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Nighttime meridional neutral wind responses to SAPS simulated by the TIEGCM: A universal time effect

KeDeng Zhang Hui Wang WenBin Wang Jing Liu ShunRong Zhang Cheng Sheng

地球与行星物理(英文)2021,Vol.5Issue(1):52-62,11.
地球与行星物理(英文)2021,Vol.5Issue(1):52-62,11.DOI:10.26464/epp2021004

Nighttime meridional neutral wind responses to SAPS simulated by the TIEGCM: A universal time effect

Nighttime meridional neutral wind responses to SAPS simulated by the TIEGCM: A universal time effect

KeDeng Zhang 1Hui Wang 1WenBin Wang 2Jing Liu 2ShunRong Zhang 3Cheng Sheng4

作者信息

  • 1. Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan 430072, China
  • 2. High Altitude Observatory, National Center for Atmospheric Research, Boulder 80301, Colorado, USA
  • 3. Haystack Observatory, Massachusetts Institute of Technology, Westford 01886, Massachusetts, USA
  • 4. Department of Physics, University of Texas at Arlington, Arlington 76013, Texas, USA
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摘要

关键词

Subauroral Polarization Streams/TIEGCM/poleward winds/Universal time changes

Key words

Subauroral Polarization Streams/TIEGCM/poleward winds/Universal time changes

引用本文复制引用

KeDeng Zhang,Hui Wang,WenBin Wang,Jing Liu,ShunRong Zhang,Cheng Sheng..Nighttime meridional neutral wind responses to SAPS simulated by the TIEGCM: A universal time effect[J].地球与行星物理(英文),2021,5(1):52-62,11.

基金项目

The DMSP observations are obtained from the Madrigal database (http://cedar.openmadrigal.org/index.html/). Madrigal database is sponsored by the US NSF through a cooperative agreement (AGS-1762141) with the MIT Haystack Observatory. The FPI winds are from the Madrigal database (Zhang SR et al., 2015). The simula-tion data are archived in NCAR supercomputer (https://www2. cisl.ucar.edu/resources/storage-and-file-systems/hpss). The Na-tional Center for Atmospheric Research is sponsored by the Na-tional Science Foundation. The work is supported by the National Nature Science Foundation of China (No.s 41974182, 41674153, 41521063, 41431073, 41521062 and 42004135). Research at MIT Haystack Observatory is sponsored by the US NSF award AGS-1762141 and the US AFOSR MURI award FA9559-16-1-0364. This work is also supported in part by the NSF grant AGS-1452309. The Spark Project at Wuhan University (2042020gf0024) also sponsors this work. (http://cedar.openmadrigal.org/index.html/)

地球与行星物理(英文)

OACSCDEI

2096-3955

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