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首页> 外文期刊>Advances in space research >Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occupation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia
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Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occupation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

机译:从COSMIC无线电占领中获得的电离层F2层临界频率:与东南亚子午离子探空仪链测量值的统计比较

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摘要

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.
机译:在本文中,我们比较了从2008-2015年清迈,春蓬和科托邦的FORMOSAT-3 / COSMIC无线电掩星(RO)和离子探空仪得出的F2层临界频率(foF2),以评估COSMIC RO在东南亚地区。结果表明,从COSMIC RO得到的foF2值的时间发展总体上与离子探空仪测量的一致。但是,从COSMIC RO导出的foF2与从离子探空仪观测到的foF2之间的差异显示了纬度依赖性。 COSMIC RO倾向于低估清迈和Kototabang的foF2,这两个区域分别靠近北部EIA峰和南部,而Chumphon的foF2则高估了一些,它靠近地磁赤道。 COSMIC RO在春蓬的ionosonde观点最好,在清迈的观点最差。在每个离子探空仪站,随着太阳活动的增加,COSMIC RO数据的质量会下降。此外,在清迈和科托邦车站,COSMIC RO在夏季的表现要好于春分和冬季。此外,源自COSMIC RO的foF2的差异和来自离子探空仪测量的foF2的差异会随当地时间而变化,即当赤道电离异常(EIA)得到充分发展时,foF2的差异通常在夜间较小,在中午较大。

著录项

  • 来源
    《Advances in space research 》 |2019年第1期| 327-336| 共10页
  • 作者单位

    School of Geodesy and Geomatics, Wuhan University|Key Laboratory of Geospace Environment and Geodesy, Ministry of Education;

    School of Geodesy and Geomatics, Wuhan University;

    School of Geodesy and Geomatics, Wuhan University|Collaborative Innovation Center for Geospatial Technology;

    School of Geodesy and Geomatics, Wuhan University;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    F2-Layer critical frequency; COSMIC; Radio occultation; Ionosonde;

    机译:F2-层临界频率;COSMIC;无线电掩星;离子探空仪;

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