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排序方式: 共有842条查询结果,搜索用时 15 毫秒
1.
Space Science Reviews - We discuss afresh the problem of the auroral electron acceleration based on the controversy reports of Bryant, D. A. et al.: 1992, Phys. Rev. Lett. 68, 37, and Borovsky, J.:... 相似文献
2.
The earth's foreshock is a region where particularly large amplitude MHD waves are commonly observed. They exhibit various
waveforms, suggesting that nonlinear interaction between the waves is in progress. In a previous paper (Hada et al., 2003) we have introduced a method to quantitatively evaluate the strength of phase coherence among the waves from a given
time series data. Here we further develop our method by applying wavelet filtering technique. From the analysis it was found
that, although the turbulence is consisted of waves with a wide range of plasma rest frame frequencies, only those frequencies
lower than the ion gyrofrequency are responsible for generating the phase coherence.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
3.
EFFECT OF THE RIBLETS SURFACE ON THE BOUNDARY LAYER DEVELOPMENT 总被引:3,自引:0,他引:3
EFFECT OF THE RIBLETS SURFACE ON THE BOUNDARY LAYER DEVELOPMENTWangJinjun;LanShilong;LianQixiang(InstituteofFluidMechanicsIBe... 相似文献
4.
5.
Large amplitude MHD waves are commonly found in the solar wind. Nonlinear interactions between the MHD waves are likely to
produce finite correlation among the wave phases. For discussions of various transport processes of energetic particles, it
is fundamentally important to determine whether the wave phases are randomly distributed (as assumed in quasi-linear theories)
or they have a finite coherence. Using a method based on a surrogate data technique and a fractal analysis, we analyzed Geotail
magnetic field data (provided by S. Kokubun and T. Nagai through DARTS at the Institute of Space and Astronautical Science)
to evaluate the phase coherence among the MHD waves in the earth's foreshock region. The correlation of wave phases does exist,
indicating that the nonlinear interactions between the waves is in progress.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
6.
用激光多普勒技术测量了二维扩压器中不可压湍流边界层分离流动,得到了时均速度和雷诺剪应力分布。实验结果分析表明:以Coles速度律发展的Bardina速度分布可以描述瞬时间歇分离点以前和瞬时间歇再附点以后的时均速度分布,但无法描述分离区的边界层速度型。Cross速度分布可描述分离区的边界层速度分布。Cebeci&Smith涡粘性代数模型难以正确地描述分离边界层的雷诺剪应力。 相似文献
7.
轴对称降落伞稳定下降阶段的流场特性 总被引:2,自引:0,他引:2
文章根据降落伞的特点,通过3点假设(伞衣的薄膜假设、降落伞的轴对称假设和流场的定常 假设),将三维复杂流动问题,转化成二维轴对称问题,以节约计算时间。然后,建立轴对称降落伞的流体力 学计算模型,利用数值模拟手段,求解RNG(Renormalization Group)k-epsilon湍流模型下的N—S方程组,获 得与有关单位试验相吻合的计算结果。分析发现带顶孔的轴对称降落伞绕流和亚临界状态下带中心孔的 圆球绕流,在尾流区拓扑结构上几乎完全一致。结果表明建立的轴对称降落伞模型,能够揭示降落伞流场 的本质特性,为进一步研究降落伞流场的流动机理和流固耦合问题打下基础。 相似文献
8.
9.
QIN Guotai QIU Shiyan HE Aiqing Zhu Yiqiang SUN Lilin LIN Xianwen LI Hong XU Xuepei 《空间科学学报》2002,22(Z1)
Upper atmosphere composition data were obtained for the last half year with a quadruple mass spectrometer on board spacecraft "SZ-2" launched on 10 Jan uary 2001. Based on the analysis of these data, the variations of atmospheric compositions in solar and geomagnetic quiet conditions are reported first, then a detailed discussion on the atmospheric composition variations under the so lar and geomagnetic disturbed conditions is given. The results show that near the altitude of 400 km the variations of main atmospheric compositions corre sponding to solar disturbances are more remarkable in the sunlit area than in the shade area. On the contrary, in geomagnetic disturbance events the corre sponding variations are more obvious in the shade area, an evident increase of N2 density at relatively higher latitudes was observed. 相似文献
10.
在介绍大气湍流光学长曝光像的两个模型——高斯模型(空间域模型)和统计平均光学传递函数模型(空间频率域模型)的基础上,推导两模型之间的关系与差别,并应用两模型数值计算了扩展目标通过大气的长曝光成像结果。此外,还应用高斯模型给出了自适应光学系统校正后的远场光斑。 相似文献