首页> 美国卫生研究院文献>Scientific Reports >North-South Asymmetry in the Geographic Location of Auroral Substorms correlated with Ionospheric Effects
【2h】

North-South Asymmetry in the Geographic Location of Auroral Substorms correlated with Ionospheric Effects

机译:与电离层效应相关的极光亚暴地理位置的南北不对称

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

Energetic particles of magnetospheric origin constantly strike the Earth’s upper atmosphere in the polar regions, producing optical emissions known as the aurora. The most spectacular auroral displays are associated with recurrent events called magnetospheric substorms (aka auroral substorms). Substorms are initiated in the nightside magnetosphere on closed magnetic field lines. As a consequence, it is generally thought that auroral substorms should occur in both hemispheres on the same field line (i.e., magnetically conjugated). However, such a hypothesis has not been verified statistically. Here, by analyzing 2659 auroral substorms acquired by the Ultraviolet Imager on board the NASA satellite “Polar”, we have discovered surprising evidence that the averaged location for substorm onsets is not conjugate but shows a geographic preference that cannot be easily explained by current substorm theories. In the Northern Hemisphere (NH) the auroral substorms occur most frequently in Churchill, Canada (~90°W) and Khatanga, Siberia (~100°E), up to three times as often as in Iceland (~22°W). In the Southern Hemisphere (SH), substorms occur more frequently over a location in the Antarctic ocean (~120°E), up to ~4 times more than over the Antarctic Continent. Such a large difference in the longitudinal distribution of north and south onset defies the common belief that substorms in the NH and SH should be magnetically conjugated. A further analysis indicates that these substorm events occurred more frequently when more of the ionosphere was dark. These geographic areas also coincide with regions where the Earth’s magnetic field is largest. These facts suggest that auroral substorms occur more frequently, and perhaps more intensely, when the ionospheric conductivity is lower. With much of the magnetotail energy coming from the solar wind through merging of the interplanetary and Earth’s magnetic field, it is generally thought that the occurrence of substorms is externally controlled by the solar wind and plasma instability in the magnetotail. The present study results provide a strong argument that the ionosphere plays a more active role in the occurrence of substorms.
机译:磁层起源的高能粒子不断撞击两极的地球高层大气,产生称为极光的光发射。最壮观的极光显示与称为磁层亚暴(又称极光亚暴)的复发事件有关。亚暴在封闭磁场线上的夜间磁层中引发。结果,通常认为极光亚暴应该发生在同一场线上的两个半球(即磁共轭)。但是,这种假设尚未得到统计证实。在这里,通过分析NASA卫星“极地”上的紫外线成像仪获得的2659次极光亚暴,我们发现了令人惊讶的证据,表明亚暴发作的平均位置不是共轭的,而是显示了地理偏好,而当前的亚暴理论无法轻易解释。在北半球,极光亚暴最常发生在加拿大的丘吉尔(〜90°W)和西伯利亚的卡丹加(〜100°E),是冰岛(〜22°W)的三倍。在南半球(SH)中,亚暴在南极海洋某个位置(〜120°E)上发生的频率更高,是南极大陆的约4倍。南北向的纵向分布差异如此之大,违背了人们普遍认为北半球和南半球的亚暴应该磁共轭的普遍看法。进一步的分析表明,当更多的电离层较暗时,这些亚暴事件发生的频率更高。这些地理区域也与地球磁场最大的区域重合。这些事实表明,当电离层电导率较低时,极光亚暴的发生频率更高,也许更强烈。由于星际磁场和地球磁场的合并,大部分磁尾能量来自太阳风,因此人们普遍认为,亚暴的发生是由太阳风和磁尾中等离子体的不稳定性所控制的。本研究结果提供了强有力的论据,认为电离层在亚暴的发生中起着更积极的作用。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号