Open AccessGeotail observations of energetic ion species and magnetic field in plasmoid‐like structures in the course of an isolated substorm event
Author(s) -
Zong Q.G.,
Wilken B.,
Reeves G. D.,
Daglis I. A.,
Doke T.,
Iyemori T.,
Livi S.,
Maezawa K.,
Mukai T.,
Kokubun S.,
Pu Z.Y.,
Ullaland S.,
Woch J.,
Lepping R.,
Yamamoto T.
Publication year - 1997
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/97ja00076
Subject(s) - plasmoid , substorm , physics , magnetosphere , ion , astrophysics , atomic physics , geosynchronous orbit , plasma , magnetic reconnection , nuclear physics , astronomy , satellite , quantum mechanics
On January 15, 1994, the ion spectrometer high energy particle ‐ low energy particle detector (HEP‐LD) on the Japanese spacecraft Geotail observed five quasi‐periodic energetic ion bursts in the deep tail (X=−96 R E ). These bursts were associated with plasmoid‐like structures in the magnetic field components. In. addition, three multiple TCR groups were identified in the interval. The observations in the distant tail occurred during a time interval of substorm activity which also produced multiple injections in the geosynchronous orbit region. The HEP‐LD observations show that B z bipolar plasmoid‐like structures are associated with tailward flowing particle bursts. However, earthward flowing particle bursts are predominantly associated with bipolar signatures in B y . In addition, an oxygen burst was seen in the back of a plasmoid (postplasmoid) which showed both B y and B z bipolar magnetic field signatures. The oxygen burst lasted for 23 min, and the density ratio (O/H) reached 15% for the HEP‐LD energy range (in the same plasmoid, this ratio was approximately 1% before the oxygen burst). The oxygen burst exhibited a strong beam‐like structure which occupied only 6 ∼ 7% of the full solid angle (4π). We suggest that energized oxygen ions of ionospheric origin travel downtail in the narrow postplasmoid‐plasma sheet which trails the plasmoid. Furthermore, we suggest that the magnetosphere dissipated larger quantities of energy during this very intense substorm event by ejecting multiple relatively small plasmoids rather than through the formation and ejection of a single large plasmoid.