Multiple Satellite Observations of the High-Latitude Cusp Aurora During Northward IMF Conditions

被引:0
|
作者
Zhou, Su [1 ]
Luan, Xiaoli [2 ]
Hou, Ying [1 ]
机构
[1] Guizhou Univ, Sch Sci, Guiyang, Peoples R China
[2] Univ Sci & Technol China, Sch Earth & Space Sci, CAS Key Lab Geospace Environm, Hefei, Peoples R China
基金
中国国家自然科学基金;
关键词
INTERPLANETARY MAGNETIC-FIELD; DAYSIDE CONVECTION; PRECIPITATION; IDENTIFICATION; EXCITATION; PRESSURE;
D O I
10.1029/2024JA032963
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Cusp auroras poleward of the typical auroral oval are ascribed to high-latitude lobe reconnection when the Interplanetary Magnetic Field (IMF) Bz is predominantly northward. In this study, we further investigate the ionospheric characteristics of a unique high-latitude cusp region employing multiple satellite observations. A cusp aurora event with wide spatial spread was observed in the postnoon polar cap region. It was found to be associated with northward IMF Bz and positive By components. The cusp aurora was located from 68 degrees to 86 degrees in magnetic latitude and within 15-17 hr in magnetic local time. This broad coverage in the polar cap indicates direct precipitating particles from the magnetosheath. Particle energy is different between the equatorward and poleward edges of the cusp aurora. The precipitating ions at the equatorward side maintain magnetosheath particle characteristics as expected, while ions with higher energies occurred in the poleward side. Further, the poleward edge of the cusp aurora was nearly situated in the center of a convection shear and was associated with an upward field-aligned current. These observations suggest a lobe cell circulation, hence we attribute the formation of the cusp aurora to the high-latitude lobe reconnection. Simultaneous observations in the southern hemisphere indicate the absence of cusp aurora. The auroral presence only in the northern hemisphere is probably due to the combination of large dipole tilt angle and positive IMF Bz, which facilitates the lobe reconnection. Average energy of precipitating ions in the cusp region is higher at the poleward edge than at the equatorward edge The poleward edge of the observed cusp aurora coexists with a significant convection shear center and an upward field-aligned current Occurrence of the high-latitude cusp aurora is attributed to the combination of a large dipole tilt angle and northward Interplanetary Magnetic Field conditions
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页数:14
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