Direction of semi-diurnal anisotropy in relation to interplanetary magnetic fields

Details Direction of semi-diurnal anisotropy in relation to interplanetary magnetic fields Direction of semi-diurnal anisotropy in relation to interplanetary magnetic fields

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ijrsp..11..124a&link_type=abstract

Indian Journal of Radio and Space Physics, vol. 11, June 1982, p. 124, 125.

Physics

Space Physics

Cosmic Rays, Interplanetary Magnetic Fields, Anisotropy, Annual Variations, Particle Flux Density

Scientific paper

A comparison of the direction of the maximum flux of the second harmonic of the daily variation of cosmic ray intensity observed at Deep River with the direction of the interplanetary magnetic field has been made for each day during 1973-75. The results show that, in general, the direction of the maximum flux is perpendicular to the direction of the interplanetary magnetic field which is in agreement with the earlier observations as well as with the theoretical predictions

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