The energy spectrum of primary cosmic ray electrons from 2 GeV to 200 GeV

1971 ◽  
Vol 14 (2) ◽  
pp. 301-313 ◽  
Author(s):  
J. L. Fanselow ◽  
R. C. Hartman ◽  
Peter Meyer ◽  
P. J. Schmidt
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray ◽  
200 Gev

scholarly journals Measurement of the Cosmic Ray Helium Energy Spectrum from 70 GeV to 80 TeV with the DAMPE Space Mission

2021 ◽  
Vol 126 (20) ◽  
Author(s):  
F. Alemanno ◽  
Q. An ◽  
P. Azzarello ◽  
F. C. T. Barbato ◽  
P. Bernardini ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray ◽  
Space Mission

scholarly journals Power laws and the cosmic ray energy spectrum

2007 ◽  
Vol 27 (5) ◽  
pp. 455-464 ◽  
Author(s):  
J.D. Hague ◽  
B.R. Becker ◽  
M.S. Gold ◽  
J.A.J. Matthews
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray ◽  
Power Laws

scholarly journals Anomaly in the cosmic-ray energy spectrum at GeV–TeV energies

2015 ◽  
Vol 632 ◽  
pp. 012026
Author(s):  
Satyendra Thoudam ◽  
Jörg R Hörandel
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray

scholarly journals Cosmic ray composition at the ankle in the energy spectrum

2011 ◽  
Vol 7 (3) ◽  
pp. 275-278 ◽  
Author(s):  
T. Wibig ◽  
A. W. Wolfendale
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray

Energy spectrum of cosmic-ray muons at sea level

1964 ◽  
Vol 32 (6) ◽  
pp. 1524-1540 ◽  
Author(s):  
S. Miyake ◽  
V. S. Narasimham ◽  
P. V. Ramana Murthy
Keyword(s):  
Energy Spectrum ◽  
Sea Level ◽  
Cosmic Ray

scholarly journals On the cosmic ray energy spectrum “knees”

2019 ◽  
Vol 1181 ◽  
pp. 012021
Author(s):  
Yu V Stenkin ◽  
O B Shchegolev
Keyword(s):  
Energy Spectrum ◽  
Cosmic Ray

scholarly journals Atmospheric Muons Measured with IceCube

2019 ◽  
Vol 208 ◽  
pp. 08007 ◽  
Author(s):  
Dennis Soldin
Keyword(s):  
Angular Distribution ◽  
Energy Spectrum ◽  
Cosmic Ray ◽  
Cherenkov Detector ◽  
South Pole ◽  
Lateral Separation ◽  
Hadronic Interactions ◽  
Air Shower ◽  
Shower Development ◽  
Detector Volume

IceCube is a cubic-kilometer Cherenkov detector in the deep ice at the geographic South Pole. The dominant event yield is produced by penetrating atmospheric muons with energies above several 100 GeV. Due to its large detector volume, IceCube provides unique opportunities to study atmospheric muons with large statistics in detail. Measurements of the energy spectrum and the lateral separation distribution of muons offer insights into hadronic interactions during the air shower development and can be used to test hadronic models. We will present an overview of various measurements of atmospheric muons in IceCube, including the energy spectrum of muons between 10 TeV and 1 PeV. This is used to derive an estimate of the prompt contribution of muons, originating from the decay of heavy (mainly charmed) hadrons and unflavored mesons. We will also present measurements of the lateral separation distributions of TeV muons between 150m and 450m for several initial cosmic ray energies between 1 PeV and 16 PeV. Finally, the angular distribution of atmospheric muons in IceCube will be discussed.

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