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通量峰
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  flux peak
     2.the ion O+ exists in larger geo-space and the flux peak is less prominent when Kp=3-5 than that when Kp=0;
     (2)磁扰动时,O+离子占据的空间范围较磁宁静时大,通量峰较不突出;
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  相似匹配句对
     In addition,there also exist C=C vibra tion peak as the result of the de-hydrogen chloride reaction.
     C振动
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     The decline of membrane flux
     膜通量衰减
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     On the Teaching of Flux
     关于通量的教学
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     The Peak Type of Tailed Peak
     拖尾的类型
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     2.the ion O+ exists in larger geo-space and the flux peak is less prominent when Kp=3-5 than that when Kp=0;
     (2)磁扰动时,O+离子占据的空间范围较磁宁静时大,通量较不突出;
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  flux peak
At the flux peak, the spectrum was characterized by a photon index α ? -1.5 and a peak energy Ep ? 95 keV.
      
The first methane flux peak was noticed during the reproductive phase and the second peak coincided with the grain-ripening stage of the rice cultivars.
      
In a typical burst, the flux peak occurs between 2 and 24 hours after its origin and decays over a period of a few days.
      
This leads to a large flux peak in the interior fuel assemblies close to the spallation target.
      
The lower panels show the counts in the 2.4 and 4.8 keV electron channels that straddle the energy flux peak.
      
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Based on the distribution function got by solving the dynamic equation,the flux distribution and its features of ionospheric heavy ion O+ originating in the auroral zone on the meridian plane are studied.The results show that:1.the flux distribution o f the O+ along the z-direction mainly appears as a peak--like structure,its maximum reduces as the geo-centre distance increasing and more quickly in near geo-space than that in far geo-space;2.the ion O+ exists in larger geo-space and the flux peak is less prominent...

Based on the distribution function got by solving the dynamic equation,the flux distribution and its features of ionospheric heavy ion O+ originating in the auroral zone on the meridian plane are studied.The results show that:1.the flux distribution o f the O+ along the z-direction mainly appears as a peak--like structure,its maximum reduces as the geo-centre distance increasing and more quickly in near geo-space than that in far geo-space;2.the ion O+ exists in larger geo-space and the flux peak is less prominent when Kp=3-5 than that when Kp=0;3.the calculated flux of the ion O+ in the boundary of the plasmasheet is about 105cm2.s-1.The results are consistent with the observation.

应用求解得到的分布函数,研究了北半球子午面内极光带区起源的重离子O+在磁层中的通量密度定态分布及其特性.结果表明:(1)重离子O+通量密度分布沿GSMZ轴方向呈峰状结构,其峰值随地心距离增大而减小,在近地空间减小较快;(2)磁扰动时,O+离子占据的空间范围较磁宁静时大,通量峰较不突出;(3)理论估算的磁尾等离子体片边界层附近重离子O+通量密度与观测结果相一致.

 
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