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截止线
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  cut-off line
     The pulsars with long pulse nulling distribute near the radio cut-off line and constitute a line nearly parallel to the cut-off line.
     发现缺脉冲现象显著的脉冲星分布在射电辐射的截止线附近,组成一条近于和截止线平行的直线。
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  closing line
     This paper has discussed the light-shape quality problem of E-type automobile headlight, such as unsuitable angle, vageu light - dark closing line and diffusing lightshape. The paper has also pointed out the relation between the internal geometric size and light-shape quality of E-type bulb.
     本文论述了E型汽车前照灯光形存在的角度不合格、明暗截止线不清、光形散射等方面的质量问题,指出了E型灯泡的内部几何尺寸与其光形质量的密切关系。
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  “截止线”译为未确定词的双语例句
     3. It is better to combine Kuno's sequential sampling method with Iwao's one. The accumulated number of the spider mite in Iwao's model can be determined byT_(?) (n)=3n±6.6283n~(1/2),and the stop critical number in Kuno's model determined byT_n=2.1991/D~2-(0.5337/n)
     序贯抽样可依Iwao法确定的两条截止线T_0(n)=3n±6.6283n~(1/2)女和据Kuno法确定的最大抽样数结合起来使用。
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     Calculation of the High Beam Shadow Line Height of Headlamp Leng Yongjie (Jinan Qingqi Suzuki Motorcycle Co. ,Ltd. )
     前大灯近光明暗截止线高度的计算
短句来源
     The sample size requirements and sequential sampling plans of fixed levels with precision were determined by utilizing estimated variance/mean relationship obtained from Taylor′s power law regression.
     通过Tay-lor的指数回归式参数确定了在一定精确度水平下的理论抽样数和序贯抽样公式:理论抽样数n=5.3641x-0.64D2,序贯抽样截止线Tn=13.8D3.125·n0.563。
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  相似匹配句对
     ONLINE
     在线
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     TECHNOLOGY ON LINE
     成果在线
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     Calculation of the High Beam Shadow Line Height of Headlamp Leng Yongjie (Jinan Qingqi Suzuki Motorcycle Co. ,Ltd. )
     前大灯近光明暗截止线高度的计算
短句来源
     Change in polarization direction of laser beam may change the cut-off order and spectrum intensity of HHG simultaneously.
     不同的激光偏振方向会导致高次谐波的截止频率和谱线强度的变化.
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  dead line
HIPERLAN architecture for data transfer is based on a mix of two main mechanisms: hierarchically independent priority levels and an earliest dead line first algorithm.
      
Applications received after the dead line will be processed for the following term.
      
A voltage of zero thus implies a dead line or terminal.
      
All new, incoming fall freshmen who apply for housing by the dead line are guaranteed housing in the residence halls.
      
Dead line for applications is 15 February 1984 or until the position is filled.
      
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  cut-off line
However, in a minority of cases only Ig levels were above the cut-off line: this was true for IgM in 11/63 (17%) cases and for IgA in 14/63 (22%) of cases but none of the tested infants was anti-A60 IgG ELISA positive.
      
This method is also used to easily compare two equations of motion of a slender vortex filament: the one obtained in an ad-hoc way by a cut-off line-integral technique and the other derived from the Navier-Stokes equations by Callegari and Ting.
      
An area of the black line on the right of a cut-off line is the percentage of positive cells.
      
Furthermore, some firms may leave the sample set because of shrinkage in size; the Basic Survey has a cut-off line in size as mentioned above.
      
Figure 1 Impact of cut-off line choice on correct identification of anomalies.
      
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83 pulsars are statistically studied in this paper. The main results are as follows: (1)Taking the ratio λ of the loss rate of rotational energy to the radio luminosity of pulsars as a parameter of classification, we divide the 83 pulsars into 3 categories. This is not only necessary to the study of the statistical relationship between the luminosity and the magnetic energy in various regions, but it may also be a better method of classification. It may be seen from the plots of P-P, L_(radlo)-P and L_(radlo)-t...

83 pulsars are statistically studied in this paper. The main results are as follows: (1)Taking the ratio λ of the loss rate of rotational energy to the radio luminosity of pulsars as a parameter of classification, we divide the 83 pulsars into 3 categories. This is not only necessary to the study of the statistical relationship between the luminosity and the magnetic energy in various regions, but it may also be a better method of classification. It may be seen from the plots of P-P, L_(radlo)-P and L_(radlo)-t that different categories of pulsars have different evolutionary tracks and physical properties. The evolutionary tracks of the 3 categories of pulsars by the λ classification are something similar to those of the model proposed by Lyne et al.(1975) which involves a secular decay of magnetic dipole moment. Therefore the various categories of pulsars may reflect the fact that the different categories of pulsars have different time constants of decay, or the initial values of the magnetic moments were different at birth. There are no apparent properties on the above mentioned plots for the morphological classification by the integrated pulse profiles(S,D and C)(Taylor and Huguenin, 1971). (2)The radio luminosities of pulsars of various categories are all closely correlated to the magnetic energies and“twining”magnetic energies at the light cylinder, and not correlated to the magnetic energies at the surface of the neutron star. This shows that the local radiation regions are in the vicinity of the light cylinder. These magnetic energies may be the energy sources of pulsar radiation. (3)Some pulsars in the right region of the plot of P against P constitute a cut-off line of radio radiation, whose slope is just—4.So that it is a line for which the“twining”magnetic energy PP~(-4)is constunt, It is closer to the observational results than the cut-off line, proposed by Lyne et al.(1975), for which PP~(-5)is constant. This result gives support to the accumulatimi and release of energy in the vicinity of the light cylinder.

本文对83颗脉冲星进行了分类统计研究。主要结果如下: 1.采用转动能损失率与射电光度的比值作为分类参数可以较好地反映不同类型脉冲星的物理特性和演化方式。 2.由于各类脉冲星的射电光度和光速圆柱附近的磁能之间都有着相关系数较高的回归关系,而射电光度和表面磁能之间却不相关,由此推论脉冲星辐射部位很可能在光速圆柱附近。 3.在周期变率户和周期P的关系图上,光速圆柱附近的“缠绕”磁能PP-4的某一临界值可作为射电辐射的截止线,它比Lyne等提出的光速圆柱处的磁能户PP~(-5)作为射电辐射截止线更接近观测事实。

In this paper, the pulsars with pulse nulling are regarded as a subtype to be investigated. The pulsars with long pulse nulling distribute near the radio cut-off line and constitute a line nearly parallel to the cut-off line. From this paper, it can also be seen that the magnetie field at the distance of light cylinder is rather low and the rate of energy loss is rather small for the pulsars with long pulse nulling. The possible reason for the pulse nulling is discussed.

本文把呈现缺脉冲现象的脉冲星作为一种次型来进行研究。发现缺脉冲现象显著的脉冲星分布在射电辐射的截止线附近,组成一条近于和截止线平行的直线。此外,这种脉冲星还有如下的特点:它在光速圆柱距离处的磁场偏小,能损率也偏小。文中讨论了缺脉冲产生的可能原因。

In this paper,it is supposed that three quasars laying out the cut-off curve of the QSO's θ—Z diagram namely 4C_(48·28),4C_(09·37) and 4C_(29·68) have gravitation redshift produced by the field of the neutrino astronomical objects (NAO).It is estimated that the time of the for_ mation of the NAO is earlier than 10~7 years (the nuiverse age) and the mass of neutrino heavier than 1ev.

本文假设类星体θ—Z图截止线外的三颗星存在引力红移,认为这种红移由中微子天体(NAO)引起。从而给出类星体θ—Z图截止线外的反常分布一种解释,指出这些类星体可能位于NAO中。同时,推断出NAO的形成时间早于10~7年(宇宙时),并且中微子的质量约大于1ev。

 
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