作者: G. D. Aburjania , Z. A. Kereselidze , A. G. Khantadze , M. S. Chkhitunidze
DOI: 10.1134/S0016793207050027
关键词: Magnetopause 、 Computational physics 、 Interplanetary magnetic field 、 Magnetosphere particle motion 、 Magnetosphere 、 Physics 、 Geophysics 、 Dipole model of the Earth's magnetic field 、 Magnetosheath 、 Earth's magnetic field 、 Mercury's magnetic field 、 Space and Planetary Science
摘要: The model equations describing the dynamics of solar wind and interplanetary magnetic field in dayside Earth’s magnetosheath have been studied. large-scale flow structure near critical point magnetosphere is determined an approximation Chaplygin stagnation zone identified with focal part. It has indicated that gradient waves (MGWs), which represent a special branch ULF electromagnetic oscillations magnetospheric resonator, can be generated magnetized plasma case when distribution spatially inhomogeneous. characteristic frequencies, periods, phase velocities, wavelengths, amplitudes MGW pulsations determined.