From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection
From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection
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DOI：
10.1007/s11207-010-9602-8
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发表时间：
2010-08
期刊：
影响因子：
2.8
通讯作者：
M. Bisi;A. Breen;B. Jackson;R. Fallows;A. Walsh;Z. Mikić;P. Riley;C. Owen;A. González-Esparza;E. Aguilar-Rodriguez;H. Morgan;E. Jensen;A. Wood;M. Owens;M. Tokumaru;P. K. Manoharan;I. Chashei;A. Giunta;J. Linker;V. Shishov;S. Tyul’bashev;G. Agalya;S. K. Glubokova;M. S. Hamilton;K. Fujiki;P. Hick;J. Clover;B. Pintér
中科院分区：
文献类型：
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作者：
M. Bisi;A. Breen;B. Jackson;R. Fallows;A. Walsh;Z. Mikić;P. Riley;C. Owen;A. González-Esparza;E. Aguilar-Rodriguez;H. Morgan;E. Jensen;A. Wood;M. Owens;M. Tokumaru;P. K. Manoharan;I. Chashei;A. Giunta;J. Linker;V. Shishov;S. Tyul’bashev;G. Agalya;S. K. Glubokova;M. S. Hamilton;K. Fujiki;P. Hick;J. Clover;B. Pintér
我们报告了2005年5月13日太阳爆发事件的多仪器，多技术，协调研究的结果。我们讨论了日冕物质抛射（CME）的结果，以及对地球空间环境和地球上层大气的影响。行星际日冕物质抛射（ICME）对地球磁层的影响造成了2005年最强烈的地磁风暴，扰动风暴时间（Dst）指数峰值达到- 263 nT。陆地环境在全球范围内对风暴做出了反应。我们结合了日冕和行星际遥感仪器的观测和测量，行星际和近地遥感测量，地球磁层和电离层的遥感观测和现场测量，以及日冕和日球层模型。这些分析被用来追踪这一事件的起源、发展、传播、对陆地的影响以及随后的后果，以获得迄今为止对地球有效的太阳喷发最全面的看法。这一特殊事件也是美国国家航空航天局（nasa）赞助的“与恒星一起生活”（LWS）研究和美国国家科学基金会（nsf）正在进行的“太阳、日光层和行星际环境”（SHINE）社区调查的一部分。
We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environment and upper Earth atmosphere. The interplanetary CME (ICME) impacted the Earth’s magnetosphere and caused the most-intense geomagnetic storm of 2005 with a Disturbed Storm Time (Dst) index reaching −263 nT at its peak. The terrestrial environment responded to the storm on a global scale. We have combined observations and measurements from coronal and interplanetary remote-sensing instruments, interplanetary and near-Earthin-situmeasurements, remote-sensing observations andin-situmeasurements of the terrestrial magnetosphere and ionosphere, along with coronal and heliospheric modelling. These analyses are used to trace the origin, development, propagation, terrestrial impact, and subsequent consequences of this event to obtain the most comprehensive view of a geo-effective solar eruption to date. This particular event is also part of a NASA-sponsored Living With a Star (LWS) study and an on-going US NSF-sponsored Solar, Heliospheric, and INterplanetary Environment (SHINE) community investigation.