The study of primary cosmic rays energy spectrum and mass composition in the energy range 0.5 – 50 PeV with TUNKA Eas Cherenkov array

1999 ◽  
Vol 75 (1-2) ◽  
pp. 299-301 ◽  
Author(s):  
O.A. Gress ◽  
T.I. Gress ◽  
E.E. Korosteleva ◽  
L.A. Kuzmichev ◽  
B.K. Lubsandorzhiev ◽  
...  
2020 ◽  
Vol 15 (09) ◽  
pp. C09061-C09061
Author(s):  
D. Chernov ◽  
E. Bonvech ◽  
M. Finger Jr. ◽  
M. Finger ◽  
V. Galkin ◽  
...  

1968 ◽  
Vol 46 (10) ◽  
pp. S530-S532 ◽  
Author(s):  
A. Danjo ◽  
S. Hayakawa ◽  
F. Makino ◽  
Y. Tanaka

The energy spectrum of electrons in the primary cosmic rays was measured at a location where the vertical geomagnetic cutoff rigidity is 11.5 GV, using a balloon-borne counter system. The differential spectrum was determined in the energy range from 13 to 50 GeV and is represented by a power law with exponent −2.4 ± 0.6. This result is consistent with a spectrum extending smoothly from lower energies with the same slope.


2009 ◽  
Vol 64 (5) ◽  
pp. 536-540 ◽  
Author(s):  
N. N. Kalmykov ◽  
G. V. Kulikov ◽  
V. P. Sulakov ◽  
Yu. A. Fomin

2003 ◽  
Vol 66 (7) ◽  
pp. 1145-1206 ◽  
Author(s):  
Andreas Haungs ◽  
Heinigerd Rebel ◽  
Markus Roth

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