Is the large-scale sidereal anisotropy of the galactic cosmic-ray intensity really instable at TeV energies?

2012 ◽  
Vol 36 (1) ◽  
pp. 237-241 ◽  
Author(s):  
M. Amenomori ◽  
X.J. Bi ◽  
D. Chen ◽  
W.Y. Chen ◽  
S.W. Cui ◽  
...  
Keyword(s):  
Large Scale ◽  
Cosmic Ray ◽  
Cosmic Ray Intensity ◽  
Galactic Cosmic Ray ◽  
Sidereal Anisotropy

scholarly journals Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array

2005 ◽  
Vol 626 (1) ◽  
pp. L29-L32 ◽  
Author(s):  
M. Amenomori ◽  
S. Ayabe ◽  
S. W. Cui ◽  
Danzengluobu ◽  
L. K. Ding ◽  
...  
Keyword(s):  
Large Scale ◽  
Cosmic Ray ◽  
Cosmic Ray Intensity ◽  
Air Shower ◽  
Galactic Cosmic Ray ◽  
Shower Array ◽  
Sidereal Anisotropy ◽  
Air Shower Array

Heliospheric signatures seen in the sidereal anisotropy of high-energy galactic cosmic ray intensity

2010 ◽  
Author(s):  
M. Amenomori ◽  
X. J. Bi ◽  
D. Chen ◽  
S. W. Cui ◽  
Danzengluobu ◽  
...  
Keyword(s):  
Cosmic Ray ◽  
High Energy ◽  
Cosmic Ray Intensity ◽  
Galactic Cosmic Ray ◽  
Sidereal Anisotropy

A two-way sidereal anisotropy

1968 ◽  
Vol 46 (10) ◽  
pp. S611-S613 ◽  
Author(s):  
K. Nagashima ◽  
H. Ueno ◽  
S. Mori ◽  
S. Sagisaka
Keyword(s):  
Time Variation ◽  
Cosmic Ray ◽  
Sidereal Time ◽  
Cosmic Ray Intensity ◽  
Data Support ◽  
Ion Chambers ◽  
Using Data ◽  
Sidereal Anisotropy

The sidereal time variation is analyzed using data for the ion chambers at Cheltenham and Christchurch for the period 1938–58 and for the meson and neutron components during the IGY. All the results derived from these three kinds of data support the existence of a two-way sidereal anisotropy, suggested by Jacklyn, which has two maxima of the cosmic-ray intensity in the directions of 8 h and 20 h S.T. (sidereal time).

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