Matter traversal of high-energy primary cosmic rays from antiproton measurements

1969 ◽  
Vol 1 (6) ◽  
pp. 336-339
Author(s):  
S. Rosen
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Primary Cosmic Rays

Uncertanties of atmospheric high-energy muon fluxes and spectrum of primary cosmic rays

2007 ◽  
Vol 50 (9) ◽  
pp. 891-897
Author(s):  
A. A. Kochanov ◽  
T. S. Sinegovskaya ◽  
S. I. Sinegovskii
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
High Energy Muon ◽  
Primary Cosmic Rays

Modeling the TREK Detector’s Response When Detecting Muon Bundles from Ultra-High Energy Primary Cosmic Rays

2021 ◽  
Vol 85 (4) ◽  
pp. 438-440
Author(s):  
R. V. Nikolaenko ◽  
A. G. Bogdanov ◽  
V. S. Vorobev ◽  
E. A. Zadeba ◽  
I. Yu. Troshin ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Ultra High Energy ◽  
Muon Bundles ◽  
Primary Cosmic Rays

High energy gamma-families with halo and mass composition of primary cosmic rays in energy region above 10 PeV

2001 ◽  
Vol 97 (1-3) ◽  
pp. 113-115
Author(s):  
A.S. Borisov ◽  
Z.M. Guseva ◽  
S.A. Karpova ◽  
J. Kempa ◽  
A. Krys ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Energy Region ◽  
High Energy ◽  
Mass Composition ◽  
High Energy Gamma ◽  
Energy Gamma ◽  
Primary Cosmic Rays

scholarly journals Observation of the Energy Dependence of Primary and Secondary Cosmic Rays with the AMS Detector on the International Space Station

2019 ◽  
Vol 209 ◽  
pp. 01020
Author(s):  
V. Formato
Keyword(s):  
Cosmic Rays ◽  
Supernova Remnants ◽  
Space Station ◽  
Cosmic Ray ◽  
High Energy ◽  
High Energy Particle ◽  
Detailed Knowledge ◽  
Precision Study ◽  
Peculiar Case ◽  
Primary Cosmic Rays

Precision study of cosmic nuclei provides detailed knowledge on the origin and propagation of cosmic rays. AMS is a multi-purpose high energy particle detector designed to measure and identify cosmic ray nuclei with unprecedented precision. It is able to provide precision studies of nuclei simultaneously to multi-TeV energies. In 7 years on the Space Station, AMS has collected more than 120 billion both primary and secondary cosmic rays. Primary cosmic rays, such as p, He, C and O, are believed to be mainly produced and accelerated in supernova remnants, while secondary cosmic rays, such as Li, Be and B are thought to be produced by collisions of heavier nuclei with interstellar matter. Primary cosmic rays such as He, C, and O are found to have identical rigidity dependence, similarly to secondary cosmic rays (such as Li, Be and B) which share the same the same spectral shape. The peculiar case of Nitrogen being a mixture of a primary and secondary component will also be shown.

scholarly journals MUON CHARGE RATIO OF ULTRAHIGH ENERGY COSMIC RAYS

2008 ◽  
Vol 23 (17n20) ◽  
pp. 1443-1446
Author(s):  
BO-QIANG MA
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Transverse Plane ◽  
Extensive Air Showers ◽  
Charge Ratio ◽  
Ultrahigh Energy ◽  
Air Showers ◽  
Ultrahigh Energy Cosmic Rays ◽  
Primary Cosmic Rays

The muon charge ratio of ultrahigh energy cosmic rays may provide information to detect the composition of the primary cosmic rays. We propose to extract the charge information of high energy muons in very inclined extensive air showers by analyzing their relative lateral positions in the shower transverse plane.

Characteristics of primary cosmic rays and ultra-high-energy interactions from multiple muon data

1975 ◽  
Vol 29 (3) ◽  
pp. 317-334 ◽  
Author(s):  
A. Goned ◽  
T. R. Stewart ◽  
A. W. Wolfendale ◽  
J. Wdowczyk
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Ultra High Energy ◽  
Primary Cosmic Rays

Composition of primary cosmic rays at energies ∼1015eV from data on high-energy muons in extensive air showers

1984 ◽  
Vol 29 (5) ◽  
pp. 892-901 ◽  
Author(s):  
G. B. Yodh ◽  
J. A. Goodman ◽  
S. C. Tonwar ◽  
R. W. Ellsworth
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Extensive Air Showers ◽  
Air Showers ◽  
Primary Cosmic Rays
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