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Magnetic cloud as a dual-polarity flux rope

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    0124856 - ASU-R 20010109 RIV US eng C - Conference Paper (international conference)
    Vandas, Marek - Geranios, A.
    Magnetic cloud as a dual-polarity flux rope.
    Recent insights onto the physics of the Sun and heliosphere. Highlights from SOHO and other space missions. San Francisco: Astronomical Society of the Pacific, 2001 - (Brekke, P.; Fleck, B.; Gurman, J.), s. 541-543
    [Symposium of the International Astronomical Union /203./. Manchester (GB), 05.08.2000-18.08.2000]
    R&D Projects: GA ČR GA205/99/1712; GA MŠMT ME 183; GA AV ČR IBS1003006
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : solar wind * interplanetary magnetic field * magnetic clouds
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    The magnetic cloud of November 17/18, 1975 is analyzed and it is shown that measurements of magnetic field and solar wind plasma are consistent with the interpretation that this magnetic cloud is a dual-polarity flux rope which consists of a cor and an annular region. The core has a strong magnetic field, the annular region has a higher plasma density and opposite magnetic polarity.
    Permanent Link: http://hdl.handle.net/11104/0023115


     
     

Number of the records: 1  

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