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fluxes
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     and the fluxes and residence times for NH4-N, NO3-N, NO2-N were 33.9, 401.0, 15.8 g·atN/s, and 3.84, 3.96, 4.41 days, respectively.
     NH_4-N,NO_3-N,NO_2-N的通量和停留时间分别为33.9,401.0,15.8g·atN/s和3.84,3.96,4.41d。
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     The permeation fluxes of hydrogen and nitrogen through the composite membrane were 7.9×10~(-3)m~3/(m~2·s) and 2.1×10~(-6)m~3/(m~2·s)respectively.
     在350℃和0.3 MPa下,氢气和氮气通过膜的渗透通量分别为7.9×10-3m3/(m2.s)和2.1×10-6m3/(m2.s)。
短句来源
     The nitrogen and water fluxes of the asymmetry membrane are 24.69×103 m3/(m2h) and 1.87×103 m3/(m2h),per MPa;
     非对称膜单位压力降(1 MPa)下的氮气通量和水通量分别为:24.69×103m3/(m2h)和1.87×103m3/(m2h);
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     Relationships between CO_2, CH_4 and N_2O Concentrations and Fluxes in Antarctic Tundra
     南极苔原近地面CO_2、CH_4、N_2O浓度和通量的相互关系
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     Impat of Reclamation of Grassland on the Fluxes of CO_2, CH_4 and N_2O in Temperate Grassland Ecosystem
     农垦对温带草地生态系统CO_2、CH_4、N_2O通量的影响
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  “fluxes”译为未确定词的双语例句
     Study on Related Basic Theories of Continuous Casting Mold Fluxes and Application in Industry
     连铸结晶器保护渣相关基础理论的研究及其应用实践
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     Structures and Turbulent Fluxes of Atmospheric Boundary Layer over Heterogeneous Surface
     非均匀边界层结构和湍流通量特征的研究
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     INITIAL STUDY OF HIGH-BASIC SINTERED FLUXES——THE BASICITY AND STRENGTH OF THE FLUXES AND THE DIFFUSIBLE HYDROGEN CONTENT OF DEPOSITED METAL
     高碱度烧结焊剂的初步研究——碱度、强度和熔敷金属的扩散氢含量
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     A Research on the Production of the SH-11 and SH-12 Soldering Fluxes
     SH-11和SH-12锡焊助焊剂的研制
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     Study on Fluxes Used in Flux Growth of KTP Crystals
     熔盐法生长KTP晶体的助熔剂研究
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  相似匹配句对
     SELECTION OF FLUXES FOR ALUMINUM BRAZING
     高温铝钎剂的选择
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     Solid Fluxes for Aluminium and Its Alloys
     铝及其合金用固态熔剂
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  fluxes
This paper deals with asymptotic analysis of a parabolic system with inner absorptions and coupled nonlinear boundary fluxes.
      
Relations between carbon dioxide fluxes and environmental factors of Kobresia humilis meadows and Potentilla fruticosa meadows
      
There exists a negative correlation between the vegetation albedos and the carbon dioxide fluxes.
      
The fluxes of carbon dioxide generated during this degradation were deduced from differences in the carbon isotope abundance ratios of glucose δ13C = -11.4 per mil) and SOM δ13C = -27.01 per mil).
      
2D [1H,13C] NMR study of carbon fluxes during glucose utilization by Escherichia coli MG1655
      
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By means of two adiabatic in-variants of relativistic charge particles, some variations of the structure in the outer radiation belt during the main phase of a magnetic storm are discussed. It is supposed that the main phase is caused by the ring current of the "storm belt" situated outside the centre of the radiation belt and consisted of solar plasma penetrating into the magnetosphere. The calculation had been proceeded for electrons with initial energy W=20Kev and W=1 Mev respectively. It is shown that during...

By means of two adiabatic in-variants of relativistic charge particles, some variations of the structure in the outer radiation belt during the main phase of a magnetic storm are discussed. It is supposed that the main phase is caused by the ring current of the "storm belt" situated outside the centre of the radiation belt and consisted of solar plasma penetrating into the magnetosphere. The calculation had been proceeded for electrons with initial energy W=20Kev and W=1 Mev respectively. It is shown that during the main phase of a magnetic storm the electrons drift outward, the pitch angles are decreased, but the height of the mirror points is increased. This means that the excitation of aurora during the main phase can not be attributed to the precipitation of electrons into atmosphere caused by the slow change of geomagnetic field. It is also shown that the variation of counting rate during the main phase is produced primarily by the decrease of the density of electrons in accompanying with the expansion of the tubes of force and by the electrons deceleration, the changes in the dis tribution of electrons fluxes along the lines of force could explaned in terms of the deceleration related to the pitch angles. The results obtained agree fairly well with the observation by Explorer Ⅵ.

本文利用相对論带电粒子的两个寝渐不变量,討論了磁暴主相期間外輻射带中心結构的变化。作者认为磁暴主相是由“磁暴带”环电流所产生。“磁暴带”假設位于外輻射带中心之外,它是太阳等离子体穿入磁层后形成的。本文对初始能量W=20Kev和W=1Mev的电子分別进行了計算。 結果表明,在磁暴主相期間电子向外漂移,其赤道投擲角減小,但镜点离地面距离增高。因此,主相时所观測到的极光,并不是由于地磁場的平緩下降使小投擲角电子注入大气层而形成的。此外,計数率降低的主要原因是由于力管截面膨胀造成的粒子密度減小以及电子減速,而电子減速与投擲角有关,由此决定了电子通量沿磁力线分布的变化。以上結果与探险者6号(Explorer Ⅵ)的观測一致。

In this paper, We have calculated the r-ray fluxes from synchrotron self-Compton for a number of representative cases with two methods: an approximate method and a more accurate method. From a comparison of the results from them, We find that the results are close to each other in a great range of energy.

对于一些有代表性的情形,本文同时用近似方法和比较准确的方法计算了由同步加速辐射的自康普顿效应所产生的γ辐射流。得到:在大部份能量范围内,由两种方法得到的结果很相近。

In this paper, We have calculated the r-ray fluxes from synchrotron self-Compton for a number of representative cases with two methods: an approximate method and a more accurate method. From a comparison of the results from them, We find that the results are close to each other in a great range of energy.

对于一些有代表性的情形,本文同时用近似方法和比较准确的方法计算了由同步加速辐射的自康普顿效应所产生的γ辐射流。得到:在大部份能量范围内,由两种方法得到的结果很相近。

 
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