coronal mass ejection

Progress in the Study on the Solar Coronal Mass Ejection

日冕物质抛射研究进展

Coronal Mass Ejection Associated with Solar Type ⅱ Radio Bursts

日冕物质抛射与米波射电Ⅱ型爆发和Hα耀斑的关系

Fuzzy Classification of Solar Coronal Mass Ejection Properties

太阳日冕物质抛射特性的模糊分类研究

Classified prediction of geomagnetic disturbance caused by coronal mass ejection

日冕物质抛射引起地磁扰动的分类预报

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

模拟结果再现了环状日冕物质抛射的主要观测特征。

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

等离子体团型日冕物质抛射的形成机制

Metric Type ⅲ Radio Bursts and Coronal Mass Ejection

米波Ⅲ型爆发与日冕物质抛射

The formation and evolution of asymmetrical high density cloud and non-linear wave in a coronal mass ejection event

日冕物质抛射中非对称高密度云和非线性波的形成和演化

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

太阳质子事件、双带耀斑及日冕物质抛射

This event was of special interest because it gave off a coronal mass ejection at an angle that made it easy to view .

这次事件特别吸引人，因为它所引发日冕团块喷射的角度很容易观测。

the eruption called coronal mass ejection was caught on camera by NASA 's solar dynamic observatory , spacecraft that launched up back in February .

这次日冕大规模喷发由NASA的太阳能动态观察仪拍摄下来。这架航天器于二月份发射。

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 .

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。

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

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 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 .

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 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 .

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。

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 .

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。

This paper presents a numerical simulation of the slow shock triggered by a coronal mass ejection , taking a coronal streamer with an equatorial electric current sheet as the background as well as a magnetic flux eruption at the base of the coronal streamer as the driving mechanism .

本文取带赤道电流片的冕流结构作为背景，用冕流底部的磁通量喷发作为驱动机制，对日冕物质喷射触发的慢激波进行数值模拟。