Stochastic space-time and the primary energy spectrum of cosmic rays atE 0≥1019 eV

1985 ◽  
Vol 8 (5) ◽  
pp. 531-537 ◽  
Author(s):  
M. Sinha ◽  
S. Roy
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Primary Energy ◽  
Space Time ◽  
Stochastic Space

Primary energy spectrum of cosmic rays obtained by arrival time spread of particles in EAS

2008 ◽  
Vol 175-176 ◽  
pp. 322-325 ◽  
Author(s):  
M. Okita ◽  
T. Wada ◽  
Y. Yamashita ◽  
K. Okei ◽  
T. Morita ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Arrival Time ◽  
Primary Energy ◽  
Time Spread

Energy spectrum of superhigh-energy cosmic rays

1982 ◽  
Vol 136 (2) ◽  
pp. 351 ◽  
Author(s):  
G.B. Khristiansen
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Superhigh Energy

scholarly journals The measurement of the energy of cosmic rays - II—The curvature measurements and the energy spectrum

1936 ◽  
Vol 154 (883) ◽  
pp. 573-587 ◽  
Keyword(s):  
Magnetic Field ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
The Earth ◽  
Primary Particles ◽  
Curvature Measurements

Both the penetrating power of the cosmic rays through material ab­sorbers and their ability to reach the earth in spite of its magnetic field, make it certain that the energy of many of the primary particles must reach at least 10 11 e-volts. However, the energy measurements by Kunze, and by Anderson, using cloud chambers in strong magnetic fields, have extended only to about 5 x 10 9 e-volts. Particles of greater energy were reported, but the curvature of their tracks was too small to be measured with certainty. We have extended these energy measurements to somewhat higher energies, using a large electro-magnet specially built for the purpose and described in Part I. As used in these experiments, the magnet allowed the photography of tracks 17 cm long in a field of about 14,000 gauss. The magnet weighed about 11,000 kilos and used a power of 25 kilowatts.

Energy spectrum and mass composition of high-energy cosmic rays

2003 ◽  
Vol 66 (7) ◽  
pp. 1145-1206 ◽  
Author(s):  
Andreas Haungs ◽  
Heinigerd Rebel ◽  
Markus Roth
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
High Energy ◽  
Mass Composition ◽  
High Energy Cosmic Rays

SPECTRUM OF COSMIC RAYS WITH ENERGY ABOVE 1017 EV

2005 ◽  
Vol 20 (29) ◽  
pp. 6878-6880 ◽  
Author(s):  
V. P. EGOROVA ◽  
A. V. GLUSHKOV ◽  
A. A. IVANOV ◽  
S. P. KNURENKO ◽  
V. A. KOLOSOV ◽  
...  
Keyword(s):  
Distribution Function ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Time Distribution ◽  
Arrival Time ◽  
Lateral Distribution ◽  
Arrival Time Distribution ◽  
Array Data ◽  
Lateral Distribution Function ◽  
High Energies

The energy spectrum of primary cosmic rays with ultra-high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The effect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered.

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