Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations

Yukitoshi Nishimura, Takashi Kikuchi, Yusuke Ebihara, Akimasa Yoshikawa, Shun Imajo, Wen Li, Hisashi Utada

Research output: Contribution to journalArticle

6 Citations (Scopus)

Abstract

We investigated evolution of ionospheric currents during sudden commencements using a ground magnetometer network in conjunction with an all-sky imager, which has the advantage of locating field-aligned currents much more accurately than ground magnetometers. Preliminary (PI) and main (MI) impulse currents showed two-cell patterns propagating antisunward, particularly during a southward interplanetary magnetic field (IMF). Although this overall pattern is consistent with the Araki (solar wind sources of magnetospheric ultra-low-frequency waves. Geophysical monograph series, vol 81. AGU, Washington, DC, pp 183-200, 1994. doi:10.1029/GM081p0183) model, we found several interesting features. The PI and MI currents in some events were highly asymmetric with respect to the noon- midnight meridian; the post-noon sector did not show any notable PI signal, but only had an MI starting earlier than the pre-noon MI. Not only equivalent currents but also aurora and equatorial magnetometer data supported the much weaker PI response. We suggest that interplanetary shocks impacting away from the subsolar point caused the asymmetric current pattern. Additionally, even when PI currents form in both pre- and post-noon sectors, they can initiate and disappear at different timings. The PI currents did not immediately disappear but coexisted with the MI currents for the first few minutes of the MI. During a southward IMF, the MI currents formed equatorward of a preexisting DP-2, indicating that the MI currents are a separate structure from a preexisting DP-2. In contrast, the MI currents under a northward IMF were essentially an intensification of a preexisting DP-2. The magnetometer and imager combination has been shown to be a powerful means for tracing evolution of ionospheric currents, and we showed various types of ionospheric responses under different upstream conditions.

Original languageEnglish
Article number144
Journalearth, planets and space
Volume68
Issue number1
DOIs
Publication statusPublished - Dec 1 2016

Fingerprint

wind pressure
pressure pulses
aurora
magnetometer
magnetometers
solar wind
noon
interplanetary magnetic fields
ionospheric currents
magnetic field
sectors
interplanetary shock waves
extremely low frequencies
field aligned currents
tracing
upstream
ionospherics
sky
impulses
time measurement

All Science Journal Classification (ASJC) codes

  • Geology
  • Space and Planetary Science

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Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations. / Nishimura, Yukitoshi; Kikuchi, Takashi; Ebihara, Yusuke; Yoshikawa, Akimasa; Imajo, Shun; Li, Wen; Utada, Hisashi.

In: earth, planets and space, Vol. 68, No. 1, 144, 01.12.2016.

Research output: Contribution to journalArticle

Nishimura, Yukitoshi ; Kikuchi, Takashi ; Ebihara, Yusuke ; Yoshikawa, Akimasa ; Imajo, Shun ; Li, Wen ; Utada, Hisashi. / Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations. In: earth, planets and space. 2016 ; Vol. 68, No. 1.
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