Explosion point

The thermal stability of TEX and its mixtures respectively with HMX and RDX was characterized by VST,Bourdon type glass manometer test and critical temperature determination,and their theoretical half lives were calculated.

采用真空安定性试验(VST)、布氏压力计法、5秒爆发点等实验方法对TEX以及TEX分别与HMX、RDX的混合物的热安定性进行了表征,并对其半衰期进行了理论推算,结果表明: TEX具有很好的热安定性能; RDX、HMX对TEX的热安定性能几乎无影响,彼此之间具有良好的相容性。

An Outbreak of HEV Among Aged People in a Nursing Home;

某敬老院一起戊型病毒性肝炎爆发的调查

An investigation and analysis on an outbreak of norovirus diarrhea in a community in Dongguan City;

东莞市一起社区诺如病毒腹泻爆发调查分析

An epidemiological study on an outbreak of viral meningitis caused by ECHO virus 30 in Lianyungang;

连云港市一起ECHO_(30)病毒性脑膜炎爆发流行病学调查

Composite analysis of evolution of tropical circulation associated with summer monsoon onset in the South China Sea;

伴随南海季风爆发热带环流演变的合成分析

The regional durative rainstorm during pre-rainy season over South China is defined and its climatic distribution features before and after the onset of South China Sea summer monsoon are studied using daily rainfall data of 175 stations in Guangdong and Guangxi provinces.

对南海夏季风爆发前后区域持续性暴雨的气候分布特征的分析发现,季风爆发前持续性暴雨频数从60年代至今呈现出正态分布的年代际变化特征,而季风爆发后的区域持续性暴雨频数变化则几乎相反;广东省前汛期区域持续性暴雨降水明显比广西强。

Generally speaking,the South China Sea summer monsoon(SCSSM) onset marks the arrival of the East and Southeast Asian summer monsoon and the beginning of the major rainy season in these regions.

利用高分辨率的区域气候模式(RegCM-NCC)对南海夏季风爆发进行模拟研究。

Physical Explanation to SU UMa-type Dwarf Nova s Explosion and Super-explosion;

SU UMa-type矮新星爆发和超爆发的物理解释

In this paper, author has made a further study of [1,2] such properties for a conserrative and nonregular Markov chains in single exit case, which can be expressed by the properties of the first hit and the first explosion.

我们将[1,2]性质进行了推广,对于保守单流出非规则的Markov链,研究了该过程首次爆发后关于有界集合B的反复击中以及反复爆发的若干性质。

Woosley and using an equation of state improved by the authors, the probable implications of progenitors on supernova collapse, shock wave transport and explosion are investigated by numerical simulation with our own computer program.

对其结果进行分析比较，考察前身星对超新星的坍缩、激波传输和爆发等过程的影响。