初始分布的英文

• initial distribution

• "初始"英文翻译    initial
• "分布"英文翻译    distribute; spread; scatter; ...
• "初始分布体积" 英文翻译 :    initial distribution volume
• "初始分程序" 英文翻译 :    original block
• "初始分离" 英文翻译 :    primary partitioning
• "初始分组" 英文翻译 :    original packet
• "初始分解温度" 英文翻译 :    temperature of initial decomposition
• "初始年龄分布" 英文翻译 :    initial age distribution
• "初始温度分布" 英文翻译 :    initial temperature distribution
• "初始质量分布" 英文翻译 :    initial mass distribution
• "开始分" 英文翻译 :    starting score
• "初始" 英文翻译 :    initial
• "创始分录" 英文翻译 :    initial entry
• "开始分程序" 英文翻译 :    begin block; beginning block; beginning-block
• "开始分录" 英文翻译 :    opening entry
• "起始分界符" 英文翻译 :    start delimiter
• "起始分裂" 英文翻译 :    original fission
• "原始分解" 英文翻译 :    primary decomposition
• "原始分类图" 英文翻译 :    prime sort chart
• "原始分录" 英文翻译 :    original entry; prime entry
• "原始分录簿" 英文翻译 :    book of original entry
• "原始分数" 英文翻译 :    raw score; raw-score; row score
• "原始分数法" 英文翻译 :    raw score method
• "原始分异" 英文翻译 :    primary differentiation; primordial differentiation
• "原始分子" 英文翻译 :    primary molecules

• Beam halo - chaos for five different initial ion distributions is effectively controlled by a logarithm - function controller based on the variable
  结果显示，新的控制方法对强流加速器中5种初始分布的离子束均有较好的控制效果。
• An explicit solution for the probability distribution as a function of the time and position in the master equation is obtained when the substeps between arbitrary adjacent states in a single period are equal for the molecular motor
  并取得了如下成果： 1计算了分子马达在等间距跃迁情况下，当给定初始分布时，任意位置任意时刻主方程中几率分布的解析表达式。
• A simple model for primary breakup of energetic liquid jets was established using unstable wave theory . based on the jet - embedding method , the jet - core shape , the distribution of jet velocity and the primary distribution of liquid drops were computed
  使用不稳定波理论，建立了射流初始破碎的简化模型，采用射流嵌入法( je )进行了数值计算，得到了hy911射流核形状、速度分布以及液滴尺寸的初始分布。
• The integrands in the dispersion equation are not integrable in general , so we used the asymptotic expansion solution to analyze the behavior of the dispersion relation at the singularity and mapped the dispersion relation curves approximately the system composed of collisionless particles which obey maxwellian distribution or all kinds of degenerate distribution , even in their mixture system , their dispersion relation are analogous
  一般来说，色散方程中的被积函数都是难以求积的，本文是用函数逼近法分析色散方程在奇点处的行为，并大致划出色散关系曲线。由无碰撞粒子组成的系统，不管初始分布是maxwell分布还是各种简并分布，甚至是这些分布的混合体，色散关系都是相似的。
• On the basis of this , we selected rms as feedback variable and constructed the controller g : add this controller to the right of ion radial self - edlctric force equation like equation ( 1 ) . we simulated the motion of ion beam by using muti - paticle code ( partice - in - cell ( pic ) code ) . the results demonstrated that the beam halo of five different initial distribution is eliminated well under the same controller . the halo intensity of k - v distribution , water - bag distribution and parabolic distribution and be reduced to zero . in the case of 3 - sigma distribution and full gauss distribution , the result is agree with minimum limitation ( 10 " ) of halo intensity of factual high intensity accelerator
  在此基础上，选择a为控制变量，构造延迟反馈控制器g ： g （ s glrrms （ s ）一rms （ s ） （ 2 ）同（ l ）式一致，将此控制器函数加在粒子径向所受束自生场力方程的右边。利用多粒子数值模拟程序（ pic ）进行了控制试验。模拟结果表明，用同一个控制器和同一个控制参数即可实现五种不同初始分布情况下的束运一混饨的有效控制。
• Comparing with the current observations , which include the number density distribution in space , mass function , etc . , the so - called standard modes for both the power law and gaussian cluster initial mass functions are selected among many runs of simulations . the deviation from the standard modes , which is resulted from the change of the parameter for the initial conditions , is discussed in detail . the discussion of the model parameters is also presented although they are adopted as the typical values based on previous work
  对应一定的初始分布我们发现无论是幂律的还是对数高斯的球状星团初始质量谱经过长时间的动力学演化都会得到和现在银河系观测到的球状星团系统相符的对数高斯的质量分布；动力学演化会明显地改变球状星团系统的空间密度分布，靠近银心区域的球状星团瓦解得更多；经过动力学演化后的球状星团速度分布函数在靠近银心的区域明显得不同于初始分布，初始拥有较大轨道偏心率的球状星团更容易瓦解。
• Supposed that the fluid in all the fields will accomplish a transport in down - flow distance a z , the flow in trickle - bed is a m step markov process , where m = z / z ( z - the height of trickle - bed ) . according to the theory of random process , the statistic of the markov process will be calculated out from the original distribution and state - transport matrix
  假定液体从床层上端面向下流过z距离后，处于各区的流体就实现了一步转移，则可将床内液体的流动视为从一个初始分布开始，经过m步( m = z z ， z为床层高度)转移的状态离散、滴流床流率分布的模拟与整流时间离散的markov过程。

• 初始分布的日语：しょきぶんぷ