apel ◽  
J.C. Arteaga-Velázquez ◽  
K. Bekk ◽  
M. Bertaina ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Range ◽  
Elemental Composition ◽  
Large Scale ◽  
Hadronic Interaction ◽  
Primary Spectrum ◽  
Interaction Models ◽  
Primary Cosmic Rays

The KASCADE and KASCADE-Grande experiments operated in KIT-Campus North, Karlsruhe (Germany) from 1993 to 2012. The two experiments studied primary cosmic rays in the energy range from 1014 eV to 1018 eV, investigating the change of slope of the spectrum detected at 2 - 4 × 1015 eV, the so called knee. We briefly review the performance of the experiments and then the main results obtained in the operation of both experiments: the test of hadronic interaction models, the all particle primary spectrum, the elemental composition of primary cosmic rays (with the first claim of a knee-like feature of the heavy primaries spectrum) and the search for large scale anisotropies.

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