Woodman R F. Spread F-an old equatorial aeronomy problem finally resolved? Ann. Geophys., 2009, 27(5): 1915-1934.
[2]
Kelley M C. The Earth''s Ionosphere: Plasma Physics and Electrodynamics (2nd ed). London: Elsevier, 2009.
[3]
Basu B. On the linear theory of equatorial plasma instability: Comparison of different descriptions. J. Geophys. Res., 2002, 107(A8): 1199, doi: 10.1029/2001JA000317.
[4]
Anderson D N, Reinisch B, Valladare C, et al. Forecasting the occurrence of ionospheric scintillation activity in the equatorial ionosphere on a day-to-day basis. J. Atmos. Sol-Terr. Phys., 2004, 66(17): 1567-1572.
[5]
罗伟华, 徐继生, 田茂.通量管积分瑞利-泰勒不稳定性的半球不对称和随经度变化的研究. 地球物理学报, 2012,55(4): 1078-1087. Luo W H, Xu J S, Tian M. Investigation of hemispheric asymmetry and longitudinal variation of flux-tube integrated Rayleigh-Taylor instability. Chinese J. Geophys. (in Chinese), 2012, 55(4): 1078-1087.
[6]
罗伟华, 徐继生, 徐良. 赤道电离层R-T不稳定性发展的控制因素分析. 地球物理学报, 2009, 52(4): 849-858. Luo W H, Xu J S, Xu L. Analysis of controlling factors leading to the development of R-T instability in equatorial ionosphere. Chinese J. Geophys. (in Chinese), 2009, 52(4): 849-858.
[7]
Bilitza D. International reference ionosphere 2000. Radio Science, 2001, 36(2): 261-275.
[8]
熊波, 万卫星, 宁百齐等. 海南三亚地区S4指数与C/N、ROTI的比较分析. 地球物理学报, 2007, 50(6): 1639-1648. Xiong B, Wan W X, Ning B Q, et al. A comparison and analysis of the S4 index, C/N and ROTI over Sanya. Chinese J. Geophys. (in Chinese), 2007, 50(6): 1639-1648.
[9]
Huang C Y, Burke W J, Machuzak J S, et al. Equatorial plasma bubbles observed by DMSP satellites during a full solar cycle: Toward a global climatology. J. Geophys. Res., 2002, 107(A12): SIA7-1-SIA7-10, doi: 10.1029/2002JA009452.
[10]
Burke W J, Gentile L C, Huang C Y, et al. Longitudinal variability of equatorial plasma bubbles observed by DMSP and ROCSAT-1. J. Geophys. Res., 2004, 109(A12): A12301, doi: 10.1029/2004JA010583.
[11]
Gentile L C, Burke W J, Rich F J. A climatology of equatorial plasma bubbles from DMSP 1989—2004. Radio Science, 2006, 41(5): RS5S21, doi: 10.1029/2005RS003340.
[12]
Su S Y, Chao C K, Liu C H. On monthly/seasonal/longitudinal variations of equatorial irregularity occurrences and their relationship with the postsunset vertical drift velocities. J. Geophys. Res., 2008, 113(A5): A05307, doi: 10.1029/2007JA012809.
[13]
Liu L B, Wan W X, Chen Y D, et al. Solar activity effects of the ionosphere: A brief review. Chinese Science Bulletin, 2011, 56(12): 1202-1211, doi: 10.1007/s11434-010-4226-9.
[14]
Fejer B G, Paula E R, Gonzalez S A, et al. Average vertical and zonal F region plasma drifts over Jicamarca. J. Geophys. Res., 1991, 96(A8): 13901-13906.
[15]
Fejer B G, Jensen J W, Su S Y. Quiet time equatorial F region vertical plasma drift model derived from ROCSAT-1 observations. J. Geophys. Res., 2008, 113(A5): A05304, doi: 10.1029/2007JA012801.
[16]
Niranjan K, Brahmanandam P S, Rao P R, et al. Post midnight spread-F occurrence over Waltair (17.7°N, 83.3°E) during low and ascending phases of solar activity. Ann. Geophys., 2003, 21: 745-750.
[17]
Burke W J, de La Beaujardière O, Gentile L C, et al. C/NOFS observations of plasma density and electric field irregularities at post-midnight local times. Geophys. Res. Lett., 2009, 36(18): L00C09, doi: 10.1029/2009GL038879.
[18]
Li G Z, Ning B Q, Abdu M A, et al. On the occurrence of postmidnight equatorial F region irregularities during the June solstice. J. Geophys. Res., 2011, 116(A4): A04318, doi: 10.1029/2010JA016056.
[19]
Retterer J M, Decker D T, Borer W S, et al. Assimilative modeling of the equatorial ionosphere for scintillation forecasting: Modeling with vertical drifts. J. Geophys. Res., 2005, 110(A11): A11307, doi: 10.1029/2002JA009613.
[20]
Retterer J M. Physics-based forecasts of equatorial radio scintillation for the communication and navigation outage forecasting system (C/NOFS). Space Weather, 2005, 3(12): S12C03, doi: 10.1029/2005SW000146.
[21]
Kelley M C, Retterer J. First successful prediction of a convective equatorial ionospheric storm using solar wind parameters. Space Weather, 2008, 6(8): S08003, doi: 10.1029/2007SW000381.
[22]
Singh S B, Patel K, Patel R P, et al. Modeling of VHF scintillation observed at low latitude. J. Physics: Conf. Ser., 2010, 208(1): 012065, doi: 10.1088/1742-6596/208/1/012065.
[23]
Drob D P, Emmert J T, Crowley G, et al. An empirical model of the Earth''s horizontal wind fields: HWM07. J. Geophys. Res., 2008, 113(A12): A12304, doi: 10.1029/2008JA013668.
[24]
Picone J M, Hedin A W, Drob D P, et al. NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues. J. Geophys. Res., 2002, 107(A12): 1468, doi: 10.1029/2002JA009430.
[25]
Adewale A O, Oyeyemi E O, Adeloye A B, et al. A study of L-band scintillations and total electron content at an equatorial station, Lagos, Nigeria. Radio Science, 2012, 47: RS2011, doi: 10.1029/2011RS004846.
[26]
徐继生, 朱洁, 李莉等. 武汉与桂林L-波段电波闪烁与TEC起伏特征比较. 电波科学学报, 2007, 22(2): 181-186. Xu J S, Zhu J, Li L, et al. Comparison of L-band radio wave scintillations and TEC fluctuations from observation of Wuhan and Guilin. Chinese J. Radio Sci. (in Chinese), 2007, 22(2): 181-186.
[27]
胡连欢, 宁百齐, 李国主. 海南地区电离层闪烁观测与GISM模式预测的比较分析. 空间科学学报, 2007, 27(5): 384-390. Hu L H, Ning B Q, Li G Z. Comparison between GISM predictions and ionospheric scintillation measurements over Hainan region. Chin. J. Space Sci. (in Chinese), 2007, 27(5): 384-390.
[28]
Dandekar B S, Groves K M. Using ionospheric scintillation observations for studying the morphology of equatorial ionospheric bubbles. Radio Science, 2004, 39(3): RS3010, doi: 10.1029/2003RS003020.
[29]
Aarons J. The longitudinal morphology of equatorial F-layer irregularities relevant to their occurrence. Space Sci. Rev., 1993, 63(3-4): 209-243.
[30]
Joshi L M, Patra A K, Rao S V B. Equatorial F-region irregularities during low and high solar activity conditions. Ind. J. Radio Space Phys., 2012, 41(2): 208-219.
[31]
Abdu M A. Equatorial spread F development and quiet time variability under solar minimum conditions. Ind. J. Radio Space Phys., 2012, 41(2): 168-193.