Echer E, Gonzalez W D, Tsurutani B T. 2008. Interplanetary conditions leading to superintense geomagnetic storms (Dst≤-250 nT) during solar cycle 23. Geophysical Research Letters, 35(6): L06S03, doi: 10.1029/2007GL031755.
[2]
Echer E, Tsurutani B T, Gonzalez W D. 2013. Interplanetary origins of moderate (-100 nT
[3]
Jian L, Russell C T, Luhmann J G, et al. 2006b. Properties of stream interactions at one AU during 1995—2004. Solar Physics, 239(1-2): 337-392.
[4]
Jian L K, Russell C T, Luhmann J G. 2011. Comparing solar minimum 23/24 with historical solar wind records at 1 AU. Solar Physics, 274(1-2): 321-344.
[5]
Kilpua E K J, Luhmann J G, Jian L, et al. 2014. Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? Journal of Atmospheric and Solar-Terrestrial Physics, 107: 12-19, doi: 10.1016/j.jastp.2013.11.001.
[6]
Wang Y M, Wang B Y, Shen C L, et al. 2014. Deflected propagation of a coronal mass ejection from the corona to interplanetary space. Journal of Geophysical Research: Space Physics, 119(7): 5117-5132, doi: 10.1002/2013JA-19537.
[7]
Wang Y M, Wang S, Ye P Z. 2002a. Multiple magnetic clouds in interplanetary space. Solar Physics, 211(1-2): 333-344.
[8]
Wang Y M, Ye P Z, Wang S, et al. 2002b. A statistical study on the geoeffectiveness of Earth-directed coronal mass ejections from March 1997 to December 2000. Journal of Geophysical Research, 107(A11): SSH 2-1-SSH 2-9.
[9]
Wang Y M, Ye P Z, Wang S. 2003a. Multiple magnetic clouds: Several examples during March-April 2001. Journal of Geophysical Research, 108(A10): 1370, doi: 10.1029/2003JA009850.
[10]
Wang Y M, Ye P Z, Wang S, et al. 2003b. Theoretical analysis on the geoeffectiveness of a shock overtaking a preceding magnetic cloud. Solar Physics, 216(1-2): 295-310.
[11]
Wang Y M, Ye P Z, Wang S, et al. 2003c. An interplanetary cause of large geomagnetic storms: Fast forward shock overtaking preceding magnetic cloud. Geophysical Research Letters, 30(13): 31-33.
[12]
Gonzalez W D, Joselyn J A, Kamide Y, et al. 1994. What is a geomagnetic storm? Journal of Geophysical Research, 99(A4): 5771-5792.
[13]
Gonzalez W D, Tsurutani B T, Clúa de Gonzalez A L. 1999. Interplanetary origin of geomagnetic storms. Space Science Reviews, 88(3-4): 529-562.
[14]
Gonzalez W D, Echer E, Clúa Gonzalez A L, et al. 2007. Interplanetary origin of intense geomagnetic storms (Dst<-100 nT) during solar cycle 23. Geophysical Research Letters, 34(6): L06101, doi: 10.1029/2006GL028879.
[15]
Gonzalez W D, Echer E, Tsurutani B T, et al. 2011. Interplanetary origin of intense, superintense and extreme geomagnetic storms. Space Science Reviews, 158(1): 69-89.
[16]
Gopalswamy N, M？kel？ P, Xie H, et al. 2009. CME interactions with coronal holes and their interplanetary consequences. Journal of Geophysical Research, 114(A3): A00A22, doi: 10.1029/2008JA013686.
[17]
Gopalswamy N, Akiyama S, Yashiro S, et al. 2014. Anomalous expansion of coronal mass ejections during solar cycle 24 and its space weather implications. Geophysical Research Letters, 41(8): 2673-2680.
[18]
Jian L, Russell C T, Luhmann J G, et al. 2006a. Properties of interplanetary coronal mass ejections at one AU during 1995—2004. Solar Physics, 239(1-2): 393-436.
[19]
Li K J, Feng W, Liang H F. 2010. The abnormal 24th solar cycle-The first complete solar cycle of the new millennium. Scientia Sinica Phys., Mech. & Astron. (in Chinese), 40(10): 1293-1301.
[20]
Lugaz N, Farrugia C J. 2014. A new class of complex ejecta resulting from the interaction of two CMEs and its expected geoeffectiveness. Geophysical Research Letters, 41(3): 769-776.
[21]
Lugaz N, Manchester IV W B, Gombosi T I. 2005. Numerical simulation of the interaction of two coronal mass ejections from sun to earth. Astrophysical Journal, 634(1): 651-662.
[22]
Richardson I G. 2013. Geomagnetic activity during the rising phase of solar cycle 24. Journal of Space Weather and Space Climate, 3(A8), doi: 10.1051/swsc/2013031.
[23]
Shen C L, Wang Y M, Gui B, et al. 2011a. Kinematic evolution of a slow CME in corona viewed by STEREO-B on 8 October 2007. Solar Physics, 269(2): 389-400.
[24]
Shen C L, Wang Y M, Pan Z H, et al. 2013. Full halo coronal mass ejections: Do we need to correct the projection effect in terms of velocity? Journal of Geophysical Research: Space Physics, 118(11): 6858-6865, doi: 10.1002/2013JA018872.
[25]
Shen C L, Wang Y M, Pan Z H, et al. 2014. Full-halo coronal mass ejections: arrival at the earth. Journal of Geophysical Research: Space Physics, 119(7): 5107-5116, doi: 10.1002/2014JA020001.
[26]
Shen F, Feng X S, Wang Y M, et al. 2011b. Three-dimensional MHD simulation of two coronal mass ejections'' propagation and interaction using a successive magnetized plasma blobs model. Journal of Geophysical Research, 116(A9), doi: 10.1029/2011JA016584.
[27]
Wang Y M, Shen C L, Wang S, et al. 2004. Deflection of coronal mass ejection in the interplanetary medium. Solar Physics, 222(2): 329-343.
[28]
Xue X H, Wang Y M, Ye P Z, et al. 2005. Analysis on the interplanetary causes of the great magnetic storms in solar maximum (2000—2001). Planetary and Space Science, 53(4): 443-457.
[29]
Yu W, Farrugia C J, Lugaz N, et al. 2013. A statistical analysis of properties of small transients in the solar wind 2007—2009: STEREO and Wind observations. Journal of Geophysical Research: Space Physics, 119(2): 689-708, doi: 10.1002/2013JA019115.
[30]
Zhang J, Dere K P, Howard R A, et al. 2003. Identification of solar sources of major geomagnetic storms between 1996 and 2000. Astrophysical Journal, 582(1): 520-533.
[31]
Zhang J, Richardson I G, Webb D F, et al. 2007a. Correction to "Solar and interplanetary sources of major geomagnetic storms (Dst≤-100 nT) during 1996—2005". Journal of Geophysical Research, 112(A12): A12103, doi: 10.1029/2007JA012891.
[32]
Zhang J, Richardson I G, Webb D F, et al. 2007b. Solar and interplanetary sources of major geomagnetic storms (Dst≤-100 nT) during 1996—2005. Journal of Geophysical Research, 112(A10): A10102, doi: 10.1029/2007JA012321.
