Numerical simulation of an ionospheric disturbance over EISCAT using a global ionospheric model

被引:11
|
作者
Namgaladze, AA [1 ]
Martynenko, OV [1 ]
Namgaladze, AN [1 ]
Volkov, MA [1 ]
Korenkov, YN [1 ]
Klimenko, VV [1 ]
Karpov, IV [1 ]
Bessarab, FS [1 ]
机构
[1] INST TERR MAGNETISM IONOSPHERE & RADIOWAVE PROPAG,KALININGRAD OBSERV,KALININGRAD 236017,RUSSIA
来源
关键词
D O I
10.1016/0021-9169(95)00037-2
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
A global numerical model of the Earth's upper atmosphere has been used to simulate numerically the behaviour of the ionosphere observed by EISCAT on 24-25 March 1987 when the quiet day of 24 March was followed by the disturbed day of 25 March, with a Sudden Commencement (SC) starting about 1540 UT. We have selected the model input data for the auroral precipitating particle fluxes and the field-aligned currents to obtain an acceptable agreement between the calculated and observed ionospheric variations. A rather good similarity between the calculated and observed variations of the electric field, E-region electron concentration, F2-region ion temperature and electron concentration has been found. Spatial distributions of the electric potential and F2-region electron concentration and ion temperature have been obtained. The dynamics of the main ionospheric trough during the disturbed period has been investigated. It has been found that the equatorward movement of the midnight part of the trough is connected with the enhanced plasma transport, while the apparent westward and eastward movements of the evening and morning edges of the trough are connected with the ''hot spots'' caused by Joule heating of the ion gas.
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页码:297 / &
页数:9
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