Geomagnetic activity at Northern Hemisphere's mid-latitude ground stations: How much can be explained using TS05 model

被引:3
|
作者
Castillo, Yvelice [1 ,2 ,4 ]
Pais, Maria Alexandra [1 ,2 ]
Fernandes, Joao [1 ,3 ]
Ribeiro, Paulo [1 ]
Morozova, Anna L. [1 ]
Pinheiro, Fernando J. G. [1 ]
机构
[1] Univ Coimbra, Geophys & Astron Observ, CITEUC, P-3040004 Coimbra, Portugal
[2] Univ Coimbra, Dept Phys, P-3004516 Coimbra, Portugal
[3] Univ Coimbra, Dept Math, P-3004516 Coimbra, Portugal
[4] Natl Autonomous Univ Honduras, Dept Astron & Astrophys, Tegucigalpa, Honduras
关键词
Magnetic observatories; Geomagnetic activity; Magnetospheric sources; Tsyganenko and Sitnov model; MAGNETOSPHERIC CURRENT SYSTEMS; DAWN-DUSK ASYMMETRY; MAGNETIC STORMS; INNER MAGNETOSPHERE; RING CURRENT; SOLAR-WIND; FIELD; CURRENTS; SQ; PARAMETERIZATION;
D O I
10.1016/j.jastp.2017.11.002
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
For the 2007 to 2014 period, we use a statistical approach to evaluate the performance of Tsyganenko and Sitnov [2005] semi-empirical model (TS05) in estimating the magnetospheric transient signal observed at four Northern Hemisphere mid-latitude ground stations: Coimbra, Portugal; Panagyurishte, Bulgary; Novosibirsk, Russia and Boulder, USA. Using hourly mean data, we fmd that the TS05 performance is clearly better for the X (North-South) than for the Y (East-West) field components and for more geomagnetically active days as determined by local K-indices. In similar to 50% (X) and similar to 30% (Y) of the total number of geomagnetically active days, correlation values yield r >= 0.7. During more quiet conditions, only similar to 30%(X) and similar to 15% (Y) of the number of analyzed days yield r >= 0.7. We compute separate contributions from different magnetospheric currents to data time variability and to signal magnitude. During more active days, all tail, symmetric ring and partial ring currents contribute to the time variability of X while the partial ring and field aligned currents contribute most to the time variability of Y. The tail and symmetric ring currents are main contributors to the magnitude of X. In the best case estimations when r >= 0.7, remaining differences between observations and TS05 predictions could be explained by global induction in the Earth's upper layers and crustal magnetization. The closing of field aligned currents through the Earth's center in the TS05 model seems to be mainly affecting the Y magnetospheric field predictions.
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页码:38 / 53
页数:16
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