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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/987654321/103128


    題名: Effects of ionizing energetic electrons and plasma transport in the ionosphere during the initial phase of the December 2006 magnetic storm
    作者: 蘇亞拉;Suvorova, A. V.;Huang, C.‐M.;Dmitriev, A. V.;Kunitsyn, V. E.;Andreeva, E. S.;Nesterov, I. A.;Klimenko, M. V.;Klimenko, V. V.;Tumanova, Yu. S.
    貢獻者: 全球大氣觀測與資料應用研究中心
    關鍵詞: direct ionization impact;Electrons;Fluxes;Geomagnetic storms;Geomagnetism;Global positioning systems;GPS;Interplanetary magnetic field;Ionosphere;Ionospheric electron content;ionospheric modeling;Ionospheric models;Ionospheric storms;Ionospherics;Jupiter;Latitude;Magnetic fields;Magnetic storms;Magnetism;Mathematical models;POES satellites;positive ionospheric storm;precipitating and quasi‐trapped electrons;radio tomography;Satellite observation;Storms;Thermosphere;Total Electron Content;Transport
    日期: 2016-06-01
    上傳時間: 2026-04-23 11:23:57 (UTC+8)
    出版者: Wiley-Blackwell;Washington: Blackwell Publishing Ltd
    摘要: 摘要: The initial phase of a major geomagnetic storm on 14 December 2006 was selected in order to investigate the ionizing effect of energetic electrons in the ionosphere. The global network of GPS receivers was used to analyze the total electron content (TEC). A strong positive ionospheric storm of ~20 TEC units (TECU) with ~6 h duration was observed on the dayside during the interval of northward interplanetary magnetic field. At the same time, the NOAA/POES satellites observed long‐lasting intense fluxes of >30 keV electrons in the topside ionosphere at middle and low latitudes, including a near‐equatorial forbidden zone outside of the South Atlantic Anomaly (SAA). We found that the TEC increases overlapped well with the enhancements of energetic electrons. Modeling of the ionospheric response by using a Global Self‐consistent Model of the Thermosphere, Ionosphere, and Protonosphere, based on the standard mechanisms of plasma transport, could only partially explain the ionospheric response and was unable to predict the long‐duration increase of TEC. For the energetic electrons, we estimated the ionizing effect of ~45 TECU and ~23 TECU in the topside ionosphere, respectively, inside and outside of SAA. The ionizing effect contributed from 50% to 100% of TEC increases and provided the long duration and wide latitudinal extension of the positive ionospheric storm. This finding is a very important argument in supporting significant ionizing effect of energetic electrons in the storm time ionosphere both at middle and low latitudes. Key Points TEC increases in the low‐ and middle‐latitude ionosphere at the initial storm phase Greater than 30 keV electron fluxes enhance significantly at the initial storm phase Energetic electron enhancements produce significant ionizing effect in the ionosphere
    出版者: Washington: Blackwell Publishing Ltd
    出版日期: 2016-06
    出處: Journal of geophysical research : Space physics (2013 - Present), 2016-06, Vol.121 (6), p.5880-5896
    資源來源: Wiley Online Library journals
    版權: 2016. American Geophysical Union. All Rights Reserved.
    識別號: ISSN: 2169-9380
    識別號: ISSN: 2169-9402
    識別號: EISSN: 2169-9402
    識別號: DOI: 10.1002/2016JA022622
    顯示於類別:[全球大氣觀測與資料應用研究中心] 期刊論文

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