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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/987654321/102129


    題名: Coordinated observations of F region 3 m field-aligned plasma irregularities associated with medium-scale traveling ionospheric disturbances
    作者: 朱延祥;Lin, F F;Wang, C Y;Su, C L;Shiokawa, K;Saito, S;Chu, Y H
    貢獻者: 太空科學與科技研究中心
    關鍵詞: Airglow;Correlation;Depletion;Drift;Echo surveys;F region;Instability;Interferometry;Ionospheric disturbances;Irregularities;Measuring instruments;Plasma;Radar;Radar echoes;Traveling ionospheric disturbances
    日期: 2016-04-01
    上傳時間: 2026-04-23 11:03:19 (UTC+8)
    出版者: Wiley-Blackwell;Washington: Blackwell Publishing Ltd
    摘要: 摘要: Three meter field-aligned irregularities (3m FAIs) associated with medium-scale traveling ionospheric disturbances (MSTIDs) that occurred on 5 February 2008 were observed by using the Chung-Li 52MHz coherent scatter radar. Interferometry measurements show that the plasma structures responsible for the 3m FAI echoes are in a clumpy shape with a horizontal dimension of about 10-78km in a height range of 220-300km. In order to investigate the dynamic behaviors of the plasma irregularities at different scales in the bottomside of F region, the VHF radar echo structures from the 3m FAIs combined with the 630nm airglow images provided by the Yonaguni all-sky imager are compared and analyzed. The results show that the radar echoes were located at the west edge of the depletion zones of the 630nm airglow image of the MSTIDs. The bulk echo structures of the 3m FAIs drifted eastward at a mean trace velocity of about 30m/s that is in general agreement with the zonal trace velocity of the MSTIDs shown in the 630nm airglow images. These results suggest that the observed F region 3m FAIs for the present case can be regarded as the targets that are frozen in the local region of the MSTIDs. In addition, the radar-observed 3m FAI echo intensity and spectral width bear high correlations to the percentage variations of the 630nm emission intensity. These results seem to suggest that through the nonlinear turbulence cascade process, the MSTID-associated 3m FAIs are very likely generated from the kilometer-scale plasma irregularities with large amplitude excited by the gradient drift instability. Key Points Eastward drifting MSTID was observed at low latitude during nighttime Three meter FAIs occurred at west boundary of depletion region of MSTID Gradient drift instability is believed to be responsible for the generation of 3m FAIs
    出版者: Washington: Blackwell Publishing Ltd
    出版日期: 2016-04-01
    出處: Journal of geophysical research : Space physics (2013 - Present), 2016-04, Vol.121 (4), p.3750-3766
    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: EISSN: 2169-9402
    識別號: DOI: 10.1002/2016JA022511
    顯示於類別:[太空科學與科技研究中心] 期刊論文

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