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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 16, issue 5
Ann. Geophys., 16, 528–541, 1998
https://doi.org/10.1007/s00585-998-0528-5
© European Geosciences Union 1998
Ann. Geophys., 16, 528–541, 1998
https://doi.org/10.1007/s00585-998-0528-5
© European Geosciences Union 1998

  31 May 1998

31 May 1998

Magnetotail response during a strong substorm as observed by GEOTAIL in the distant tail

A. Belehaki1, R. W. McEntire2, S. Kokubun3, and T. Yamamoto4 A. Belehaki et al.
  • 1Institute of Space Research, National Observatory of Athens, Metaxa and Vas. Pavlou Str., Palaia Pendeli, GR-152 36, Greece
  • 2The Johns Hopkins University, Applied Physics Laboratory, Laurel, MD 20723, USA
  • 3Solar Terrestrial Environment Laboratory, Nagoya University, Toyokawa Aichi, 442, Japan
  • 4Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229, Japan

Abstract. Simultaneous energetic particle and magnetic field observations from the GEOTAIL spacecraft in the distant tail (XGSM≈ –150 Re) have been analysed to study the response of the Earth's magnetotail during a strong substorm (AE ≤ 680 nT). At geosynchronous altitude, LANL spacecraft recorded three electron injections between 0030 UT and 0130 UT, which correspond to onsets observed on the ground at Kiruna Ground Observatory. The Earth's magnetotail responded to this substorm with the ejection of five plasmoids, whose size decreases from one plasmoid to the next. Since the type of magnetic structure detected by a spacecraft residing the lobes, depends on the Z extent of the structure passing underneath the spacecraft, GEOTAIL is first engulfed by a plasmoid structure; six minutes later it detects a boundary layer plasmoid (BLP) and finally at the recovery phase of the substorm GEOTAIL observes three travelling compression regions (TCRs). The time-of-flight (TOF) speed of these magnetic structures was estimated to range between 510 km/s and 620 km/s. The length of these individual plasmoids was calculated to be between 28 Re and 56 Re. The principal axis analysis performed on the magnetic field during the TCR encountered, has confirmed that GEOTAIL observed a 2-D perturbation in the X-Z plane due to the passage of a plasmoid underneath. The first large plasmoid that engulfed GEOTAIL was much more complicated in nature probably due to the external, variable draped field lines associated with high beta plasma sheet and the PSBL flux tubes surrounding the plasmoid. From the analysis of the energetic particle angular distribution, evidence was found that ions were accelerated from the distant X-line at the onset of the burst associated with the first magnetic structure.

Key words. Magnetospheric physics (magnetospheric configuration and dynamics; magnetotail).

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