Ionospheric Plasma Density Oscillation Related to EMIC Pc1 Waves

Hyangpyo Kim, Kazuo Shiokawa, Jaeheung Park, Yoshizumi Miyoshi, Yukinaga Miyashita, Claudia Stolle, Khan Hyuk Kim, Jürgen Matzka, Stephan Buchert, Tanja Fromm, Junga Hwang

Research output: Contribution to journalArticlepeer-review

10 Citations (Scopus)

Abstract

We report the first observation of plasma density oscillations coherent with magnetic Pc1 waves. Swarm satellites observed compressional Pc1 wave activity in the 0.5–3 Hz band, which was coherent with in situ plasma density oscillations. Around the Pc1 event location, the Antarctic Neumayer Station III (L ~ 4.2) recorded similar Pc1 events in the horizontal component while NOAA-15 observed isolated proton precipitations at energies above 30 keV. All these observations support that the compressional Pc1 waves at Swarm are oscillations converted from electromagnetic ion cyclotron (EMIC) waves coming from the magnetosphere. The magnetic field and plasma density oscillate in-phase. We compared the amplitudes of density and magnetic field oscillations normalized to background values and found that the density power is much larger than the magnetic field power. This difference cannot be explained by a simple magnetohydrodynamic (MHD) model, although steep horizontal/vertical gradients of background ionospheric density can partly reconcile the discrepancy.

Original languageEnglish
Article numbere2020GL089000
JournalGeophysical Research Letters
Volume47
Issue number15
DOIs
Publication statusPublished - 16 Aug 2020

Bibliographical note

Publisher Copyright:
©2020. American Geophysical Union. All Rights Reserved.

Keywords

  • EMIC Pc1 wave
  • ULF wave
  • compressional mode
  • plasma density oscillation
  • proton precipitation
  • swarm satellite

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