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首页|期刊导航|地球与行星物理(英文)|Coordinated observations on the spatiotemporal development of global-scale dipolarizations and their coupling to meso-scale dipolarizations

Coordinated observations on the spatiotemporal development of global-scale dipolarizations and their coupling to meso-scale dipolarizations

Sheng Tian J.M.Weygand J.Liu J.R.Wygant L.Lyons V.Angelopoulos J.Bortnik G.D.Reeves

地球与行星物理(英文)2026,Vol.10Issue(2):291-301,11.
地球与行星物理(英文)2026,Vol.10Issue(2):291-301,11.DOI:10.26464/epp2026021

Coordinated observations on the spatiotemporal development of global-scale dipolarizations and their coupling to meso-scale dipolarizations

Coordinated observations on the spatiotemporal development of global-scale dipolarizations and their coupling to meso-scale dipolarizations

Sheng Tian 1J.M.Weygand 2J.Liu 3J.R.Wygant 4L.Lyons 5V.Angelopoulos 2J.Bortnik 5G.D.Reeves6

作者信息

  • 1. School of Physics and Astronomy,University of Minnesota,Minneapolis,Minnesota,USA||Department of Atmospheric and Oceanic Sciences,University of California,Los Angeles,California,USA
  • 2. Institute of Geophysics and Planetary Physics,University of California,Los Angeles,California,USA
  • 3. Department of Atmospheric and Oceanic Sciences,University of California,Los Angeles,California,USA||Institute of Geophysics and Planetary Physics,University of California,Los Angeles,California,USA
  • 4. School of Physics and Astronomy,University of Minnesota,Minneapolis,Minnesota,USA
  • 5. Department of Atmospheric and Oceanic Sciences,University of California,Los Angeles,California,USA
  • 6. Los Alamos National Laboratory,Los Alamos,New Mexico,USA
  • 折叠

摘要

关键词

dipolarization/field-aligned current/magnetosphere-ionosphere coupling

Key words

dipolarization/field-aligned current/magnetosphere-ionosphere coupling

引用本文复制引用

Sheng Tian,J.M.Weygand,J.Liu,J.R.Wygant,L.Lyons,V.Angelopoulos,J.Bortnik,G.D.Reeves..Coordinated observations on the spatiotemporal development of global-scale dipolarizations and their coupling to meso-scale dipolarizations[J].地球与行星物理(英文),2026,10(2):291-301,11.

基金项目

We thank the following spacecraft missions and relevant instrument teams for providing the data used in this study,including the THEMIS all-sky imagers and ground magnetometers,the FGM(Fluxgate Magnetometer),EFI(Electric Field Instrument),and ESA(Electrostatic Analyzer)instruments onboard THEMIS (Fluxgate Magnetometer)

the magnetometer and particle instrument onboard GOES ()

the EMFISIS(Electric and Magnetic Field Instrument Suite and Integrated Science),EFW(Electric Field and Waves Suite),HOPE(Helium,Oxygen,Proton and Electron Mass Spectrometer),and MagEIS(Magnetic Electron Ion Spectrometer)instruments onboard RBSP (Electric and Magnetic Field Instrument Suite and Integrated Science)

the FGM instrument onboard MMS ()

and the particle instrument onboard LANL 1991-080.S.Tian acknowledges NASA(National Aeronautics and Space Administration)grant 81NSSC19K0306 and NASA prime contract NAS5-01072.J.Liu acknowledges AFOSR(Air Force Office of Scientific Research)grant FA9559-16-1-0364 (National Aeronautics and Space Administration)

NSF(National Science Foundation)grant AGS-2055192 (National Science Foundation)

NASA grants 80NSSC20K1314,80NSSC20K1316,and 80NSSC21K1407 ()

and NASA Contract NAS5-02099.J.M.Weygand acknowledges NASA grants:80NSSC18K1220 and 80NSSC18K0570,NASA contracts 80GSFC17C0018,and NAS5-02099.J.Bortnik acknowledges NASA award 80NSSC18K1227.S.Tian sincerely thanks M.K.Hudson,L.R.Lyons,A.Runov,and X.Chu for helpful suggestions related to this study. ()

地球与行星物理(英文)

2096-3955

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