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Magnetic Reconnection in Different Environments: Similarities and Differences

  • Michael Hesse
  • , Nicolas Aunai
  • , Masha Kuznetsova
  • , Seiji Zenitani
  • , Joachim Birn
  • NASA Goddard Space Flight Center
  • National Astronomical Observatory
  • MST-8, Los Alamos National Laboratory
  • Space Science Institute

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Résumé

This chapter addresses two important aspects of magnetic reconnection: time-dependent rates affected by island formation and the preferred direction of the reconnection line if merging magnetic field components are not anti-parallel. While it is widely known that magnetic reconnection facilitates mass, momentum, and energy transport in plasmas, it is illustrative to consider an analytical approach to describing the efficacy of reconnection as a transport mechanism. The chapter performs a detailed analysis of the correlation between diffusion region dimensions and reconnection rate. For this purpose, it employs open boundary condition calculations of a continuously driven reconnecting system. In summary, results indicate that the magnetic reconnection line in asymmetric systems is preferentially oriented in such a way that it bisects the direction of the asymptotic magnetic field direction on both inflow sides. This orientation is identical to the one for which the product of available magnetic energy is maximized.

langue originaleAnglais
titreMagnetotails in the Solar System
Editeurwiley
Pages259-267
Nombre de pages9
ISBN (Electronique)9781118842324
ISBN (imprimé)9781118842348
Les DOIs
étatPublié - 9 janv. 2015
Modification externeOui

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