抛射

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

线阵CCD图像减影技术实现抛射物体轨迹实时检测

Linear CCD and image-subtraction analysis to detect projectile motion in real time

1980年9月8日的3B级耀斑及物质抛射

A 3B Flare on SePt.8 in 1980 and Its Mass Ejection

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 .

方法制备了含抛射剂的两相INS气雾剂，并用HPLC方法测定其每揿剂量。

METHODS Two phase INS aerosol in propellant system was prepared and the amount of insulin delivered per actuation was determined by HPLC method .

对高度和时间的检测，采用了线阵电荷耦合器件（CCD）为图像传感器进行摄像并采用图像减影的方法识别抛射物体。

Two sets of linear charge coupled device ( CCD ) cameras were used with the image subtraction technique to determine the heights and time above mentioned .

球罐BLEVE碎片抛射的Monte-Carlo分析

Monte-Carlo analysis of fragments projectile from spherical tank BLEVE

用Matlab从阻力系数和物体质量对斜抛运动的轨迹和最大射程抛射角影响方面进行数值研究和分析。

Applying matlab , in this paper the number research and analysis have been made in the aspect that the air resistance coefficient and the object mass affect the projectile motion .

大气气溶胶中NO￣－＿3、SO￣（2－）＿4研究对我国逐步淘汰医用气雾剂所用CFCs抛射剂的建议

THE STUDIES OF AND IN AEROSOL Suggestion on Phasing out CFCs Propellants from Medical Aerosol in China

研究了抛射曲线问题实验设计中的演示部分，将数学模型和计算机演示的flash技术作为演示实验的重要部分。

In this paper , demonstration part of designing experiment about curve of projectile is studied . Math model and Flash technology are taken as an important part in the demonstration experiment .

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 .

大耀斑爆发的Hα初始亮点，双带出现，环系形成，亮物质抛射和吸收冕珥等现象同3.2cm射电流量的变化在时间上有较好的对应关系。

During the major flare , the two-ribbon appearance , loop system formation , mass ejections and their flows back to the chromosphere had a good correspondance in time to the peaks of the 3.2 cm radio flux curve .

球罐BLEVE碎片抛射的危害性研究

Research on Hazard of Fragments from Spherical Tank BLEVE

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 .

星体经过物质抛射后，核能耗尽的恒星质量超过3M⊙，则此星体将继续坍缩成黑洞。

After the process of matter ejection stellar body will continue collapsing into black hole if the mass of the nuclear-energy-exhausted star is more than 3 MQ .

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 .

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 .

基于电偏转抛射式快速成型（RP）工艺方法是通过电场控制带电颗粒的运动轨迹实现分层截面的成型，作者开发了电偏转的抛射式RP工艺的仿真系统。

Based on the electrostatic deflection spraying , the rapid prototyping ( RP ) is to form layered sections and make the prototype or part layer-by-layer by the deflection spraying of electrically charged powder granules passing through the electrostatic field .

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 ) .

现在常用白光日冕仪的观测来研究日冕物质抛射的传输和演化过程，因而如何恰当地理解白光日冕仪中的CME的观测特征对太阳和空间物理领域的许多相关研究至关重要。

Observations of white-light coronagraphs are widely used to study the propagation and evolution of CMEs , and thus how to properly understand CMEs viewed in white-light coronagraphs is crucial to many relative researches in solar and space physics .

肺部给药系统中，干粉吸入器（DPI）一直是很受关注的一种给药装置，不需要氟利昂作为抛射剂的优点使其发展迅速。

Dry powder inhaler ( DPI ) is always popular in pulmonary drug delivery system . It develops so rapidly as a result of avoiding problems inherent in the use of propellant gases ( Freon ) .

虽然证据显示SN1979C形成的是一个新兴黑洞，另外一个有趣的假设认为，它可能是一个年轻的，快速旋转的中子星，强大的波云风抛射出高能量粒子也可能产生强x射线。

Although the evidence points to a newly formed black hole in SN 1979C , another intriguing possibility is that a young , rapidly spinning neutron star with a powerful wind of high energy particles could be responsible for the X-ray emission .

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 .