Do the Throat Auroras Create Polar Cap Patches?

Author:

Zhang Duan1ORCID,Zhang Qing‐He1ORCID,Oksavik Kjellmar23ORCID,Xu Tong4ORCID,Xing Zan‐Yang1ORCID,Lyons L. R.5ORCID,Han De‐Sheng6ORCID,Zhang Hong‐Bo4ORCID,Ma Yu‐Zhang1ORCID,Hu Ze‐Jun7ORCID,Liu Jian‐Jun7ORCID,Wang Yong1ORCID,Wang Xiang‐Yu1

Affiliation:

1. Shandong Provincial Key Laboratory of Optical Astronomy and Solar‐Terrestrial Environment Institute of Space Sciences Shandong University Weihai China

2. Birkeland Centre for Space Sciences Department of Physics and Technology University of Bergen Bergen Norway

3. Arctic Geophysics University Centre in Svalbard Longyearbyen Norway

4. National Key Laboratory of Electromagnetic Environment China Research Institute of Radiowave Propagation Qingdao China

5. Department of Atmospheric and Oceanic Sciences University of California CA Los Angeles USA

6. State Key Laboratory of Marine Geology School of Ocean and Earth Science Tongji University Shanghai China

7. Polar Research Institute of China Shanghai China

Abstract

AbstractThroat auroras and polar cap patches are common phenomena in the polar ionosphere resulting from magnetosphere‐ionosphere coupling. A campaign was organized, with all‐sky imagers at Yellow River Station, the European Incoherent Scatter Svalbard Radar, and coordinated low‐altitude spacecraft observations. During periods of radial interplanetary magnetic field (IMF), observations showed that, as poleward moving throat auroras faded around the polar cap boundary, they linked to poleward moving ionization patches. The throat auroras were produced by soft‐electron precipitation associated with dayside magnetic reconnection. The red line emission intensity of throat auroras was correlated with dayside reconnection events. Dense plasma from lower latitudes was transported poleward via enhanced convection in the throat auroras to form patches. This is a potentially new formation mechanism for patches associated with throat auroras and magnetic reconnection for radial IMF. Moreover, the patches move anti‐sunward due to the E × B drift.

Funder

National Natural Science Foundation of China

China Postdoctoral Science Foundation

China Scholarship Council

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3