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  • Waves and Oscillations in the Solar Atmosphere (IAU S247): Heating and Magneto-Seismology

    Waves and Oscillations in the Solar Atmosphere (IAU S247) by Erdélyi, Robert; Mendoza-Briceno, César A.;

    Heating and Magneto-Seismology

    Series: Proceedings of the International Astronomical Union Symposia and Colloquia;

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      • Publisher's listprice GBP 72.00
      • 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.

        34 398 Ft (32 760 Ft + 5% VAT)
      • Discount 10% (cc. 3 440 Ft off)
      • Discounted price 30 958 Ft (29 484 Ft + 5% VAT)

    34 398 Ft

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    Availability

    Estimated delivery time: In stock at the publisher, but not at Prospero's office. Delivery time approx. 3-5 weeks.
    Not in stock at Prospero.

    Why don't you give exact delivery time?

    Delivery time is estimated on our previous experiences. We give estimations only, because we order from outside Hungary, and the delivery time mainly depends on how quickly the publisher supplies the book. Faster or slower deliveries both happen, but we do our best to supply as quickly as possible.

    Product details:

    • Publisher Cambridge University Press
    • Date of Publication 12 June 2008

    • ISBN 9780521874694
    • Binding Hardback
    • No. of pages398 pages
    • Size 244x179x24 mm
    • Weight 940 g
    • Language English
    • Illustrations 15 b/w illus. 10 tables
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    Short description:

    Provides the latest summary on the solar coronal heating enigma and magneto-seismology of the solar atmosphere, for solar physics researchers.

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    Long description:

    IAU Symposium 247 addresses the latest discoveries on magnetic waves and oscillations, observed recently in the atmosphere of the Sun. The energy sources which maintain the extraordinarily high temperature of the Sun's outer coronal layer continue to fascinate solar researchers. It is now clear that the ubiquitous magnetic fields in the solar atmosphere are the crucial ingredient to understanding the solar corona. These proceedings of IAU S247 contain a selection of presentations and reviews made by internationally renowned scientists on the solar heating enigma and magneto-seismology of the solar atmosphere. It emphasizes magnetic wave and oscillation observations in different observational bands, consolidation of the theory and the observational findings, and observations with new and future solar missions.

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    Table of Contents:

    Preface; Organizing committee; Conference participants; Address by the Scientific Organizing Committee R. Erd&&&233;lyi; Progress in coronal seismology B. Roberts; Session 1. Waves and oscillations in solar and stellar interior Robert Erd&&&233;lyi; Session 2. Coupling of global solar and stellar motions into the lower atmosphere Bernard Roberts; Session 3. Seismology of the lower solar atmosphere and stellar chromospheres Siraj S. Hasan; Session 4. Seismology of open versus closed magnetic structures Marcel Goossens; Session 5. Prominence seismology Jose Luis Ballester; Session 6. Dynamical processes and coupling in the magnetic atmosphere of Sun and stars Miguel Iba&&&241;ez; Session 7. Wave-particle interactions in magnetized plasmas Cesar A. Mendoza-Brice&&&241;o; Session 8. Solar and stellar global coronal seismology Viggo Hansteen; Session 9. Fundamental physical processes in coronae: waves, turbulence, reconnection Saku Tsuneta; Session 10. Waves and instabilities in atmospheric plasmas Arnold O. Benz; Summary of meeting Cesar A. Mendoza-Brice&&&241;o; Concluding remarks A. O. Benz; Late papers; Author index.

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