Analysis of the ionosphere/plasmasphere electron content variability during strong geomagnetic storm

被引:8
|
作者
Cherniak, Iu. V. [1 ,3 ]
Zakharenkova, I. E. [1 ,3 ]
Dzubanov, D. [2 ]
Krankowski, A. [3 ]
机构
[1] W Dept IZMIRAN, Kaliningrad 23601, Russia
[2] MES Ukraine, Inst Ionosphere NAS, Kharkov, Ukraine
[3] Univ Warmia & Mazury, Geodynam Res Lab, Olsztyn, Poland
关键词
Plasmasphere; Ionosphere; Total electron content; Electron density profiles; Incoherent scatter radar; GPS TEC; IONOSPHERE; PLASMASPHERE; CHAMP; FIELD;
D O I
10.1016/j.asr.2014.04.011
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps. The comparison between two independent measurements was performed by analysis of the height-temporal distribution for specific location corresponding to the mid-latitudes of Europe. The percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 70%) during night-time. During day-time the lesser values (30-45%) were observed for quiet geomagnetic conditions and rather high values of the PEC contribution to GPS TEC (up to 90%) were observed during strong negative storm. These changes can be explained by the competing effects of electric fields and winds, which tend to raise the layer to the region with lower loss rate and movement of the ionospheric plasma to the plasmasphere. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:586 / 594
页数:9
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