Large amplitude wave-trains of cosmic-ray intensity

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Cosmic Rays, Data Processing, Diurnal Variations, Neutron Spectra, Particle Diffusion, Radiant Flux Density, Anisotropy, Explorer 47 Satellite, Explorer 50 Satellite, Heos Satellites, Interplanetary Magnetic Fields, Polar Regions, Solar Wind, Temperate Regions

Scientific paper

The large amplitude wave-trains of cosmic-ray intensity observed during June, July and August, 1973, were analyzed. These events exhibit the same characteristics as the event of May, 1973. During these days the phase of the enhanced diurnal anisotropy is shifted to a point earlier than either the corotation direction or the anti-garden-hose direction. For this analysis data from high- and middle-latitude neutron monitors and from the satellites HEOS-2, IMP-7 and IMP-8 were used. The diurnal variation of these days is well understood in terms of a radially outward convective vector and a field-aligned inward diffusive vector yielding a diurnal anisotropy vector along about 1600 h in space.

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