Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988sssmp..31.1240w&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 31, Oct. 1988, p.
Astronomy and Astrophysics
Astronomy
Bow Waves, Interplanetary Magnetic Fields, Magnetic Field Configurations, Magnetohydrodynamic Waves, Shock Wave Propagation, Computerized Simulation, Magnetosheath, Shock Wave Interaction, Solar Wind
Scientific paper
Fluctuations in plasma and magnetic fields on a time scale of the order of minutes are present in interplanetary space almost constantly and impinge on the bow shock from all directions. A model studying the interaction between MHD waves and the earth's bow shock under ordinary conditions is presented. The results show that the state of fluctuations undergoes a significant jump across the earth's bow shock. Simulations for the spatial variation in the state of fluctuations behind the bow shock reveal a dawn-dusk asymmetry higher in the dawn than in the dusk side. When the background IMF turns southward (or northward), the maximum region for the magnetic field fluctuations moves from lower to higher latitudes in the northern (or southern) hemisphere, so that the south-north (or north-south) asymmetry appears in magnetosheath fluctuation activities. This asymmetry could be one of the causes for some magnetospheric asymmetrical phenomena.
Du Heng
Wei Fengsi
Whang Yun C.
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