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Tail reconnection region versus auroral activity inferred from conjugate ARTEMIS plasma sheet flow and auroral observations

  • Published:2013-09 Issue:9 Volume:118 Page:5758-5766
  • ISSN:2169-9380
  • Container-title:Journal of Geophysical Research: Space Physics
  • language:en
  • Short-container-title:J. Geophys. Res. Space Physics

Author:

Nishimura Y.1,Lyons L. R.1,Xing X.1,Angelopoulos V.2,Donovan E. F.3,Mende S. B.4,Bonnell J. W.4,Auster U.5

Affiliation:

1. Department of Atmospheric and Oceanic Sciences; University of California, Los Angeles; Los Angeles California USA

2. Department of Earth and Space Sciences; University of California, Los Angeles; Los Angeles California USA

3. Department of Physics and Astronomy; University of Calgary; Calgary Alberta Canada

4. Space Science Laboratory; University of California, Berkeley; Berkeley California USA

5. Institut für Geophysik und extraterrestrische Physik; Technischen Universität Braunschweig; Braunschweig Germany

Funder

NASA

NSF

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference40 articles.

1. The development of the auroral substorm;Akasofu;Planet. Space Sci.,1964

2. The ARTEMIS mission;Angelopoulos;Space Sci. Rev.,2011

3. Statistical characteristics of bursty bulk flow events;Angelopoulos;J. Geophys. Res.,1994

4. Correlated dynamical changes in the near-Earth and distant magnetotail regions: ISEE 3;Baker;J. Geophys. Res.,1984

5. On the propagation of bubbles in the geomagnetic tail;Birn;Ann. Geophys.,2004

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4. Arase Observation of the Source Region of Auroral Arcs and Diffuse Auroras in the Inner Magnetosphere;Journal of Geophysical Research: Space Physics;2020-08

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