The Impact of Century-Scale Changes in the Core Magnetic Field on External Magnetic Field Contributions

被引:0
作者
Ingrid Cnossen
机构
[1] British Antarctic Survey,
[2] GFZ German Center for Geosciences,undefined
来源
Space Science Reviews | 2017年 / 206卷
关键词
Magnetic field; Magnetosphere; Ionosphere; Secular variation; Current systems;
D O I
暂无
中图分类号
学科分类号
摘要
The Earth’s internal magnetic field controls to a degree the strength, geographic positioning, and structure of currents flowing in the ionosphere and magnetosphere, which produce their own (external) magnetic fields. The secular variation of the Earth’s internal magnetic field can therefore lead to long-term changes in the externally produced magnetic field as well. Here we will examine this more closely. First, we obtain scaling relations to describe how the strength of magnetic perturbations associated with various different current systems in the ionosphere and magnetosphere depends on the internal magnetic field intensity. Second, we discuss how changes in the orientation of a simple dipolar magnetic field will affect the current systems. Third, we use model simulations to study how actual changes in the Earth’s internal magnetic field between 1908 and 2008 have affected some of the relevant current systems. The influence of the internal magnetic field on low- to mid-latitude currents in the ionosphere is relatively well understood, while the effects on high-latitude current systems and currents in the magnetosphere still pose considerable challenges.
引用
收藏
页码:259 / 280
页数:21
相关论文
共 156 条
  • [11] Wang W.(1998)Generalized theorem of no ground magnetic effect of vertical current connected with Pedersen currents in the uniform conductivity ionosphere J. Geophys. Res. 103 11,155-309
  • [12] Schmitt P.(2004)Longitudinal and interhemispheric variations of auroral ionospheric electrodynamics in a realistic geomagnetic field Ann. Geophys. 22 284-12,376
  • [13] Cnossen I.(1976)Concerning long-term geomagnetic variations and space climatology Geophys. Res. Lett. 3 12,365-604
  • [14] Richmond A.D.(2007)Mercury and Mars: the role of ionospheric conductivity in the acceleration of magnetospheric particles J. Geophys. Res. 112 601-298
  • [15] Wiltberger M.(2004)Modeling seasonal and diurnal effects on ionospheric conductances, region-2 currents, and plasma convection in the inner magnetosphere J. Geophys. Res. 109 293-1328
  • [16] Cnossen I.(2016)Intercomparison of ionospheric electrodynamics from the iridium constellation with global MHD simulations Space Sci. Rev. 107 1325-68
  • [17] Wiltberger M.(2002)North-South asymmetries: effects on high-latitude geospace J. Geophys. Res. 66 32-547
  • [18] Ouellette J.E.(2004)Ionospheric currents and field-aligned currents generated by dynamo action in an asymmetric magnetic field J. Atmos. Sol.-Terr. Phys. 29 521-4680
  • [19] De Haro Barbas B.F.(2011)The Lyon-Fedder-Mobarry (LFM) global MHD magnetospheric simulation code Ann. Geophys. 99 4675-489
  • [20] Elias A.G.(1994)Climatology of the inter-hemispheric field-aligned current system in the equatorial ionosphere as observed by CHAMP J. Geophys. Res. 154 485-3556