Investigation of electron fluxes with energies of 40-500 keV in quiet periods of solar activity by the methods of correlation and spectral analysis

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Electron Flux Density, Interplanetary Medium, Solar Activity, Spectral Correlation, Spectrum Analysis, Cosmic Rays, Electron Energy, Energy Spectra, Galactic Radiation

Scientific paper

Prognoz-3 data from 1973-1974 on background fluxes of low-energy electrons (40-500 keV), observed in interplanetary space in the absence of solar-cosmic-ray flares, are examined. Fluctuation power spectra are calculated along with correlation functions of simultaneous series of low-energy electron fluxes, galactic cosmic rays, and certain parameters characterizing solar activity and the state of the interplanetary medium. The analysis indicates that the background fluxes of low-energy electrons have a possible solar origin, but not a flare-related one.

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