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首页|期刊导航|地球与行星物理(英文)|Relationships between ionospheric parameters derived from ionosonde observations and characteristics of post-sunset GHz scintillation during high solar activities(2012-2013)at Sanya(18.3°N,109.6°E),China

Relationships between ionospheric parameters derived from ionosonde observations and characteristics of post-sunset GHz scintillation during high solar activities(2012-2013)at Sanya(18.3°N,109.6°E),China

JunJie Luo Ying Xiong WeiHua Luo ZhengPing Zhu ChaoWan Fan

地球与行星物理(英文)2023,Vol.7Issue(3):389-406,18.
地球与行星物理(英文)2023,Vol.7Issue(3):389-406,18.DOI:10.26464/epp2023038

Relationships between ionospheric parameters derived from ionosonde observations and characteristics of post-sunset GHz scintillation during high solar activities(2012-2013)at Sanya(18.3°N,109.6°E),China

Relationships between ionospheric parameters derived from ionosonde observations and characteristics of post-sunset GHz scintillation during high solar activities(2012-2013)at Sanya(18.3°N,109.6°E),China

JunJie Luo 1Ying Xiong 1WeiHua Luo 2ZhengPing Zhu 3ChaoWan Fan1

作者信息

  • 1. College of Electronic and Information Engineering,South-Central Minzu University,430074 Wuhan,China
  • 2. College of Electronic and Information Engineering,South-Central Minzu University,430074 Wuhan,China||Hubei Key Laboratory of Intelligent Wireless Communications,South-Central Minzu University,430074 Wuhan,China
  • 3. College of Electronic and Information Engineering,South-Central Minzu University,430074 Wuhan,China||Hubei Key Laboratory of Intelligent Wireless Communications,South-Central Minzu University,430074 Wuhan,China||Hubei Engineering Research Center of Intelligent Internet of Things Technology,South-Central Minzu University,430074 Wuhan,China
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摘要

关键词

equatorial ionosphere/scintillation/low latitude/iononsonde/equinoctial asymmetry

Key words

equatorial ionosphere/scintillation/low latitude/iononsonde/equinoctial asymmetry

引用本文复制引用

JunJie Luo,Ying Xiong,WeiHua Luo,ZhengPing Zhu,ChaoWan Fan..Relationships between ionospheric parameters derived from ionosonde observations and characteristics of post-sunset GHz scintillation during high solar activities(2012-2013)at Sanya(18.3°N,109.6°E),China[J].地球与行星物理(英文),2023,7(3):389-406,18.

基金项目

This work is supported by the Fundamental Research Funds for the Central Universities,South-Central MinZu University(Grant Number:CPT22019).We acknowledge use of ionosonde and GNSS scintillation data from the Institute of Geology and Geophysics,Chinese Academy of Sciences.The scintillation and ionosonde data were provided by Beijing National Observatory of Space Environment,Institute of Geology and Geophysics,Chinese Academy of Sciences through the Data Center for Geophysics,National Earth System Science Data Sharing Infrastructure(http://wdc.geophys.ac.cn/).The sunspot number,F10.7 and ap data were downloaded from the National Geophysical Data Center(ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/).The ROCS AT-1 data can be downloaded from the website(https://cdaweb.gsfc.nasa.gov/index.html/). (Grant Number:CPT22019)

地球与行星物理(英文)

OACSCDEI

2096-3955

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