Formation of polar ionospheric tongue of ionization during minor geomagnetic disturbed conditions

被引:27
作者
Liu, Jing [1 ,2 ]
Nakamura, Takuji [3 ]
Liu, Libo [1 ]
Wang, Wenbin [2 ]
Balan, Nanan [3 ]
Nishiyama, Takanori [3 ]
Hairston, Marc R. [4 ]
Thomas, E. G. [5 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
[2] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[3] Natl Inst Polar Res, Tokyo, Japan
[4] Univ Texas Dallas, Ctr Space Sci, Richardson, TX 75083 USA
[5] Virginia Tech, Bradley Dept Elect & Comp Engn, Blacksburg, VA USA
基金
美国国家科学基金会; 中国国家自然科学基金; 中国博士后科学基金;
关键词
storm-enhanced density; tongue of ionization; TOTAL ELECTRON-CONTENT; STORM-ENHANCED DENSITY; TIME INCREASES; ION DRIFTS; LATITUDES; EQUATORIAL; NETWORK; RADAR; PHASE;
D O I
10.1002/2015JA021393
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Previous investigations of ionospheric storm-enhanced density (SED) and tongue of ionization (TOI) focused mostly on the behavior of TOI during intense geomagnetic storms. Little attention has been paid to the spatial and temporal variations of TOI during weak to moderate geomagnetic disturbed conditions. In this paper we investigate the source and development of TOI during a moderate geomagnetic storm on 14 October 2012. Multi-instrumental observations including GPS total electron content (TEC), Defense Meteorological Satellite Program (DMSP) in situ measured total ion concentration and ion drift velocity, SuperDARN measured polar ion convection patterns, and electron density profiles from the Poker Flat Incoherent Scatter Radar (PFISR) have been utilized in the current analysis. GPS TEC maps show salient TOI structures persisting for about 5h over high latitudes of North America on 14 October 2012 in the later recovery phase of the storm when the magnitudes of IMF By and Bz were less than 5nT. The PFISR electron density profiles indicate that the extra ionization for TEC enhancements mainly occurred in the topside ionosphere with no obvious changes in the bottomside ionosphere and vertical plasma drifts. Additionally, there were no signatures of penetration electric fields in the equatorial electrojet data and upward ion drifts at high latitudes. At the same time, strong subauroral polarization streams with ion drift speeds exceeding 2.5km/s carried sunward fluxes and migrated toward lower latitudes for about 5 degrees based on the DMSP cross-track drift measurements. Based on those measurements, we postulate that the combined effects of initial build-up of ionization at midlatitudes through daytime production of ionization and equatorward (or less poleward than normal daytime) neutral wind reducing downward diffusion along the inclined filed lines, and an expanded polar ion convection pattern and its associated horizontal plasma transport are important in the formation of the TOI.
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页码:6860 / 6873
页数:14
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