Study of cosmic ray scintillations from 5-minute data of the scintillations telescope Izmran and world-wide network stations

Details Study of cosmic ray scintillations from 5-minute data of the scintillations telescope Izmran and world-wide network stations Study of cosmic ray scintillations from 5-minute data of the scintillations telescope Izmran and world-wide network stations

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..281g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 281-284 (SEE N85-34991 23-93)

Other

Cosmic Rays, Interplanetary Space, Particle Telescopes, Scintillation Counters, Amplitudes, Charged Particles, Periodic Variations, Spectrum Analysis, Turbulence

Scientific paper

During cosmic ray propagation in interplanetary space there appear characteristic cosmic-ray intensity scintillations which are due to charged particle scattering on random inhomogeneities of the interplanetary magnetic field. The power spectra of cosmic ray scintillations on the Earth during some intervals from 1977 to 1982 (for quiet periods, for solar flares and Forbush decreases due to power shock waves) have been calculated from five-minute, one and two-hour values of the cosmic-ray intensity measured by the scintillator supertelescope IZMIRAN. The spectra were estimated by the methods of spectral analysis and by autoregressive methods which mutually control each other and make it possible not only to analyze scintillation powers at distinguished frequencies, but also to determine the behavior of spectrum slopes in some frequency ranges.

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