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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/102278


    題名: Occurrence probability and amplitude of equatorial ionospheric irregularities associated with plasma bubbles during low and moderate solar activities (2008-2012)
    作者: 劉正彥;Huang, Chao-Song;de La Beaujardiere, O.;Roddy, P. A.;Hunton, D. E.;Liu, J. Y.;Chen, S. P.
    貢獻者: 地球科學學院太空科學與工程學系
    關鍵詞: equatorial ionosphere;Ionosphere;ionospheric irregularities;occurrence probability;Plasma;plasma bubbles;Probability;scintillation;Solar activity;Solar physics;Statistical analysis
    日期: 2014-02-01
    上傳時間: 2026-04-23 11:05:29 (UTC+8)
    出版者: Wiley-Blackwell;Washington: Blackwell Publishing Ltd
    摘要: 摘要: We present a statistical analysis of the occurrence probability of equatorial spread F irregularities measured by the Communication/Navigation Outage Forecasting System satellite during 2008–2012. We use different criteria (plasma density perturbations, ΔN, and relative density perturbations, ∆N/N0) to identify the occurrence of ionospheric irregularities. The purpose of this study is to determine whether the occurrence probability of irregularities is the same for different criteria, whether the patterns of irregularity occurrence vary with solar activity and with local time, and how the patterns of irregularity occurrence are correlated with ionospheric scintillation. It is found that the occurrence probability of irregularities and its variation with local time are significantly different when different identification criteria are used. The occurrence probability based on plasma density perturbations is high in the evening sector and becomes much lower after midnight. In contrast, the occurrence probability based on relative density perturbations is low in the evening sector but becomes very high after midnight in the June solstice. We have also compared the occurrence of ionospheric irregularities with scintillation. The occurrence pattern of the S4 index and its variation with local time are in good agreement with the irregularity occurrence based on plasma density perturbations but are significantly different from those based on relative density perturbations. This study reveals that the occurrence pattern of equatorial ionospheric irregularities varies with local time and that only the occurrence probability of irregularities based on plasma density perturbations is consistent with the occurrence of scintillation at all local times. Key Points New occurrence probability of equatorial irregularities is derived Dependence of the irregularity occurrence on local time is identified The occurrence of plasma irregularities is compared with scintillation
    其他題名: J. Geophys. Res. Space Physics
    出版者: Washington: Blackwell Publishing Ltd
    出版日期: 2014-02
    出處: Journal of geophysical research : Space physics (2013 - Present), 2014-02, Vol.119 (2), p.1186-1199
    資源來源: Wiley Online Library All Journals
    版權: 2014. American Geophysical Union. All Rights Reserved.
    識別號: ISSN: 2169-9380
    識別號: EISSN: 2169-9402
    識別號: DOI: 10.1002/2013JA019212
    顯示於類別:[太空科學與工程學系] 期刊論文

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