ejections

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

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。

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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.

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。

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Solar coronal mass ejections in space weather

日冕物质抛射&空间天气的扰动源

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Radio Moving Type ⅳ Bursts and Coronal Mass Ejections

射电运动Ⅳ型爆发和日冕物质抛射

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Design of Earth Gravity Assist Trajectories for the Coronal Mass Ejections Probe

基于地球引力变轨的日冕探测器轨道设计

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The hydromagnetic nature of solar coronal mass ejections

太阳日冕物质抛射的磁流体力学性质

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Coronal mass ejections and solar particle events

日冕物质抛射与太阳粒子事件

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An absence of sunspots also means an absence of solar flares and their more violent siblings, coronal mass ejections.

黑子的缺失还预示着太阳耀斑的缺席，同时，猛烈的日冕喷发也不会出现。

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The observation of ejections of Comet Hale-Bopp

海尔-波普彗星喷出物的观测

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A mathematical model of dual-objective programming was developed, in which a number of thermal parameters of exhaust gas boiler-turbogenerator system were taken as design variables and investment cost and net electrical power output of the system were taken as two objective ejections.

在建立的多目标优化模型中，将余热锅炉&汽轮发电机组的主要热力参数作为设计变量，选取系统造价和输出电功率作为两个目标函数。

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Numerical simulation of coronal mass ejections between two coronal streamers

两冕流间物质抛射事件的数值模拟

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The Neutral Current Sheet and Its Radiation Pairs of Side Sources in Coronal Mass Ejections

日冕物质抛射的中性电流片及边源辐射对

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Constructing and realizing the computer fast arithmetic for Daya Bay PWR nuclear power station's liquid ejections around the sea area and statistics analysis of the inspected data

大亚湾核电站液态排放在受纳海域中监测数据计算机快速算法的构造与实现

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One telescope aboard SOHO can provide three or four days' warning of major solar events by spotting coronal mass ejections.

通过观测日冕物质的喷发，SOHO上的一台望远镜能提前三到四天预报太阳的重大活动。

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Correlation Between Coronal Mass Ejections and Solar Surface Magnetic Activities

日冕物质抛射和太阳表面磁活动的关系

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Solar Radio Meter Burst and Coronal Mass Ejections

太阳射电米波爆发与日冕物质喷射

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Solar Atmospheric Responses to. Magnetic Flux Eruptions I. A Mechanism for Coronal Mass Ejections

磁通量喷发的大气响应Ⅰ.日冕物质喷射机制

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The occasionality and randomicity of droplet ejections are also attributed to the droplet pulsation resulting from the contact angle hysteresis.

液滴受接触角滞后影响而发生的脉动行为还表现为液滴偶然与随机的弹射。

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Moreover, solar radio microwave bursts which accompany with coronal mass ejections during February 1999 to August 1999 are analyzed.

此外，分析讨论了1999年2月至1999年8月期间与CME共生的太阳微波爆发。

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Observations on Coronal Mass Ejections and Its Associated Solar Activities

日冕物质抛射及相关太阳活动的观测研究

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At least in some flares, these twisted magnetic field loops must become coronal mass ejections.

至少在一些闪焰事件里，这些扭曲的磁场环圈会产生日冕团块喷射。

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