Formation and evolution of the ionospheric plasma density shoulder and its relationship to the superfountain effects investigated during the 6 November 2001 great storm
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[1] I. McCrea,et al. Relative effects of electric field and neutral wind on positive ionospheric storms , 2009 .
[2] R. Roble,et al. A dayside ionospheric positive storm phase driven by neutral winds , 2008 .
[3] A. Mannucci,et al. Prompt penetration electric fields (PPEFs) and their ionospheric effects during the great magnetic storm of 30-31 October 2003 , 2008 .
[4] Y. Otsuka,et al. F3 layer during penetration electric field , 2008 .
[5] B. Tsurutani,et al. Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23 , 2008 .
[6] A. Mannucci,et al. Oxygen ion uplift and satellite drag effects during the 30 October 2003 daytime superfountain event , 2007 .
[7] I. Horvath. A total electron content space weather study of the nighttime weddell sea Anomaly of 1996/1997 southern summer with TOPEX/Poseidon radar altimetry , 2006 .
[8] T. Iyemori,et al. Equatorial electrojet as a diagnostic tool of geomagnetic field models , 2006 .
[9] M. K. Ramamurthy,et al. A new generation of cyberinfrastructure and data services for earth system science education and research , 2006 .
[10] Jann‐Yenq Liu,et al. Theoretical study of the low- and midlatitude ionospheric electron density enhancement during the October 2003 superstorm: Relative importance of the neutral wind and the electric field , 2005 .
[11] M. A. Abdu,et al. South Atlantic magnetic anomaly ionization: A review and a new focus on electrodynamic effects in the equatorial ionosphere , 2005 .
[12] R. W. Spiro,et al. Simulation study of penetration electric field effects on the low‐ to mid‐latitude ionosphere , 2005 .
[13] V. Vasyliūnas. Relation between magnetic fields and electric currents in plasmas , 2005 .
[14] R. Schunk,et al. On the sensitivity of total electron content (TEC) to upper atmospheric/ionospheric parameters , 2005 .
[15] V. Vasyliūnas. Time evolution of electric fields and currents and the generalized Ohm's law , 2005 .
[16] A. Komjathy,et al. Dayside global ionospheric response to the major interplanetary events of October 29–30, 2003 “Halloween Storms” , 2005 .
[17] A. Mannucci,et al. The October 28, 2003 extreme EUV solar flare and resultant extreme ionospheric effects: Comparison to other Halloween events and the Bastille Day event , 2005 .
[18] Toshitaka Tsuda,et al. Global dayside ionospheric uplift and enhancement associated with interplanetary electric fields , 2004 .
[19] Bruce T. Tsurutani,et al. The extreme magnetic storm of 1–2 September 1859 , 2003 .
[20] E. Essex,et al. The Weddell sea anomaly observed with the Topex satellite data , 2003 .
[21] V. Vasyliūnas. Electric field and plasma flow: What drives what? , 2001 .
[22] S. Watanabe,et al. Variability of an additional layer in the equatorial ionosphere over Fortaleza , 2000 .
[23] R. Heelis,et al. Analysis of the ionospheric cross polar cap potentialdrop and electrostatic potential distribution patternsduring the January 1997 cme event using DMSP data , 1999 .
[24] I. Batista,et al. Physical mechanism and statistics of occurrence of an additional layer in the equatorial ionosphere , 1998 .
[25] G. J. Bailey,et al. The Sheffield University plasmasphere ionosphere model--a review , 1997 .
[26] P. Richards,et al. Equatorial plasma fountain and its effects over three locations: Evidence for an additional layer, the F 3 layer , 1997 .
[27] J. Titheridge. Winds in the ionosphere - a review. , 1995 .
[28] G. J. Bailey,et al. Equatorial plasma fountain and its effects-possibility of an additional layer , 1995 .
[29] David A. Imel,et al. Evaluation of the TOPEX/POSEIDON dual-frequency ionosphere correction , 1994 .
[30] H. W. Kroehl,et al. What is a geomagnetic storm , 1994 .
[31] D. Crain,et al. Effects of electrical coupling on equatorial ionospheric plasma motions: When is the F region a dominant driver in the low-latitude dynamo? , 1993 .
[32] B. Tsurutani,et al. Great magnetic storms , 1992 .
[33] M. Clilverd,et al. The annual variation in quiet time plasmaspheric electron density, determined from whistler mode group delays , 1991 .
[34] John A. Klobuchar,et al. Ionospheric electron content within the equatorial F2 layer anomaly belt , 1990 .
[35] R. Schunk,et al. A comparison of foF2 obtained from a time-dependent ionospheric model with Argentine Islands' data for quiet conditions , 1988 .
[36] R. A. Mewaldt,et al. The Advanced Composition Explorer , 1988 .
[37] Arthur D. Richmond,et al. The ionospheric disturbance dynamo , 1980 .
[38] J. Titheridge. Plasma temperatures from alouette 1 electron density profiles , 1976 .
[39] R. J. Moffett,et al. lonization transport effects in the equatorial F region , 1966 .
[40] G. J. Bailey,et al. Response of the ionosphere to super geomagnetic storms: Observations and modeling , 2008 .
[41] A. Mannucci,et al. The extreme Halloween 2003 solar flares (and Bastille Day, 2000 Flare), ICMEs, and resultant extreme ionospheric effects: A review , 2006 .
[42] S. Kuznetsov,et al. Dynamics of the Earth’s radiation belts during the magnetic storm of November 6th, 2001 , 2005 .
[43] B. M. Pathan,et al. Response of the low latitude geomagnetic field to the major proton event of November 2001 , 2005 .
[44] B. Tsurutani,et al. Interplanetary phenomena associated with very intense geomagnetic storms , 2002 .
[45] L. Scherliess,et al. On the variability of equatorial F-region vertical plasma drifts , 2001 .