Dependence of the neutron monitor count rate and time delay distribution on the rigidity spectrum of primary cosmic rays

2016 ◽  
Vol 121 (12) ◽  
pp. 11,620-11,636 ◽  
Author(s):  
P.-S. Mangeard ◽  
D. Ruffolo ◽  
A. Sáiz ◽  
W. Nuntiyakul ◽  
J. W. Bieber ◽  
...  
Keyword(s):  
Time Delay ◽  
Cosmic Rays ◽  
Neutron Monitor ◽  
Count Rate ◽  
Delay Distribution ◽  
Rigidity Spectrum ◽  
Primary Cosmic Rays

scholarly journals Relationship between the Neutron Time Delay Distribution and the Rigidity Spectrum of Primary Cosmic Rays up to 16.8GV

2016 ◽  
Author(s):  
Pierre-Simon Mangeard ◽  
David Ruffolo ◽  
A. Saiz ◽  
Waraporn Nuntiyakul ◽  
Suttiwat Madlee ◽  
...  
Keyword(s):  
Time Delay ◽  
Cosmic Rays ◽  
Delay Distribution ◽  
Rigidity Spectrum ◽  
Neutron Time ◽  
Primary Cosmic Rays

Determination of the solar-flare cosmic-ray rigidity spectrum using the worldwide neutron monitor network

1970 ◽  
Vol 48 (4) ◽  
pp. 419-431 ◽  
Author(s):  
R. A. R. Palmeira ◽  
R. P. Bukata ◽  
P. T. Gronstal
Keyword(s):  
Cosmic Rays ◽  
Solar Flare ◽  
Neutron Monitor ◽  
Cosmic Ray ◽  
Spectral Exponent ◽  
The Earth ◽  
Rigidity Spectrum

The determination of the rigidity spectrum of solar-flare-produced cosmic rays is examined. A method based on the ratio of relative enhancements observed at two stations sufficiently separated in latitude is discussed, and graphs are presented showing the expected ratio of enhancements as a function of the spectral exponent of the flare-produced cosmic rays for 6 pairs of stations. This method, which assumes that the cosmic-ray particles arrive at the earth isotropically, is then applied to the 28 January 1967 event during which this condition of isotropy is shown to exist. An extension of this method to the case of anisotropic arrival of solar cosmic-ray particles using the concept of variational coefficient is outlined.

Rigidity Spectrum of Helium Nuclei above 17 GV and a Search for High Energy Anti-nuclei in Primary Cosmic Rays

1972 ◽  
Vol 240 (102) ◽  
pp. 135-137 ◽  
Author(s):  
R. P. VERMA ◽  
T. N. RENGARAJAN ◽  
S. N. TANDON ◽  
S. V. DAMLE ◽  
YASH PAL
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
Rigidity Spectrum ◽  
Primary Cosmic Rays

The energy spectrum of the heavy primary cosmic rays

1964 ◽  
Vol 281 (1387) ◽  
pp. 553-564 ◽  
Keyword(s):  
Cosmic Rays ◽  
Power Law ◽  
Solar Modulation ◽  
Cerenkov Counter ◽  
Plausible Assumption ◽  
Integral Spectrum ◽  
Upper Limit ◽  
The Earth ◽  
Rigidity Spectrum ◽  
Primary Cosmic Rays

The magnetic rigidity spectrum of primary cosmic rays with Z ≥ 6, in the rigidity interval 2·5 to 16·0 GV, has been determined by means of a Cerenkov counter carried in the satellite Ariel. The integral spectrum shows a well-defined change in slope near 8·5 GV, indicating that this is probably the upper limit to the solar modulation process at this time (May and June 1962). In the rigidity interval covered by these measurements the integral spectrum is adequately represented by a power law with an exponent ca . 1.2 below 8.5 GV and ca . 1.5 above this rigidity. Under the plausible assumption that the integral galactic spectrum of these particles is represented by a power law with exponent 1·5, it follows that the solar modulation process in the 2·5 to 8·5 GV region is of the form J E = J ∞ [p/p o ] 0·3 , where J E is the intensity at the Earth of particles with rigidity greater than p , where p is in GV, J ∞ is the corresponding intensity outside the solar system, and p 0 ~ 8·5.

Solar modulation of primary cosmic rays as deduced from neutron monitor data

1967 ◽  
Vol 72 (21) ◽  
pp. 5347-5356
Author(s):  
D. L. Bertsch ◽  
S. A. Fody
Keyword(s):  
Cosmic Rays ◽  
Neutron Monitor ◽  
Solar Modulation ◽  
Neutron Monitor Data ◽  
Monitor Data ◽  
Primary Cosmic Rays

Uncertanties of atmospheric high-energy muon fluxes and spectrum of primary cosmic rays

2007 ◽  
Vol 50 (9) ◽  
pp. 891-897
Author(s):  
A. A. Kochanov ◽  
T. S. Sinegovskaya ◽  
S. I. Sinegovskii
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
High Energy Muon ◽  
Primary Cosmic Rays

Search for sources of primary cosmic rays at energy above 0.1 PeV at the Tien Shan

2008 ◽  
Vol 175-176 ◽  
pp. 541-543 ◽  
Author(s):  
G. Benkó ◽  
A.P. Chubenko ◽  
G. Erdös ◽  
S.I. Nikolsky ◽  
N.M. Nesterova ◽  
...  
Keyword(s):  
Cosmic Rays ◽  
Tien Shan ◽  
Primary Cosmic Rays

scholarly journals On the mass composition of primary cosmic rays in the energy region 1015–1016eV

2012 ◽  
Vol 39 (10) ◽  
pp. 105202 ◽  
Author(s):  
Y F Novoseltsev ◽  
R V Novoseltseva ◽  
G M Vereshkov
Keyword(s):  
Cosmic Rays ◽  
Energy Region ◽  
Mass Composition ◽  
Primary Cosmic Rays
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