Počet záznamů: 1

Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes

  1. 1.
    0355335 - ASU-R 2015 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
    Vandas, Marek - Romashets, E. P.
    Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes.
    Twelfth International Solar Wind Conference. Proceedings Paper. New York: Melville, 2010 - (Maksimovic, M.; Issautier, K.; Meyer-Vernet, N.; Moncuquet, M.; Pantellini, F.), s. 399-402. AIP Conference Proceedings, 1216. ISBN 978-0-7354-0759-6. ISSN 0094-243X.
    [Twelve International Solar Wind Conference. Saint-Malo (FR), 21.06.2009-26.06.2009]
    Grant CEP: GA AV ČR 1QS300120506; GA ČR GA205/09/0170; GA MŠk ME09032
    Výzkumný záměr: CEZ:AV0Z10030501
    Klíčová slova: solar magnetism * corona * magnetohydrodynamics
    Kód oboru RIV: BL - Fyzika plazmatu a výboje v plynech

    It is widely accepted that magnetic disturbances around fast interplanetary magnetic clouds can play an important role in their geo-effectiveness. An analytical solution for magnetic field in the sheath region of a cylindrical magnetic cloud with an elliptical cross-section is proposed. Upstream magnetic field can have an arbitrary direction. Normal magnetic field components are conserved through the bow shock with a high accuracy.
    Trvalý link: http://hdl.handle.net/11104/0194131