Response of the midlatitude ionosphere to extreme geomagnetic storms of the 23rd solar cycle

被引:2
|
作者
Potekhin, A. P. [1 ]
Zherebtsov, G. A. [1 ]
Kurkin, V. I. [1 ]
Medvedev, A. V. [1 ]
Ratovsky, K. G. [1 ]
Shpynev, B. G. [1 ]
机构
[1] Russian Acad Sci, Siberian Banch, Inst Solar Terr Phys, Irkutsk 664033, Russia
基金
俄罗斯基础研究基金会;
关键词
Geomagnetic Storm; Incoherent Scatter Radar; Ionospheric Layer; Auroral Activity; Relative Disturbance;
D O I
10.1134/S0016793209080350
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The ionospheric response in the Irkutsk region (52.3A degrees N, 104.3A degrees E) to the extreme geomagnetic storms of solar cycle 23 was studied based on the data of the Irkutsk incoherent scatter radar (ISR) and DPS-4 vertical sounding digital ionosonde. The deviations of parameters from the undisturbed level, i.e., from the monthly medians or the values obtained on a quiet day, were considered as an ionospheric response. Values of the electron concentration maximum (N (m)F2) and electron temperature (T (e)) at a height of 350 km were chosen as parameters. The ionospheric response is interpreted in the scope of the concept of a thermospheric storm and penetration of the magnetospheric electric field.
引用
收藏
页码:1218 / 1222
页数:5
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