Two-component model for cosmic-ray fluctuations at neutron monitor energies

Details Two-component model for cosmic-ray fluctuations at neutron monitor energies Two-component model for cosmic-ray fluctuations at neutron monitor energies

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....3.1107j&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 3. (A76-26851

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Cosmic Rays, Interplanetary Magnetic Fields, Neutrons, Particle Intensity, Anisotropy, Cross Correlation, Magnetic Effects, Monitors, Particle Energy, Power Spectra

Scientific paper

A formal model for the fluctuations of the cosmic-ray intensity near earth is presented. For frequencies exceeding 5 x 10 to the -6 Hz, the fluctuations are due to field-aligned-anisotropy induced interplanetary 'scintillations' of cosmic rays, while for lower frequencies the effects of non-field-aligned anisotropies dominate. Cross-correlations between neutron monitor counting rates and the interplanetary magnetic field components are presented which support the model.

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