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  • Magnetohydrodynamic Processes in Solar Plasmas

    Magnetohydrodynamic Processes in Solar Plasmas by Srivastava, Abhishek Kumar; Goossens, Marcel; Arregui, I?igo;

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      • Publisher's listprice EUR 143.00
      • The price is estimated because at the time of ordering we do not know what conversion rates will apply to HUF / product currency when the book arrives. In case HUF is weaker, the price increases slightly, in case HUF is stronger, the price goes lower slightly.

        60 360 Ft (57 486 Ft + 5% VAT)
      • Discount 10% (cc. 6 036 Ft off)
      • Discounted price 54 324 Ft (51 737 Ft + 5% VAT)

    60 360 Ft

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    Product details:

    • Publisher Elsevier
    • Date of Publication 14 May 2024

    • ISBN 9780323956642
    • Binding Paperback
    • No. of pages310 pages
    • Size 234x190 mm
    • Weight 450 g
    • Language English
    • 570

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    Long description:

    Magnetohydrodynamic Processes in Solar Plasmas provides a comprehensive theory and practice of basic plasma processes in the Sun and heliosphere. It deals with the basic dynamics of the Sun from its interior up to its outer atmosphere in the framework of Magnetohydrodynamics. Topics covered include essential phenomena in the solar interior such as magnetism, dynamos and helioseismology and in the solar atmosphere such as waves, shocks, instabilities, reconnection and coronal heating. The book provides frontline research aspects of solar plasma processes. In addition, the content is relevant for astrophysical plasmas, laboratory plasmas, fluid dynamics and related basic fields. Magnetohydrodynamic Processes in Solar Plasmas not only focuses on the fundamentals of the processes under consideration but in addition it presents recent research developments. In this manner it forms an essential reference for researchers, academics and advanced students in solar physics, astrophysics and related disciplines.

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    Table of Contents:

    1: Dynamical processes in the solar plasma

    2: Helioseismology

    3: The Sun’s magnetic cycle: observations and modeling

    4: MHD waves in homogeneous and continuously stratified atmospheres

    5: MHD waves in structured solar fluxtubes

    6: MHD waves in the partially ionized plasma: from single to multifluid approach

    7: Magnetohydrodynamic instabilities and transition to turbulence

    8: Shocks

    9: Magnetic reconnection

    10: Coronal heating

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