Abstract Magnetic reconnection takes place in the magnetotail of the Earth and it plays key roles in the formation of the plasma sheet and in the energy release during substorms. Three types of reconnection phenomena have been identified. These are, reconnection in the distant tail (> 100 Re), reconnection in the near tail (20 – 30 Re) associated with substorms, and formation of distributed magnetic loops in the neutral sheet. We review (1) signatures of each type of reconnection, (2) the structure of the energy conversion region with particular attention on the distinction between accelerations at the slow shock and in the neutral sheet, and (3) the condition for the onset of reconnection.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Magnetic reconnection in the tail of the magnetosphere


    Beteiligte:
    Nishida, A. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 10 , 9 ; 135-144


    Erscheinungsdatum :

    1990-01-01


    Format / Umfang :

    10 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Pivotal Role of Magnetic Reconnection in the Earth's Magnetosphere

    Nishida, A. / International Council of Scientific Unions | British Library Conference Proceedings | 2000



    Tail reconnection and plasma sheet fast flows

    Nakamura, R. / Baumjohann, W. / Runov, A. et al. | British Library Conference Proceedings | 2006


    Tail current sheet dynamics in the disturbed magnetosphere

    Alexeev, I.I. / Belenkaya, E.S. / Kalegaev, V.V. | Elsevier | 1993


    Magnetic Fluxtube Reconnection

    Dahlburg, R. B. / Antiochos, S. K. / COSPAR; Scientific Commission D | British Library Conference Proceedings | 1997