[1] MILLWARD G H, RISHBETH H, FULLER-ROWELL T J. Ionospheric F2 layer seasonal and semi-annual variations [J]. J Geophys Res, 1996, 101: 5149-5156.[2] RISHBETH H, MENDILLO M. Patterns of F2-layer variability [J]. J Atmos Solar-Terr Phys, 2001, 63: 1661-1680.[3] MENDILLO M, RISHBETH H, ROBLE R G, et al. Modelling F2-layer seasonal trends and day-to-day variability driven by coupling with the lower atmosphere [J]. J Atmos Solar-Terr Phys, 2002, 64: 1911-1931.[4] RISHBETH H. How the thermospheric circulation affects the ionospheric F2-layer [J]. J Atmos Terr Phys, 1998, 35(12): 1385-1402.[5] RISHBETH H, MULLER--WODARG I C F. Why is there more ionosphere in January than in July? The annual asymmetry in the F2-layer [J]. Ann Geophys, 2006, 24: 3293-3311.[6] ZHANG S, COSTER A J, HOLT J M, et al. Ionospheric longitudinal variations at midlatitudes: Incoherent scatter radar observation at Millstone Hill [J]. Science China Technological Sciences, 2012, 55(5): 1153-1160.[7] LIU L B, WAN W X, CHEN Y D, et al. Solar activity effects of the ionosphere: A brief review [J]. Chinese Sci Bull, 2011, 56(7):477-487.[8] LIBO LIU, BIQIANG ZHAO, WEIXINGWAN, et al. Seasonal variations of the ionospheric electron densities retrieved from Constellation Observing System for Meteorology, Ionosphere, and Climate mission radio occultation measurements [J]. J Geophys Res, 2009, 114:A02302.[9] LEI J, LIU L, WAN W. Variations of electron density based on long-term incoherent scatter radar and ionosonde measurements over Millstone Hill [J]. Radio Sci, 2005, 40:RS2008.[10] 刘顺林. 南极中山站电离层F层特性 [J]. 博士论文, 2005, [11] 沈长寿, 资民筠, 王劲松等. 南极中山站电离层的极区特性 [J]. 地球物理学报, 2005, 48(1): 1-6.[12] 徐中华, 刘瑞源, 刘顺林等. 南极中山站电离层F2 层临界频率变化特征 [J]. 地球物理学报, 2006, 49(1): 1-8.[13] 甄卫民, 曹冲, 吴健. 南极长城站电离层异常的模拟计算和分析 [J]. 南极研究, 1994, 6(3): 33-37.[14] 刘瑞源, 杨惠根. 中国极区高空大气物理学观测研究进展 [J]. 极地研究, 2011, 23(4): 241-258.[15] K. G. RATOVSKY, A. V. OINATS, A. V. MEDVEDEV. Regular features of the polar ionosphere characteristics from Digisonde measurements over Norilsk [J]. Adv Space Res, 2011. [16] H. T. CAI, S. Y. MA, Y. FAN, et al. Climatological features of electron density in the polar ionosphere from long-term observations of EISCAT/ESR radar [J]. Ann Geophys, 2007, 25: 2561-2569.[17] ZHANG S-R, J. M. Holt, A. P. van Eyken, et al. Ionospheric local model and climatology from long-term databases of multiple incoherent scatter radars [J]. Geophysical Research Letters, 2005, 32: L20102.[18] REES M H. Auroral ionization and excitation by incident energetic electrons [J]. PlanetSpace Sci, 1963, 11: 1209-1218.[19] MAYER C, JAKOWSKI N. Enhanced E-layer ionization in the auroral zones observed by radio occultation measurements onboard CHAMP and Formosat-3/COSMIC [J]. Ann Geophys, 2009, 27: 1207-1212.[20] HAJJ G A. Ionospheric electron density profiles obtained with the Global Positioning System: Results from the GPS/MET experiment [J]. Radio Sci, 1998, 33: 175-190.[21] SCHREINER W S, SOKOLOVSKIY S V, ROCKEN C. Analysis and validation of GPS/MET radio occultation data in the ionosphere [J]. Radio Sci, 1999, 34(4): 949-966.[22] KULIKOV I, MANNUCCI A J, PI X, et al. Electron density retrieval from occulting GNSS signals using a gradient-aided inversion technique [J]. Adv Space Res, 2011, 47(2): 289-295.[23] LEI J, SYNDERGAARD S, BURNS A G. Comparison of COSMIC ionospheric measurements with groundbased observations and model predictions: Preliminary results [J]. J Geophys Res, 2007, 112: A07038. [24] FELDSTEIN Y I. On Morphology and Auroral and Magnetic Disturbances at High Latitudes [J]. Geomagn Aeron 1963, 3: 227-239.[25] HOLZWORTH R H, MENG C-I. Mathematical Representation of the Auroral Oval [J]. Geophys Res Lett, 1975, 2: 377-380.[26] 蔡红涛, 马淑英. 由非相干散射雷达数据重建极光沉降粒子能谱 [J]. 地球物理学报, 2007, 50(1): 10-17. |