Spatial features of Weddell Sea and Yakutsk Anomalies in foF2 diurnal variations during high solar activity periods: Interkosmos-19 satellite and ground-based ionosonde observations, IRI reproduction and GSM TIP model simulation

被引:39
|
作者
Klimenko, M. V. [1 ,2 ]
Klimenko, V. V. [1 ]
Karpachev, A. T. [3 ]
Ratovsky, K. G. [4 ]
Stepanov, A. E. [5 ]
机构
[1] RAS, West Dept, Pushkov Inst Terr Magnetism Ionosphere & Radio Wa, Kaliningrad 236017, Russia
[2] Immanuel Kant Balt Fed Univ, Kaliningrad 236041, Russia
[3] RAS, Pushkov Inst Terr Magnetism Ionosphere & Radio Wa, Troitsk 142190, Moscow Region, Russia
[4] RAS, Inst Solar Terr Phys SB, Irkutsk, Russia
[5] Inst Cosmophys Res & Aeron, Yakutsk, Russia
基金
俄罗斯基础研究基金会;
关键词
Longitudinal variations; Weddell Sea Anomaly; Topside sounding; Ionosonde; Numerical simulation; IONOSPHERE;
D O I
10.1016/j.asr.2014.12.032
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We studied the main morphology of the formation of summer ionospheric anomalies which includes the Weddell Sea Anomaly (WSA) and the Yakutsk Anomaly (YA) in terms of positive night-to-day foF2 differences. For this purpose, we have for the first time used topside sounding (Interkosmos-19 satellite) and ground-based (ionosonde) data as well as results from an empirical model (International Reference Ionosphere - IRI) and from a first-principles model (Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere - GSM TIP). The main spatial morphological characteristics of the WSA and YA are similar which points to a common cause for their occurrence. Our preliminary GSM TIP model results showed that the foF2 values at nighttime are greater than at daytime due to: (1) the horizontal plasma transport due to electromagnetic drift; (2) the vertical component of plasma transport along the geomagnetic field lines via meridional neutral wind; (3) the distribution of the neutral composition of the thermosphere. (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.
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页码:2020 / 2032
页数:13
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