Variations of cosmic-ray intensity due to ionospheric waves during morning and evening hours

Details Variations of cosmic-ray intensity due to ionospheric waves during morning and evening hours Variations of cosmic-ray intensity due to ionospheric waves during morning and evening hours

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..486a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, May-June 1987, p. 486-488. In Russian.

Computer Science

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Cosmic Rays, Ionospheric Disturbances, Wave Propagation, Diurnal Variations, Frequency Response, Ionospheric Electron Density, Radiation Measuring Instruments, Spectrum Analysis

Scientific paper

The Alma-Ata neutron monitor located at a height of 3340 m above sea level was used to study cosmic-ray variations due to atmospheric waves. Peaks with periods of 1 and 2 hr in the variation spectrum were found which were also present in electron-density fluctuation spectra at heights of 70-100 km. The fluctuation spectra of both cosmic rays and the electron density were shifted to the low-frequency range with increasing time after sunrise or sunset. It is concluded that the spectral components of the cosmic-ray intensity variations may be due to ionospheric waves excited by the solar terminator.

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