Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field
arXiv:astro-ph/9903337 · doi:10.1134/1.568025
Abstract
The Earth's magnetic field effect on the azimuthal distribution of extensive air showers (EAS) of cosmic rays has been evaluated using a bulk of the Yakutsk array data. The uniform azimuthal distribution of the EAS event rate is rejected at the significance level 10^(-14). Amplitude of the first harmonics of observed distribution depends on zenith angle as A1=0.2*sin^2(theta) and is almost independent of the primary energy; the phase coincides with the magnetic meridian. Basing upon the value of measured effect, the correction factor has been derived for the particle density depending on a geomagnetic parameter of a shower.
4 pages, 3 figures in ps files
Cited by in corpus (10)
- Observation of the Cosmic Ray Moon shadowing effect with ARGO-YBJ
- A Northern Sky Survey for Steady TeV Gamma-Ray Point Sources Using the Tibet Air Shower Array
- The rate of cosmic ray showers at large zenith angles: a step towards the detection of ultra-high energy neutrinos by the Pierre Auger Observatory
- The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory
- Detector Time Offset and Off-line Calibration in EAS Experiments
- The analog Resistive Plate Chamber detector of the ARGO-YBJ experiment
- The effect of atmospheric attenuation on inclined cosmic ray air showers
- A minimal width of the arrival direction distribution of ultra-high energy cosmic rays detected with the Yakutsk array
- Large-scale distribution of cosmic rays in right ascension as observed by the Yakutsk array at energies above eV
- A proposed method for measurement of cosmic-ray chemical composition based on geomagnetic spectroscopy