日冕物质抛射

在子午面内，研究具有嵌套闭磁场结构冕流背景对触发日冕物质抛射（CME）特征的影响。

The influence of a streamer background with nested close magnetic structures on the properties of CME initiated from its bottom is investigated in a solar meridian plane .

微波Ⅲ型爆发与日冕物质抛射的统计分析

Statistics and Analysis on the Relation Between Microwave Type ⅲ Bursts and CME Events

晕状日冕物质抛射~（14）C激发态中子晕

Neutron Halo of the Excited States in ~ ( 14 ) C

日冕物质抛射与米波射电Ⅱ型爆发和Hα耀斑的关系

Coronal Mass Ejection Associated with Solar Type ⅱ Radio Bursts

大型日冕物质抛射如直接冲击地球将会造成大破坏，产生出的强大地磁风暴有可能会扰乱gps信号，广播通讯和电网。

Big CMEs that hit Earth squarely can wreak havoc , spawning powerful geomagnetic storms with the potential to disrupt GPS signals , radio communications and power grids .

在一维球坐标系下模拟了1998年11月4日至5日3个连续日冕物质抛射（CME）在行星际空间的传播和相互作用并最终形成复杂抛射的日地传输过程。

The solar-terrestrial transit process of three successive CMEs during November 4-5 , 1998 has been investigated numerically in one-dimensional spherical geometry .

在太阳耀斑、日冕物质抛射（CME）和其他太阳活动现象中，磁重联一直都扮演着至关重要的作用。

Magnetic reconnection plays a very important role in solar flares , corona mass ejections ( CME ), and other solar activities .

戈达德试图将戏剧性的红色极光与太阳的日冕物质抛射联系起来，而后者在SOHO图像上根本不存在。

Goddard tried to relate the dramatic red auroras to a CME on the Sun , which was nonexistent in the SOHO images .

统计分析了23周太阳活动峰年期间（1998.12～2002.12）记录到的米波Ⅱ型爆发，与Hα耀斑和日冕物质抛射（CME）事件的关系。

The statistical analyses of the metric type ⅱ bursts , Coronal mass ejection ( CME ) and H α flares duration the 23rd solar cycle are carried out in this paper .

采用理想磁流体力学方程组（MHD）作为太阳大气动力学过程的控制方程组，定性数值模拟日冕物质抛射（CME）现象。

The ideal Magnetohydrodynamic equations ( MHD ), the governing equations of the solar atmosphere dynamical process , are taken to numerically simulate Coronal Mass Ejection ( CME ) phenomena .

日冕物质抛射（CME）属于大尺度太阳活动现象，它能造成地球空间环境的剧烈扰动，是空间灾害天气的主要源头。

Coronal mass ejections ( CMEs ) belong to large-scale solar active phenomena and cause strong disturbances on the geospace environment , being a main source of disastrous space weather .

主要介绍晕状日冕物质抛射（haloCMEs）的产生机制.包括向量磁场演化是怎样触发haloCMEs的；

This paper mechanisms of halo coronal mass ejections ( halo CMEs ) have been mainly presented , including how the evolution of vector magnetic field triggers the halo CMEs ?

最近的一次大型太阳活动发生在2012年7月，日冕物质抛射（CME）穿过地球轨道并撞向日地关系天文台STEREO-A空间站。

The most recent major burst of solar activity occurred in July 2012 , when a coronal mass ejection ( CME ) passed through Earth 's orbit and hit the STEREO-A space station .

太阳活动密切地影响着日地空间环境和地球高空大气结构，太阳耀斑爆发产生的日冕物质抛射（CME）是空间灾害的主要原因之一。

Solar activity , especially , Coronal Mass Ejection ( CME ) during a large solar activity affected the space environment of human being and could be one of main reasons of the space disaster .

根据WIND飞船的观测资料，讨论了2000年发生的南向磁场（Bs）事件，分析了它们的源，发现12次事件中有11次的源是日冕物质抛射（CME）。

According to the observations from WIND spacecraft , the events of southward magnetic field ( Bs events ) occurred in 2000 are studied . Among these 12 events , there were 11 events associated with the coronal mass ejections ( CMEs ) .

给出了特殊类型的日冕物质抛射（CME）数值模拟定性结果，这种CME核心闭磁场结构前半部分磁力线的方向与太阳整体偶极场磁力线的方向相反。

Qualitative numerical result of a special type of Coronal Mass Ejection ( CME ) is presented . The magnetic field direction in front half part of central closed magnetic field of the CME is opposite to that of the solar global dipole .

当一个日冕物质抛射伴随冕流产生时，冕流的经向角大小若大于27°，可导致冕流尖角区顶部上升速度大于2km／s。

The rise velosity of the top of the cusp region in a coronal streamer may be more than 2km / s , if the longitude angular size is more than 27 ° associated with a CME occurence .

日冕物质抛射引起地磁扰动的分类预报

Classified prediction of geomagnetic disturbance caused by coronal mass ejection

日冕物质抛射研究进展

Progress in the Study on the Solar Coronal Mass Ejection

两冕流间的对称径向膨胀日冕物质抛射事件

Radial expansion of a symmetrical CME between two coronal streamers

太阳质子事件、双带耀斑及日冕物质抛射

Solar proton event , two-ribbon flare and coronal mass ejection

日冕物质抛射及相关太阳活动的观测研究

Observations on Coronal Mass Ejections and Its Associated Solar Activities

日冕物质抛射和太阳表面磁活动的关系

Correlation Between Coronal Mass Ejections and Solar Surface Magnetic Activities

米波Ⅲ型爆发与日冕物质抛射

Metric Type ⅲ Radio Bursts and Coronal Mass Ejection

射电运动Ⅳ型爆发和日冕物质抛射

Radio Moving Type ⅳ Bursts and Coronal Mass Ejections

模拟结果再现了环状日冕物质抛射的主要观测特征。

The results demonstrated the main observed characteristics of the loop-like coronal mass ejection .

等离子体团型日冕物质抛射的形成机制

D shape . a mechanism for the formation of plasmoid type coronal mass ejection

太阳日冕物质抛射的磁流体力学性质

The hydromagnetic nature of solar coronal mass ejections

太阳日冕物质抛射特性的模糊分类研究

Fuzzy Classification of Solar Coronal Mass Ejection Properties

冕流与日冕物质抛射的关系

The relationship between coronal streamers and CMES