A study has been conducted at Ahmedabad during 1957 and 1958 of the time variations of meson intensity incident from east and west at 45° to the vertical. A characteristic difference of about 6 h in the diurnal time of maximum for the east and west directions is observed to occur on many days and this has been interpreted as signifying an anisotropy of primary radiation caused by a source outside the influence of the geomagnetic field. However, there are many days on which the daily variation has a maximum near noon for both directions. On such days the predominant influence is that of a local source situated within the influence of the geomagnetic field. The local source is associated with geomagnetically disturbed days. Long-term changes ...
The dependence of the counting rate of a cosmic ray detector on the asymptotic directions of approac...
The results of the day-to-day analysis of cosmic ray daily variation with a very high counting rate ...
The primary purpose of this investigation was to study the diurnal variation of cosmic-ray intensity
Changes of the energy spectrum of primary cosmic radiation can be followed through the time variatio...
The daily variation of cosmic ray intensity at low latitudes can under certain conditions be associa...
A study of cosmic ray intensity variations has been conducted during 1956–57 at the equatorial mount...
The daily variations of total cosmic ray intensity and the intensities of meson and electron compone...
The search for an anisotrophy in the penetrating component of the cosmic-ray flux is usually carried...
The diurnal anisotropy of cosmic ray intensity has been investigated over the interval 1973\u2013197...
151-156A systematic and detailed analysis of the diurnal anisotropy on geomagnetically quiet days ha...
Conventional interpretations of the Cosmic Ray Diurnal Variation gener-ally assume that the mean vie...
From a careful examination of the diurnal variation of cosmic ray intensity at high energies and the...
233-236The average behaviour of the daily variation of cosmic ray intensity has been studied for a l...
A study of the cosmic ray intensity data from high-latitude stations reveals an isotropic variation ...
The diurnal anisotropy of cosmic ray intensity for the time period 2001 to 2014 is studied, coverin...
The dependence of the counting rate of a cosmic ray detector on the asymptotic directions of approac...
The results of the day-to-day analysis of cosmic ray daily variation with a very high counting rate ...
The primary purpose of this investigation was to study the diurnal variation of cosmic-ray intensity
Changes of the energy spectrum of primary cosmic radiation can be followed through the time variatio...
The daily variation of cosmic ray intensity at low latitudes can under certain conditions be associa...
A study of cosmic ray intensity variations has been conducted during 1956–57 at the equatorial mount...
The daily variations of total cosmic ray intensity and the intensities of meson and electron compone...
The search for an anisotrophy in the penetrating component of the cosmic-ray flux is usually carried...
The diurnal anisotropy of cosmic ray intensity has been investigated over the interval 1973\u2013197...
151-156A systematic and detailed analysis of the diurnal anisotropy on geomagnetically quiet days ha...
Conventional interpretations of the Cosmic Ray Diurnal Variation gener-ally assume that the mean vie...
From a careful examination of the diurnal variation of cosmic ray intensity at high energies and the...
233-236The average behaviour of the daily variation of cosmic ray intensity has been studied for a l...
A study of the cosmic ray intensity data from high-latitude stations reveals an isotropic variation ...
The diurnal anisotropy of cosmic ray intensity for the time period 2001 to 2014 is studied, coverin...
The dependence of the counting rate of a cosmic ray detector on the asymptotic directions of approac...
The results of the day-to-day analysis of cosmic ray daily variation with a very high counting rate ...
The primary purpose of this investigation was to study the diurnal variation of cosmic-ray intensity