喉区极光过程中的能量输入估算

P353; 伴随该事件由电子携带的输入到电离层的总能量约为1.07×1011 J,单位面积输入能量的平均功率约为1.31×10-4 W·m-2,对比以往研究中MHD模拟给出的通常情况下极隙区能量输入结果,本文给出的喉区极光过摘 要 喉区极光是一种只发生在磁正午附近的特殊分立极光,具有明显的从分立极光卵赤道侧边界向低纬延伸的特征.已有研究表明,喉区极光对应于一种由磁重联导致的磁层顶局地凹陷.磁重联是太阳风能量注入到地球磁层空间的重要方式之一,但伴随喉区极光过程有多少能量传输进入电离层尚不明确.利用 2015年 12月的地基全天空极光观测与经过电离层上方的卫星粒子共轭观测,建立了极光强度与沉降电子...

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Published in空间科学学报 Vol. 44; no. 1; pp. 51 - 59
Main Authors 范天舒, 曹永军, 邱荟璇, 王智伟, 韩德胜
Format Journal Article
LanguageChinese
Published 内蒙古师范大学物理与电子信息学院 呼和浩特 010020%同济大学海洋与地球科学学院 上海 200129 2024
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ISSN0254-6124
DOI10.11728/cjss2024.01.2023-0065

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Abstract P353; 伴随该事件由电子携带的输入到电离层的总能量约为1.07×1011 J,单位面积输入能量的平均功率约为1.31×10-4 W·m-2,对比以往研究中MHD模拟给出的通常情况下极隙区能量输入结果,本文给出的喉区极光过摘 要 喉区极光是一种只发生在磁正午附近的特殊分立极光,具有明显的从分立极光卵赤道侧边界向低纬延伸的特征.已有研究表明,喉区极光对应于一种由磁重联导致的磁层顶局地凹陷.磁重联是太阳风能量注入到地球磁层空间的重要方式之一,但伴随喉区极光过程有多少能量传输进入电离层尚不明确.利用 2015年 12月的地基全天空极光观测与经过电离层上方的卫星粒子共轭观测,建立了极光强度与沉降电子能通量之间的相关关系.在此基础上,针对发生在 2015年 12月 8日的一个典型喉区极光事件,在综合考虑持续时间与空间尺度基础上,估算出程中能量输入的效率约为MHD模拟结果的两倍,表明伴随喉区极光过程的能量输入非常可观,可能引起局地空间天气效应.
AbstractList P353; 伴随该事件由电子携带的输入到电离层的总能量约为1.07×1011 J,单位面积输入能量的平均功率约为1.31×10-4 W·m-2,对比以往研究中MHD模拟给出的通常情况下极隙区能量输入结果,本文给出的喉区极光过摘 要 喉区极光是一种只发生在磁正午附近的特殊分立极光,具有明显的从分立极光卵赤道侧边界向低纬延伸的特征.已有研究表明,喉区极光对应于一种由磁重联导致的磁层顶局地凹陷.磁重联是太阳风能量注入到地球磁层空间的重要方式之一,但伴随喉区极光过程有多少能量传输进入电离层尚不明确.利用 2015年 12月的地基全天空极光观测与经过电离层上方的卫星粒子共轭观测,建立了极光强度与沉降电子能通量之间的相关关系.在此基础上,针对发生在 2015年 12月 8日的一个典型喉区极光事件,在综合考虑持续时间与空间尺度基础上,估算出程中能量输入的效率约为MHD模拟结果的两倍,表明伴随喉区极光过程的能量输入非常可观,可能引起局地空间天气效应.
Abstract_FL The throat aurora is a kind of discrete auroras occurred around the Magnetic Local Noon(MLN).The discrete arc is almost vertical to the auroral oval and extends equatorward.Previous stu-dies have shown that the throat auroral structure corresponds to the localized magnetopause indenta-tions which are related to the particular magnetopause reconnection.As is known,magnetic reconnec-tion is the important approach inputting energy of solar wind,so the research of energy input of throat aurora is key to understand this particular magnetopause reconnection.A new way to estimate the ener-gy input by using all auroral events happened on December 2015 is built.A relational expression about auroral intensity and energy flux of electronic precipitation is set up by observations of both ground sta-tion and satellite.Estimating the total energy input of a typical throat auroral event which lasted three minutes and happened on 8 December 2015 by this relational expression,and the answer is about 1.07×1011 J.And the average power of input energy per area is about1.31×10-4 W·m-2.Compared with the usual polar gap energy input results given by MHD simulation in previous studies,the energy input efficiency of the throat auroral process given in this paper is about twice that of the MHD simula-tion results,which indicates that the energy input accompanying the throat auroral process is very con-siderable and may cause local space weather effects.
Author 韩德胜
曹永军
范天舒
邱荟璇
王智伟
AuthorAffiliation 内蒙古师范大学物理与电子信息学院 呼和浩特 010020%同济大学海洋与地球科学学院 上海 200129
AuthorAffiliation_xml – name: 内蒙古师范大学物理与电子信息学院 呼和浩特 010020%同济大学海洋与地球科学学院 上海 200129
Author_FL QIU Huixuan
HAN Desheng
FAN Tianshu
CAO Yongjun
WANG Zhiwei
Author_FL_xml – sequence: 1
  fullname: FAN Tianshu
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  fullname: HAN Desheng
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  fullname: 王智伟
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  fullname: 韩德胜
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DocumentTitle_FL Estimation of Energy Input during Throat Aurora Processes
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Keywords 能量输入功率
Electron energy flux
Energy input power
电子能通量
极光强度
喉区极光
Throat aurora
Auroral intensity
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Snippet P353; 伴随该事件由电子携带的输入到电离层的总能量约为1.07×1011 J,单位面积输入能量的平均功率约为1.31×10-4 W·m-2,对比以往研究中MHD模拟给出的通常情况下极隙区能量输入结果,本文给出的喉区极光过摘 要...
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Title 喉区极光过程中的能量输入估算
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