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Home > chinese-english > "mass ejection" in English

English translation for "mass ejection"

质量抛射

Related Translations:
ejection trajectory:  弹射轨迹
ejection strok:  顶出行程
cassette ejection:  记录器盒的弹射
stabilized ejection:  稳定弹射
ejection side:  顶出侧
ejection grid:  顶出栅
ejection stress:  出坯应力
ejection escape:  弹射离机弹射逃逸
ejection trainer:  弹射训练器
high ejection:  高空弹射
Example Sentences:
1.Progress of a coronal mass ejection observed over an eight hour period on 5 - 6 august 1999
这六帧图片捕捉了在1999年8月5日至6日期间,历时8小时的日冕抛射现象。
2.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。
3.Since sunspot number is closely related to solar activities like flares and coronal mass ejection , the sun might have entered a low - activity state for a rather long period of time during these minimums
由于太阳黑子数目与如耀斑和日冕抛射等太阳活动关系密切,在上述太阳黑子极小期内,太阳的活动可能沉寂了一段长时间。
4.Such special arrangements are probably capable of bringing about a flare , but these mechanisms cannot account for all the observations , especially the tendency for coronal mass ejections to accompany large flares
此类特殊的安排或许可以产生日焰,但这些机制不能够解释所有的观测现象,特别是日冕团块喷射为何常伴随大型日焰发生。
5.Wang , s . , zheng , h . n . , wang , x . h . , 1997 , magnetic reconnection and mechanism for the formation of coronal mass ejection in the coronal current sheets , research digest in memory of zhao jiuzhang , scientific press , beijing , 205
王水,郑惠南,王小虎, 1997 ,日冕电流片中的磁场重联和日冕物质抛射的形成机制,赵九章纪念文集(叶笃正主编) ,科学技术出版社,北京, 205
6.Although scientists have long sought to figure out what drives both flares and the coronal mass ejections that accompany many of them , only in the past decade or so have observations been good enough to reveal their intricacies and to elucidate the physical mechanism behind them , thanks to new technologies introduced during the 1990s
虽然科学家早就想要搞清楚,究竟是什麽驱动了日焰以及经常随之而生的日冕团块喷射,但直到最近10年左右的观测结果,才精良至足以揭露它们错综复杂的样貌,并阐明背后的物理机制,这得归功于1990年代才引入的新技术。
7.More and more researches have shown that most of the intense geomagnetic storms are caused by fast coronal mass ejections in interplanetary space ( icmes ) . though the ace satellite can provide solar wind data in almost real time for prediction of geomagnetic storms , the time interval is too short ( shorter than 30 - min ) for effective predictions of major geomagnetic storms
位于拉格朗日点的ace卫星可以提供近实时的太阳风数据,但依据ace卫星太阳风数据进行地磁暴预报,时间的提前量非常有限,对于大地磁暴,这个时间提前量往往不超过30分钟,这样的时间提前量对于实际应用来说,是不能令人满意的。
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