Disturbances in the ionospheric F-region peak heights in the American longitudinal sector during geomagnetic storms of September 2005

被引:22
作者
Klimenko, M. V. [1 ,2 ]
Klimenko, V. V. [1 ]
Ratovsky, K. G. [3 ]
Goncharenko, L. P. [4 ]
机构
[1] W Dept NV Pushkov IZMIRAN RAS, Kaliningrad 236010, Russia
[2] Kaliningrad State Tech Univ, Kaliningrad 236000, Russia
[3] Inst Solar Terr Phys SB RAS, Irkutsk 664033, Russia
[4] MIT, Haystack Observ, Westford, MA 01886 USA
基金
美国国家科学基金会; 俄罗斯基础研究基金会;
关键词
Geomagnetic storm; Ionospheric modeling; F-region maximum height; Electric field; F3-layer; Thermospheric wind surge; 1999 SOLAR ECLIPSE; EQUATORIAL IONOSPHERE; NUMERICAL-SIMULATION; ELECTRIC-FIELD; PROTONOSPHERE SYSTEM; PHYSICAL-MECHANISM; MODEL; PARAMETERS; AUGUST; EISCAT;
D O I
10.1016/j.asr.2011.06.002
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In this paper, we use the modified GSM TIP model to explore how the thermosphere ionosphere system in the American longitudinal sector responded to the series of geomagnetic storms on September 9-14, 2005. Comparison of modeling results with experimental data at Millstone Hill, USA (42.6 degrees N, 71.5 degrees W), Ramey, Puerto Rico (18.3 degrees N, 66.8 degrees W) and Jicamarca, Peru (11.9 degrees S, 76.9 degrees W) has shown a good agreement of ionospheric disturbances in the F-region maximum height. We examine in detail the formation mechanisms of these disturbances at different latitudes and describe some of the important physical processes affecting the behavior of the F-region. In addition, we consider the propagation of thermospheric wind surge and the formation of additional layers in the low-latitude ionosphere during geomagnetic storms. (C) 2011 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1184 / 1195
页数:12
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