Isbn: 9780792328452 - solar surface magnetism: proceedings of the nato advanced research workshop, soesterberg, the netherlands, november 1-5, 1993: v. 433 (8 risultati)

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  • Lingua: Inglese

    Editore: Springer, 1994

    0792328450 / 9780792328452

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    Da: BOOKWEST, Phoenix, AZ, U.S.A.BOOKWEST

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  • Lingua: Inglese

    Editore: Springer, 1994

    0792328450 / 9780792328452

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    • Prima edizione

    Da: BOOKWEST, Phoenix, AZ, U.S.A.BOOKWEST

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    EUR 75,57

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    Hardcover. Condizione: New. 1st Edition. US SELLER SHIPS FAST FROM USA.

  • Lingua: Inglese

    Editore: Kluwer Academic Publishers, 1994

    0792328450 / 9780792328452

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    Da: Ria Christie Collections, Uxbridge, Regno UnitoRia Christie Collections

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    EUR 103,75

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    Condizione: New. In English.

  • Lingua: Inglese

    Editore: Springer Netherlands, 1994

    0792328450 / 9780792328452

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    Da: moluna, Greven, Germaniamoluna

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    EUR 104,46

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    Gebunden. Condizione: New. While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection and magnetic field in the photosphere regulates the field dispersal and drives the instabilities which heat the outer so.

  • Lingua: Inglese

    Editore: Kluwer Academic Pub, 1994

    0792328450 / 9780792328452

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    Da: Revaluation Books, Exeter, Regno UnitoRevaluation Books

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    EUR 145,42

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    Hardcover. Condizione: Brand New. 1st edition. 552 pages. 10.00x6.75x1.25 inches. In Stock.

  • Lingua: Inglese

    Editore: Springer, 1994

    0792328450 / 9780792328452

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    Da: AHA-BUCH GmbH, Einbeck, GermaniaAHA-BUCH GmbH

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    EUR 531,73

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    Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection and magnetic field in the photosphere regulates the field dispersal and drives the instabilities which heat the outer solar atmosphere. The book presents a synthesis between observers and theorists, both with regard to the magnetic elements which make up solar magnetic fields (ranging from tiny flux tubes to whole active regions), and to the surface patterns in which these elements display properties of the subsurface dynamo. A major breakthrough comes from numerical simulations. Modeling of flux concentration, flux tube dynamics, penumbral topology, umbral fine structure, etc. turns solar physics into an experimental science. The reviews and research papers in this volume provide an up-to-date overview of the solar frontier of astrophysical magnetohydrodynamics. The elements and patterns of solar surface magnetism contain much information about the subsurface solar dynamo as well as on the magnetically dominated energy budget and structuring of the outer solar atmosphere. The volume treats high-resolution solar polarimetry, the physics of solar magnetic elements, and the information contained in their patterns of emergence on the solar surface in depth, with a good balance between theoretical and observational studies.

  • Lingua: Inglese

    Editore: Kluwer Academic Publishers, 1994

    0792328450 / 9780792328452

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    Da: THE SAINT BOOKSTORE, Southport, Regno UnitoTHE SAINT BOOKSTORE

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    Hardback. Condizione: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.

  • Lingua: Inglese

    Editore: SPRINGER NATURE Mai 1994, 1994

    0792328450 / 9780792328452

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    Da: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermaniaBuchWeltWeit Ludwig Meier e.K.

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    Buch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection and magnetic field in the photosphere regulates the field dispersal and drives the instabilities which heat the outer solar atmosphere. The book presents a synthesis between observers and theorists, both with regard to the magnetic elements which make up solar magnetic fields (ranging from tiny flux tubes to whole active regions), and to the surface patterns in which these elements display properties of the subsurface dynamo. A major breakthrough comes from numerical simulations. Modeling of flux concentration, flux tube dynamics, penumbral topology, umbral fine structure, etc. turns solar physics into an experimental science. The reviews and research papers in this volume provide an up-to-date overview of the solar frontier of astrophysical magnetohydrodynamics. The elements and patterns of solar surface magnetism contain much information about the subsurface solar dynamo as well as on the magnetically dominated energy budget and structuring of the outer solar atmosphere. The volume treats high-resolution solar polarimetry, the physics of solar magnetic elements, and the information contained in their patterns of emergence on the solar surface in depth, with a good balance between theoretical and observational studies. 552 pp. Englisch.