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AnatolyLeonovich,DmitriKlimushkin,VitaliiMazur

Magnetospheric MHD Oscillations: A Linear Theory

Magnetospheric MHD Oscillations: A Linear Theory

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  • More about Magnetospheric MHD Oscillations: A Linear Theory


A new theory of the magnetosphere explains magnetohydrodynamic (MHD) oscillations, which are caused by interactions between charged particles, Solar wind pulses, and the magnetic field. This theory offers a comprehensive overview of the theory underlying these waves and their periodicity and has significant ramifications for astronomy and beyond.

Format: Hardback
Length: 448 pages
Publication date: 17 April 2024
Publisher: Wiley-VCH Verlag GmbH


The magnetosphere is a crucial region surrounding Earth where our planet's magnetic field plays a pivotal role in capturing charged particles. Within this dynamic environment, waves known as magnetohydrodynamic (MHD) oscillations emerge due to intricate interactions among these charged particles, solar wind pulses, and the magnetic field. These oscillations exhibit a predictable interval, making them invaluable tools for gaining insights into the magnetospheric plasma, which constitutes the magnetic field.

Magnetospheric MHD Oscillations provides a comprehensive exploration of the theoretical foundations behind these waves and their periodic nature. It delves into the spatial structure of the oscillations, proposing a novel theory of MHD oscillation that holds significant promise for fields beyond astronomy. The book offers readers a deep understanding of various topics, including Alfven resonance, waveguides in plasma filaments, and numerous other crucial aspects. Additionally, detailed appendices are included, containing essential calculations and statistical parameters, making it an invaluable resource for plasma physicists, theoretical physicists, applied mathematicians, and advanced graduate students engaged in these and related subfields.

Weight: 992g
Dimension: 244 x 170 x 30 (mm)
ISBN-13: 9783527414307

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