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10.7 MB
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A0363F94D8D2B6C7616D3D9F01FF1413FDB1F9EC
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April 21, 2026, 1:51 a.m.
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(Last updated: April 21, 2026, 1:56 a.m.)
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| Leonovich A. Magnetospheric MHD Oscillations. A Linear Theory 2024.pdf | 10.7 MB |
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SOURCE: Leonovich A. Magnetospheric MHD Oscillations. A Linear Theory 2024
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MEDIAINFO
Textbook in PDF format The magnetosphere is the region around Earth in which our planet’s magnetic field exerts its influence to trap charged particles. Waves in this magnetosphere, known as magnetohydrodynamic (MHD) oscillations, are caused by interactions between these charged particles, Solar wind pulses, and the magnetic field. The predictable interval between these oscillations enables them to serve as tools for understanding the magnetospheric plasma which comprises the field. Magnetospheric MHD Oscillations offers a comprehensive overview of the theory underlying these waves and their periodicity. Emphasizing the spatial structure of the oscillations, it advances a theory of MHD oscillation that promises to have significant ramifications in astronomy and beyond
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