scholarly journals Interplanetary Magnetic Field Turbulence and Rigidity Spectrum of the Galactic Cosmic Rays Intensity Variation (1969–2011)

2018 ◽  
Vol 123 (1) ◽  
pp. 30-38 ◽  
Author(s):  
M. Siluszyk ◽  
M. V. Alania ◽  
K. Iskra ◽  
S. Miernicki
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
Interplanetary Magnetic Field ◽  
Intensity Variation ◽  
Galactic Cosmic Rays ◽  
Rigidity Spectrum ◽  
Magnetic Field Turbulence

Anisotropy of Galactic Cosmic Rays and the Interplanetary Magnetic Field

Nature ◽  
1965 ◽  
Vol 206 (4985) ◽  
pp. 703-704 ◽  
Author(s):  
V. SARABHAI ◽  
G. L. PAI ◽  
M. WADA
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
Interplanetary Magnetic Field ◽  
Galactic Cosmic Rays

Streaming of galactic cosmic rays in the interplanetary magnetic field

Solar Physics ◽  
1972 ◽  
Vol 22 (1) ◽  
pp. 220-234 ◽  
Author(s):  
A. Hashim ◽  
M. Bercovitch ◽  
J. F. Steljes
Keyword(s):  
Magnetic Field ◽  
Cosmic Rays ◽  
Interplanetary Magnetic Field ◽  
Galactic Cosmic Rays

Gradient of galactic cosmic rays normal to the solar equatorial plane

1968 ◽  
Vol 46 (10) ◽  
pp. S981-S984 ◽  
Author(s):  
D. Patel ◽  
V. Sababhai ◽  
G. Subramanian
Keyword(s):  
Magnetic Field ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Interplanetary Magnetic Field ◽  
Equatorial Plane ◽  
Cosmic Ray ◽  
Galactic Cosmic Rays ◽  
Cosmic Ray Intensity ◽  
Positive Exponent ◽  
Ray Density

Predictions concerning the anisotropy of galactic cosmic rays due to a gradient of cosmic-ray density perpendicular to the solar equatorial plane have been verified experimentally as follows. (1) The energy spectrum of the variation of the semidiurnal component has a positive exponent. (2) The diurnal and the semidiurnal components are oriented with respect to the interplanetary magnetic field. (3) A deficiency of cosmic-ray intensity, Tmin, is observed along the direction of the interplanetary magnetic field on days when the energy spectrum of the diurnal variation has an exponent different from zero.

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