A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

Tail reconnection in the global magnetospheric context: Vlasiator first results




TekijätMinna Palmroth, Sanni Hoilijoki, Liisa Juusola, Tuija I. Pulkkinen, Heli Hietala, Yann Pfau-Kempf, Urs Ganse, Sebastian von Alfthan, Rami Vainio, Michael Hesse

KustantajaCOPERNICUS GESELLSCHAFT MBH

Julkaisuvuosi2017

JournalAnnales Geophysicae

Tietokannassa oleva lehden nimiANNALES GEOPHYSICAE

Lehden akronyymiANN GEOPHYS-GERMANY

Vuosikerta35

Numero6

Aloitussivu1269

Lopetussivu1274

Sivujen määrä6

ISSN0992-7689

DOIhttps://doi.org/10.5194/angeo-35-1269-2017

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/27886624


Tiivistelmä
The key dynamics of the magnetotail have been researched for decades and have been associated with either three-dimensional (3-D) plasma instabilities and/or magnetic reconnection. We apply a global hybrid-Vlasov code, Vlasiator, to simulate reconnection self-consistently in the ion kinetic scales in the noon-midnight meridional plane, including both dayside and nightside reconnection regions within the same simulation box. Our simulation represents a numerical experiment, which turns off the 3-D instabilities but models ion-scale reconnection physically accurately in 2-D. We demonstrate that many known tail dynamics are present in the simulation without a full description of 3-D instabilities or without the detailed description of the electrons. While multiple reconnection sites can coexist in the plasma sheet, one reconnection point can start a global reconfiguration process, in which magnetic field lines become detached and a plasmoid is released. As the simulation run features temporally steady solar wind input, this global reconfiguration is not associated with sudden changes in the solar wind. Further, we show that lobe density variations originating from dayside reconnection may play an important role in stabilising tail reconnection.

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Last updated on 2024-26-11 at 17:33