Solar and terrestrial relationships of the changes of anisotropy have been studied, and theories have been advanced to explain the creation of the anisotropy by a modulation of cosmic-ray intensity incident at particular directions. The results of the investigation presented are of a preliminary character and indicate certain tentative conclusions which can be drawn from the analysis of data from narrow-angle telescopes operated over a period of eleven months in 1956. One of the most important conclusions is that there is a definite correlation between day to day changes of anisotropy and the daily mean intensity
A study has been conducted at Ahmedabad during 1957 and 1958 of the time variations of meson intensi...
Changes of the energy spectrum of primary cosmic radiation can be followed through the time variatio...
Aims. We study features of the 3D solar anisotropy of Galactic cosmic rays (GCR) for 1965−2014 (almo...
A long-standing investigations of the cosmic ray anisotropy with muon telescopes and the ionization ...
A study of cosmic ray intensity variations has been conducted during 1956–57 at the equatorial mount...
The results of a measurement of the anisotropic character of the cosmic radiation in the vicinity of...
The daily variation of cosmic ray intensity at low latitudes can under certain conditions be associa...
A study of the cosmic ray intensity data from high-latitude stations reveals an isotropic variation ...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
At least four processes appear capable of contributing to the creation of an anisotropy of galactic ...
The diurnal anisotropy of cosmic ray intensity for the time period 2001 to 2014 is studied, coverin...
1.1 Introductory Remarks There is now considerable evidence that the charged primary cosmic radiati...
We analyze the temporal variation of the solar diurnal anisotropy of the multi-TeV cosmic-ray intens...
In this paper an attempt is made to study the occurrence of a large number of high amplitude anisotr...
A study has been conducted at Ahmedabad during 1957 and 1958 of the time variations of meson intensi...
Changes of the energy spectrum of primary cosmic radiation can be followed through the time variatio...
Aims. We study features of the 3D solar anisotropy of Galactic cosmic rays (GCR) for 1965−2014 (almo...
A long-standing investigations of the cosmic ray anisotropy with muon telescopes and the ionization ...
A study of cosmic ray intensity variations has been conducted during 1956–57 at the equatorial mount...
The results of a measurement of the anisotropic character of the cosmic radiation in the vicinity of...
The daily variation of cosmic ray intensity at low latitudes can under certain conditions be associa...
A study of the cosmic ray intensity data from high-latitude stations reveals an isotropic variation ...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
At least four processes appear capable of contributing to the creation of an anisotropy of galactic ...
The diurnal anisotropy of cosmic ray intensity for the time period 2001 to 2014 is studied, coverin...
1.1 Introductory Remarks There is now considerable evidence that the charged primary cosmic radiati...
We analyze the temporal variation of the solar diurnal anisotropy of the multi-TeV cosmic-ray intens...
In this paper an attempt is made to study the occurrence of a large number of high amplitude anisotr...
A study has been conducted at Ahmedabad during 1957 and 1958 of the time variations of meson intensi...
Changes of the energy spectrum of primary cosmic radiation can be followed through the time variatio...
Aims. We study features of the 3D solar anisotropy of Galactic cosmic rays (GCR) for 1965−2014 (almo...