Occurrence of Magnetic Reconnection in the Deep Magnetotail: ARTEMIS Results

  • Zoltán VörösEmail author
  • Andrei Runov
  • Alexander Kendl
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 33)


Using two-probe ARTEMIS magnetic field and plasma measurements we have accomplished a survey of the occurrence of magnetic reconnection signatures in the distant magnetotail between October 2010 and June 2011. We have considered highly accelerated electron and fast bulk plasma flow events during ARTEMIS tail crossings. Our findings suggest that the deep-tail region between \(-60{R}_{E} < X(\mathit{GSM}) < -40{R}_{E}\) is rather active. Fourteen events have been found exhibiting signatures of magnetic reconnection occurrence during 29 days of plasma sheet crossings. Comparisons with mid-tail surveys of reconnection statistics indicate that the deep-tail region can play a significant role in global magnetosphere dynamics.



We acknowledge NASA contract NAS5- 02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically, C.W. Carlson and J.P. McFadden for use of ESA data, K. H. Glassmeier, U. Auster, and W. Baumjohann for use of FGM data, A. Roux and O. LeContel for use of SCM data. This work was made with the support of the ISSI team 185 “Dispersive cascade and dissipation in collisionless space plasma turbulence: observations and simulations”. The work was also supported by the Austrian Wissenschaftsfonds FWF under Grant No. Y398.


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Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • Zoltán Vörös
    • 1
    Email author
  • Andrei Runov
    • 2
  • Alexander Kendl
    • 3
  1. 1.Institute of Astro- and Particle PhysicsUniversity of InnsbruckInnsbruckAustria
  2. 2.Institute of Geophysics and Planetary PhysicsUniversity of CaliforniaLos AngelesUSA
  3. 3.Institute for Ion Physics and Applied PhysicsUniversity of InnsbruckInnsbruckAustria

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