Investigation of low-energy cosmic rays by means of correlation and spectral analysis

Details Investigation of low-energy cosmic rays by means of correlation and spectral analysis Investigation of low-energy cosmic rays by means of correlation and spectral analysis

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..398g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, May-June 1979, p. 398-404. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Cosmic Rays, Interplanetary Space, Solar Protons, Correlation Coefficients, Power Spectra, Satellite Observation, Spectrum Analysis, Time Response

Scientific paper

Prognoz-satellite data were used to study the background intensity of protons in the 1-4.5 MeV energy range present in interplanetary space in the absence of solar cosmic ray bursts. Information on the origin and properties of these protons is derived from an analysis of their fluctuation-power spectra; a correlation analysis of the data involves investigation of the relation of proton fluxes to fluxes of galactic cosmic rays, interplanetary magnetic field strength, and solar activity index.

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