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无球
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  without the ball
     It emphasizes the action decision-making system of the SEU2004 robotic soccer simulation team in mis paper, It divides the action decision-making system into three parts : which made by player controlling the ball the player without the ball and made by goalie .
     本文重点介绍了SEU2004仿真足球队的动作决策系统。 将动作决策模块分成控球队员动作决策、无球队员动作决策和守门员动作决策。
     Proposed are the application of oppotunitiesof the players without the ball in attacking tactics, and ways and inkasuresfor teaching and coaching by analyzing the routes and methods of movementby dttackers without the ball in various positions, and in accordance withthe characteristics of attackers without the ball.
     通过分析无球进攻队员在各个不同的位置的移动路线和方法,根据无球进攻队员移动的特点,提出了在无球队员运用进攻战术的时机,以及教学训练的步骤与方法。
短句来源
     Exploration Analysis of the Running Position Mode of the Players without the Ball in the Game Against High-level Soccer of the World
     对世界高水平足球比赛中无球队员跑位模式的探悉
短句来源
     Basic principles and requirements for guarding the players without the ball in basketball are introduced and some skills and training methods are explained in detail.
     介绍了篮球运动中防无球队员的基本原则、要求,并详细说明了防守技巧和针对性的训练方法。
短句来源
     The technical application of offensive players without the ball has important effect for a basketball team to take the initiatives and to win the game in modern matches.
     现代篮球竞赛中,无球进攻队员的技术运用对本队争取主动,获取胜利起重大作用。
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  “无球”译为未确定词的双语例句
     The FT 3 and value of free golubin sample was 0.72pmol/L and 2.18pmol/L alternatively.
     无球蛋白血样本FT3、FT4 浓度分别为 0 .72pmol/L和 2 .18pmol/L .
短句来源
     4. Through genetic map and clustering analysis, it was regarded the tree of number 1、 2and 3 as none cone variety of Platanus acerifolia and the tree of number 4、5、6 as little cones variety.
     4)通过AFLP分子标记遗传图谱和聚类分析可以看出,1、2、3号为无球单株,4、5号为少球单株。
短句来源
     True FT 3 and FT 4 value may be determined in freegolubin serum sample.
     测定无球蛋白血样本FT3、FT4 能反映出真实浓度
短句来源
     The samples of spherical aberration-free unspherical geodesic lenses were fabricated on the LiNbO3substrates with the sinze of45×20×2.5mm3,the focal Spot half-width measured at the other edge is 2.9μm.
     样品制备在45×20×2.5mm3的铌酸锂衬底上,每片有两个孔径8mm,焦距18mm的非球面无球差短程透镜。 利用670nm波长的半导体激光器端面耦合入样品一端,而在另一端测得焦面光班半宽度为2.9μm。
短句来源
     Discussion on the Body Balance in Movement Skill Without Ball in Modern Basketball
     现代篮球无球移动技术的身体平衡探讨
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  相似匹配句对
     The optical surface of eliminated spherical aberration
     差的光学曲面
短句来源
     Vibration of Momentless Spherical Shells
     壳的矩振动
短句来源
     Hard Alloy Sphere
     硬质合金
短句来源
     Yuan is nothing but wu 无 nonexistence.
     元是
短句来源
     H.
     而H.
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  non-ball
Figure 3 shows the standard deviation plot of the ball groups versus the non-ball groups.
      
Figure 4 shows a histogram of the normalized error values for ball groups and non-ball groups.
      
Our prediction was that the standard deviations for ball groups would be lower than that of non-ball groups.
      
The training set consists of 872 examples of ball and 338 examples of non-ball.
      
Wavelet pre-processing increases both the classification percentage of ball, non-ball and ball occluded with respect ICA pre-processing.
      
  without the ball
Powders were blended in the micro-ball mill without the ball.
      
Grid points that cannot be accessed without the ball overlapping protein are labeled as protein and the rest are considered electrolyte.
      


The primitive Material which the Earth consists of is probably IAB iron meteorite (core of the Earth) and H-group chondrite (mantle of the Earth). When the experimental temperature is higher than 1300℃, noticeable magmatic differentiation took place in the Jilin chondrite, and this is quite similar to the process of the formation of the core and mantle of the Earth. The metal-sulfide components within chondrite would sink to the core. During melting and recry-stallization of the Jilin chondrite the partial FeO...

The primitive Material which the Earth consists of is probably IAB iron meteorite (core of the Earth) and H-group chondrite (mantle of the Earth). When the experimental temperature is higher than 1300℃, noticeable magmatic differentiation took place in the Jilin chondrite, and this is quite similar to the process of the formation of the core and mantle of the Earth. The metal-sulfide components within chondrite would sink to the core. During melting and recry-stallization of the Jilin chondrite the partial FeO in olivine can be reduced and Fe 0 formed. These metal Fe also would move to the core.Some large parent meteorite bodies seem to have undergone such a process leading to the formation of some iron meteorites and achondrites. The Fe-Ni-S phase in the experimental products may serve as a indicator in identifying the cosmic chondrules.

组成地球的初始物质很可能是IAB铁陨石及H群球粒陨石,非均匀吸积形成地球以后,除由岩浆分异作用使幔中金属-硫化物下沉到原始地核外,在还原条件下还有部分Fe是由橄榄石中的FeO还原为Fe°而提供的并加入于地核内.对于大的陨石母体,由于内部加热或其表面受冲击加热而发生熔融和岩浆分异,导致形成某些铁陨石及无球粒陨石或7型岩石类型的球粒岩石.实验产物中的Fe-Ni-S相可作为判别宇宙球粒的标志之一. 我们曾报道过吉林陨石热变质实验研究结果~[1],根据在高温高压条件下吉林陨石的岩浆分异作用,初步探讨了类地行星金属与硅酸盐分离的机制及其核-幔的形成过程~[2].最近,我们对吉林陨石全岩熔融实验产物中的硅酸盐矿物及金属相进行了较系统的电子探针分析和研究.本文试图根据其实验产物的矿物成分特征进一步探讨组成地球初始物质的演化过程及普通球粒陨石与某些铁陨石和无球粒陨石的成因联系.

Having analyzed the experiences of bulb designs at home and abroad, the author designs a satisfactory bulb for a 15000 dwt multipurpose ship which is of block coefficient 0.736: The result of the ship's self-propulsion test has shown that: It can increase 0.4 knots speed in full-load condition compared with the original non-bulb ship and receives the benefit of resistance reducing over the low speed range. The design methods and the bulb effect line given in the paper are a valuble reference for the bulb design....

Having analyzed the experiences of bulb designs at home and abroad, the author designs a satisfactory bulb for a 15000 dwt multipurpose ship which is of block coefficient 0.736: The result of the ship's self-propulsion test has shown that: It can increase 0.4 knots speed in full-load condition compared with the original non-bulb ship and receives the benefit of resistance reducing over the low speed range. The design methods and the bulb effect line given in the paper are a valuble reference for the bulb design.

本文介绍方形系数0.736、载重量15000吨多用途船的球首设计。鉴于中速中型船舶球首设计的资料较少,且难以获得明显的减阻效果,笔者通过综合国内外球首研究经验,成功地对15000吨多用途船选择了优良球首,经船模自航试验证明,该球首在满载时比原无球首船提高航速0.4节,而且在整个低速范围内都有减阻效果。文中给出的设计方法、球首效果线等对球首设计与研究具有一定的参考价值。

40Ar/39Ar age spectra of meteorites are very useful data for the study on the collisional events in parent bodies of meteorites. Turner (1969) has calculated theoretical 40Ar/89Ar release profiles based upon diffusion loss of 40Ar* from a log normal distribution of spherical grains brought about by the effect of a discrete reheating events subsequent to the original crystallization and cooling of the object. In the ideal case the time of the degassing event is given by the 40Ar/39Ar ages found for gas released...

40Ar/39Ar age spectra of meteorites are very useful data for the study on the collisional events in parent bodies of meteorites. Turner (1969) has calculated theoretical 40Ar/89Ar release profiles based upon diffusion loss of 40Ar* from a log normal distribution of spherical grains brought about by the effect of a discrete reheating events subsequent to the original crystallization and cooling of the object. In the ideal case the time of the degassing event is given by the 40Ar/39Ar ages found for gas released at the lowest temperatures, and the 40Ar/39Ar ages found for gas fractions released at the higher temperatures should provide a minimum age for the original cooling of the object. Many chondrites show disturbed 40Ar/39Ar age spectra, similar to those predicted from the Turner model, and Bogard (1976) was gave a summary of such studies. Following the investigations on fifty-five meteorites 40Ar/39Ar collisional ages and the exposure ages of meteorites, the relation between collisional ages and types of meteorites is found. And the collisional events are divided into nine stages as follows.Stage Ⅰ: 4400-4100 Ma, Pre-lmbrium Event. It concerns mainly Ca-rich achondrites such as Bununu, Petersburg and Pasamonte, and one enstatite chondrite Abee.Stage Ⅱ: 4000-3900 Ma, Imbrium Event, animportant evolution stage for parent bodies of meteorites.Stage Ⅲ: 3800-3000 Ma, it is related to Ca-rich achondrites mainly, for example, Stan-nern, Kapoeta, Bununu, Cachari, and one iron meteorite El Taoco.Stage Ⅳ: 3000-2100 Ma, concerning H and L chondrites only, such as Ucrea, Monore, Malakal, Rose city, Kirin (Jilin)-1 and Xinyang.Stage Ⅴ: 1600-1300 Ma, it is related to Ca-rich achondrites only, for example, Malven, Lafayette and Nakhla.Stage Ⅵ: 1100-600 Ma, it concerns ten stony meteorites and stony iron meteorites, and the exposure of iron meteorites.Stage Ⅶ: 540-470 Ma, it is a very important collisional event on L and H chondrites. Thirteen L chondrites and two H chondrites (Kirin-2 and Kirin-5) which recorded the collisional event were found.Stage Ⅷ: 420-200 Ma, concerning seven ordinary chondrites and one achondrite Sher-gotty.Stage Ⅸ:<65 Ma, an important exposure event of stony meteorites, and a collisional event of H and L chondrites.The stage Ⅱ, Ⅶ and Ⅸ are the important evolution stages in parent bodies of meteorites. Stage Ⅰ, Ⅱ and Ⅲ (the collisional ages more than 3.0 Ga) concern mainly Ca-rich achondrites. The collisional ages of all chondrites are less than 3.0 Ga. And the exposure ages of iron meteorites are larger than those of stony irons which are in turn larger than those of stony meteorites.

~(40)Ar/~(39)Ar年龄谱是研究陨石冲击事件的重要资料。根据对55块陨石~(40)Ar/~(39)Ar冲击年龄和陨石暴露年龄的分析,发现陨石的冲击年龄与陨石类型之间存在对应关系。据此,将陨石冲击事件划分为九期。其中3900—4000Ma、470—540Ma和小于65Ma是陨石母体的三个重要演化阶段。阶段Ⅰ、Ⅱ和Ⅲ(冲击年龄大于30亿年)主要涉及高钙型无球粒陨石。所有球粒陨石的冲击年龄均小于30亿年。陨石暴露年龄因类型而异,铁陨石最大,石铁陨石次之,石陨石最小。

 
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