Global simulation study for the time sequence of events leading to the substorm onset

T. Tanaka, Y. Ebihara, M. Watanabe, M. Den, S. Fujita, T. Kikuchi, K. K. Hashimoto, R. Kataoka

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

We have developed a global simulation code which gives numerical solutions having an extremely high resolution. The substorm solution obtained from this simulation code reproduces the precise features of the substorm onset in the ionosphere. It can reproduce the onset that starts from the equatorward side of the quiet arc, two step development of the onset, and the westward traveling surge (WTS) that starts 2 min after the initial brightening. Then, we investigated the counter structures in the magnetosphere that correspond to each event in the ionosphere. The structure in the magnetosphere promoting the onset is the near-Earth dynamo in the inner magnetospheric region away from the equatorial plane. The near-Earth dynamo is driven by the field-aligned pressure increase due to the parallel flow associated with the squeezing, combined with equatorward field-perpendicular flow induced by the near-Earth neutral line (NENL). The dipolarization front is launched from the NENL associated with the convection transient from the growth phase to the expansion phase, but neither the launch nor the arrival of the dipolarization front coincides with the onset timing. The arrival of flow to the equatorial plane of the inner magnetosphere occurs 2 min after the onset, when the WTS starts to develop toward the west. The expansion phase is further developed by this flow. Looking at the present result that the onset sequence induced by the near-Earth dynamo reproduces the details of observation quite well, we cannot avoid to conclude that the current wedge is a misleading concept.

Original languageEnglish
Pages (from-to)6210-6239
Number of pages30
JournalJournal of Geophysical Research: Space Physics
Volume122
Issue number6
DOIs
Publication statusPublished - Jun 1 2017

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Magnetosphere
Earth (planet)
magnetospheres
magnetosphere
Ionosphere
simulation
ionospheres
arrivals
ionosphere
parallel flow
Parallel flow
expansion
pressure field
compressing
wedges
flow field
Flow fields
flow distribution
counters
convection

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Cite this

Global simulation study for the time sequence of events leading to the substorm onset. / Tanaka, T.; Ebihara, Y.; Watanabe, M.; Den, M.; Fujita, S.; Kikuchi, T.; Hashimoto, K. K.; Kataoka, R.

In: Journal of Geophysical Research: Space Physics, Vol. 122, No. 6, 01.06.2017, p. 6210-6239.

Research output: Contribution to journalArticle

Tanaka, T, Ebihara, Y, Watanabe, M, Den, M, Fujita, S, Kikuchi, T, Hashimoto, KK & Kataoka, R 2017, 'Global simulation study for the time sequence of events leading to the substorm onset', Journal of Geophysical Research: Space Physics, vol. 122, no. 6, pp. 6210-6239. https://doi.org/10.1002/2017JA024102
Tanaka, T. ; Ebihara, Y. ; Watanabe, M. ; Den, M. ; Fujita, S. ; Kikuchi, T. ; Hashimoto, K. K. ; Kataoka, R. / Global simulation study for the time sequence of events leading to the substorm onset. In: Journal of Geophysical Research: Space Physics. 2017 ; Vol. 122, No. 6. pp. 6210-6239.
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