Sheared magnetic field structure in Jupiter's dusk magnetosphere: Implications for return currents
Sheared magnetic field structure in Jupiter's dusk magnetosphere: Implications for return currents
复制标题
木星黄昏磁层中的剪切磁场结构:对返回电流的影响
DOI:
10.1029/2001ja000251
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发表时间:
2002
影响因子:
--
通讯作者:
R. Walker
中科院分区:
文献类型:
--
作者:
M. Kivelson;K. Khurana;R. Walker
[1] The configuration of the magnetic field near 100 RJ in the dusk sector of the Jovian magnetosphere varies with distance from the equatorial current sheet. The changing twist out of meridian planes is consistent with flows that lag corotation near the equator but that may lead corotation at higher latitudes. Although a portion of the field perturbation may be produced by magnetopause currents, we argue that the observed sheared field structure requires field-aligned current flowing toward Jupiter’s ionosphere inside the magnetopause but beyond � 100 RJ. This current must include a portion of the return current of the system that enforces partial corotation of outward moving magnetospheric plasma and may also be fed by boundary layer currents of the region 1 type. We estimate the total current into the auroral ionosphere as � 6 MA, and this current would flow into a narrow band of latitude (<2� ) poleward of the main auroral oval. INDEX TERMS: 5737 Planetology: Fluid Planets: Magnetospheres (2756); 2756 Magnetospheric Physics: Planetary magnetospheres (5443, 5737, 6030); 2740 Magnetospheric Physics: Magnetospheric configuration and dynamics; 2731 Magnetospheric Physics: Magnetosphere—outer; KEYWORDS: planetary magnetosphere, Jupiter’s magnetosphere, field-aligned currents, magnetospheric configuration