Other
Scientific paper
Sep 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39.1233v&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 39, Sept. 1991, p. 1233-1238.
Other
7
Heliosphere, Interplanetary Magnetic Fields, Magnetic Effects, Magnetic Field Inversions, Neutral Sheets, Solar Cosmic Rays, Solar Magnetic Field, Diurnal Variations, Mathematical Models, Periodic Variations, Plasma-Electromagnetic Interaction, Solar Activity
Scientific paper
A drift with a simulated wavy neutral sheet have been used to study the effects of the reversal of the solar magnetic field every 11 years and the changes in the waviness of the heliospheric neutral sheet, corresponding to changes in solar activity, on the diurnal anisotropy at an energy of 20 GeV. The results indicate that the long-term behavior of the diurnal anisotropy, especially the phase shift from one solar minimum period to another, which seems to depend on the polarity of the IMF, has a theoretical explanation in the drift picture of the modulation of cosmic rays in the heliosphere.
Potgieter Marius S.
van Staden M. L.
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