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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Orientation variation of dayside auroral arc alignments obtained from all-sky observation at yellow river station, Svalbard
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Orientation variation of dayside auroral arc alignments obtained from all-sky observation at yellow river station, Svalbard

机译:从黄河站斯瓦尔巴特群岛的全天候观测获得的日间极光弧线取向的变化

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The orientations of dayside auroral arc alignments were calculated for over 40,000 images from all-sky observation at Yellow River Station, Svalbard. For each arc, its "orientation" and "tilt" are defined as the angle the arc alignment makes with the dusk-dawn direction and the local east-west direction, respectively. The mean arc orientation increases linearly with the increasing magnetic local time (MLT). There is a reversal point of the arc tilt located at near 10.5 MLT. Compared with the mean orientation, auroral arc alignment tilts to morning side in the higher latitude and tilts to evening side in the lower latitude in the prenoon sector, whereas it is the opposite in the postnoon sector. We further studied the effects of the interplanetary magnetic field (IMF) on the location of the arc tilt reversal point. We found that the reversal position shifts toward the midday for negative By. (C) 2016 Elsevier Ltd. All rights reserved.
机译:在斯瓦尔巴特群岛黄河站的全天候观测中,为40,000张图像计算了日间极光弧对准的方向。对于每个弧,其“方向”和“倾斜”分别定义为弧对齐与黄昏方向和局部东西方向所成的角度。平均电弧取向随磁性局部时间(MLT)的增加线性增加。电弧倾斜的反转点位于10.5 MLT附近。与平均方向相比,极高的弧线排列在早纬区域向较高纬度的早晨侧倾斜,在低纬度向较低纬度的夜侧倾斜,而在午后区域则相反。我们进一步研究了行星际磁场(IMF)对电弧倾斜反转点位置的影响。我们发现,对于负By,反转头寸朝中午转移。 (C)2016 Elsevier Ltd.保留所有权利。

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