From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection

被引：0

作者：

M. M. Bisi

A. R. Breen

B. V. Jackson

R. A. Fallows

A. P. Walsh

Z. Mikić

P. Riley

C. J. Owen

A. Gonzalez-Esparza

E. Aguilar-Rodriguez

H. Morgan

E. A. Jensen

A. G. Wood

M. J. Owens

M. Tokumaru

P. K. Manoharan

I. V. Chashei

A. S. Giunta

J. A. Linker

V. I. Shishov

S. A. Tyul’bashev

G. Agalya

S. K. Glubokova

M. S. Hamilton

K. Fujiki

P. P. Hick

J. M. Clover

B. Pintér

机构：

[1] University of California,Center for Astrophysics and Space Sciences

[2] San Diego,Institute of Mathematics and Physics

[3] Aberystwyth University,Space Environment Physics Group, Department of Meteorology

[4] University of Reading,Mullard Space Science Laboratory

[5] University College London,MEXART, Instituto de Geofisica, Unidad Michoacán

[6] Predictive Science,Institute for Astronomy

[7] Inc.,Solar

[8] Universidad Nacional Autonoma de Mexico,Terrestrial Environment Laboratory (STELab)

[9] University of Hawaii,Radio Astronomy Centre, National Centre for Radio Astrophysics

[10] ACS Consulting,Pushchino Radio Astronomy Observatory, Astrospace Center

[11] MMT Observatory,Department of Physics

[12] Nagoya University,Space Science and Technology Department

[13] Tata Institute of Fundamental Research,San Diego Supercomputer Center

[14] Lebedev Physical Institute,undefined

[15] University of Strathclyde,undefined

[16] Rutherford Appleton Laboratory,undefined

[17] Pushchino State University,undefined

[18] University of California,undefined

[19] San Diego,undefined

来源：

Solar Physics | 2010年 / 265卷

关键词：

Active regions, magnetic fields; Corona, models; Corona, radio emission; Coronal mass ejections, initiation and propagation; Coronal mass ejections, interplanetary; Magnetic fields, interplanetary; Magnetic fields, models; Radio bursts, association with flares; Radio scintillation; Solar wind, disturbances; Sunspots, magnetic fields; Velocity fields, solar wind; X-ray bursts, association with flares;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

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-Earth in-situ measurements, remote-sensing observations and in-situ measurements 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.

引用

页码：49 / 127

页数：78

共 50 条

[1] From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection
Bisi, M. M.
Breen, A. R.
Jackson, B. V.
Fallows, R. A.
Walsh, A. P.
Mikic, Z.
Riley, P.
Owen, C. J.
Gonzalez-Esparza, A.
Aguilar-Rodriguez, E.
Morgan, H.
Jensen, E. A.
Wood, A. G.
Owens, M. J.
Tokumaru, M.
Manoharan, P. K.
Chashei, I. V.
Giunta, A. S.
Linker, J. A.
Shishov, V. I.
Tyul'bashev, S. A.
Agalya, G.
Glubokova, S. K.
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