质量范围的英文

• mass range
• quality ranges

• "质量"英文翻译    mass
• "范围"英文翻译    scope; limits; extent; bound ...
• "适当环境空气的质量范围" 英文翻译 :    desirable range of quality （of the ambient air）
• "变量范围" 英文翻译 :    range of a variable; range of variables; scope of a variable; variable range
• "测量范围" 英文翻译 :    i trument range; instrument range; measurement range; measurementrange; measuring range; range of measurement; surveying range
• "产量范围" 英文翻译 :    capacity range
• "常用量范围" 英文翻译 :    usual dose range
• "称量范围" 英文翻译 :    weighing range
• "光量范围" 英文翻译 :    lcp
• "剂量范围" 英文翻译 :    dosage range; dose range
• "进给量范围" 英文翻译 :    range of feeds
• "流量范围" 英文翻译 :    flow range; flow-rate range; range of flow
• "耐量范围" 英文翻译 :    tolerance range
• "能量范围" 英文翻译 :    energy interval; energy range; energy region
• "能量范围, 能程" 英文翻译 :    energy range
• "曝光量范围" 英文翻译 :    exposure range
• "容量范围" 英文翻译 :    containment; range of capacity
• "容许量范围" 英文翻译 :    tolerance domain
• "输送量范围" 英文翻译 :    range of throughput; throughput range
• "音量范围" 英文翻译 :    sound range; volume range
• "电平测量范围" 英文翻译 :    level range
• "剂量范围研究" 英文翻译 :    dose-raging studies; dose-ranging study
• "静校正量范围" 英文翻译 :    statics range
• "输出流量范围" 英文翻译 :    output flow range
• "套管重量范围" 英文翻译 :    casing weight range

• Our company can provide the following main specifications
  目前，我司可供的主要质量范围有：
• 2 . the abundance distributions of the sbl component part with 92 a132 are nearly similar to the solar pattern at any metallicity
  S _ ( ml )分布与太阳系有差异，但对于质量范围92 a 132 ，任何金属丰度下分布与太阳系相应分量大体相似。
• We study the code model characteristic of videos , analyse the characteristic of mpeg data structure and similarities and differences of forms of avi video . the method which compresses the information of an image and the differences of images is adopted to reach the high compression ratio . mpeg compresses algorithms as the international standard , is supported together by many computer platforms now , have better compatibility than avi video
  论文首先简要地介绍了课题背景和当前的研究状况，研究了视频编码模型特点，分析了mpeg - 2数据结构特点和avi视频格式的异同，在同等的视觉质量范围下mpeg - 2采用有损压缩方法减少运动图像中的冗余信息从而达到高压缩比，因此mpeg - 2压缩算法作为国际标准，被许多的计算机平台共同支持，较avi视频具有更好的兼容性。
• This letter aiming at this respect , hints for neutron capture element are derived : 1 . based on the adopted galactic evolution scenario , together with the three - zone multi - phase model , observational features of the solar vicinty region can be well reproduced . among those are particuly g - dwarf problem . the g - dwarf problem in halo and thin - disk can be solved
  本文正是从这方面着手，对中子俘获元素进行了研究，得到如( 1 ) r过程元素核合成产量随着超新星前身星的质量的增加而单调增加， r -过程核合成场所是sn ，质量范围是18m _ m 50m _ ，这与mathews 、 tsujimoto和travaglio等人的结果完全不同。
• Thus the cumulative consequence of galactic chemical evolution starting from low metallicity agb stars , namely , the average abundance patterns of sbh part with 140a204 ( or the snl component part with 92a132 ) in different metal conditions , should be similar ( ornearly similar ) to the corresponding solar s - bajn component
  低金属丰度条件下，由于中子辐照量随金属丰度的降低而升高， s _ ( ml )产量低于s _ ( mh ) 。虽然s _ ( ml )分布与太阳系有差异，但对于质量范围92 a 132 ，任何金属丰度下分布与太阳系大体相似。
• Our yields increase with the mass of the progenitor main - sequence stars . massive stars ( i . e . 18m < m < 50m ) is the primary sites of the neclearsynthesis of the r - process and can explain the galaxy chemical evolution . 3 . we present formula to calculat the r - process galactic chemical evolution of ba peak elements . this formula contains metallicity abundance and point out the relation of the ba peak elements and disscuss the effect of various mass supersnova . besides , our formula can be confirmed by a lot of observations
  由此可以解释以下观测事实: ( l ) mg ， eu均产生于snh星，但质量范围不同，在高质量( > 20 ) eu的产量高， mg的产量(相对于太阳) ，导致晕星中eu / mg > 0 ，而产生mg的质量范围较大，致使在厚盘的晚期较小质量超新星也开始对mg有贡献，而这些星对eu的贡献很小，致使在厚盘星中eu / mg < 0 ，在厚盘中eu / fe随金属丰度的升高而降低，仁mg / fe随金属丰度的升高而不变

• 质量范围的日语：しつりょうひてい