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排序方式: 共有88条查询结果,搜索用时 15 毫秒
1.
半实物仿真试验中,要求计算机帧时间与计算积分步长相一致,但在实际试验中不容易精确地做到。本文分析了这种不一致给半实物仿真试验带来的影响,给出了解决的办法,文章中还给出了一实例来说明。 相似文献
2.
Streamwise-body-force-model for rapid simulation combining internal and external flow fields 总被引:2,自引:0,他引:2
《中国航空学报》2016,(5):1205-1212
A streamwise-body-force-model (SBFM) is developed and applied in the overall flow simulation for the distributed propulsion system, combining internal and external flow fields. In view of axial stage effects, fan or compressor effects could be simplified as body forces along the streamline. These body forces which are functions of local parameters could be added as source terms in Navier-Stokes equations to replace solid boundary conditions of blades and hubs. The val-idation of SBFM with uniform inlet and distortion inlet of compressors shows that pressure perfor-mance characteristics agree well with experimental data. A three-dimensional simulation of the integration configuration, via a blended wing body aircraft with a distributed propulsion system using the SBFM, has been completed. Lift coefficient and drag coefficient agree well with wind tun-nel test results. Results show that to reach the goal of rapid integrated simulation combining inter-nal and external flow fields, the computational fluid dynamics method based on SBFM is reasonable. 相似文献
3.
Ondřej Ploc Lembit Sihver Dmitry Kartashov Vyacheslav Shurshakov Raisa Tolochek 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
“Protective curtain” was the physical experiment onboard the International Space Station (ISS) aimed on radiation measurement of the dose – reducing effect of the additional shielding made of hygienic water-soaked wipes and towels placed on the wall in the crew cabin of the Service module Zvezda. The measurements were performed with 12 detector packages composed of thermoluminescent detectors (TLDs) and plastic nuclear track detectors (PNTDs) placed at the Protective curtain, so that they created pairs of shielded and unshielded detectors. 相似文献
4.
以Harris Sheet作为初始条件, 使用数值模拟的方法, 研究了二级磁岛不稳定重联的一些性质. 在模拟中随着初始扰动的加入, Harris Sheet将演化到非线性阶段, 形成更薄的有剪切速度的电流片, 并伴有一级磁岛产生. 当Lundquist数大于或等于105时, 非均匀剪切速度的Sweet-Parker电流片开始不稳定, 并有二级磁岛出现. 不稳定Sweet-Parker电流片对应的临界长宽比为65. Lundquist数越大, 演化形成的Sweet-Parker电流片越薄, 更多的二级磁岛将出现, 且沿电流片两边向外喷出, 随时间变大, 相互合并. 二级磁岛的出现使重联率增大, 并与Lundquist数之间不再满足S-1/2的关系, 而似乎对它的依赖关系不明显. 相似文献
5.
P. Alexander R. Ruscica A.A. Sörensson C.G. Menéndez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Adequate representations of diverse dynamical processes in general circulation models (GCM) are necessary to obtain reliable simulations of the present and the future. The parameterization of orographic gravity wave drag (GWD) is one of the critical components of GCM. It is therefore convenient to evaluate whether standard orographic GWD parameterizations are appropriate. One alternative is to study the generation of gravity waves (GW) with horizontal resolutions that are higher than those used in current GCM simulations. Here we assess the seasonal pattern of topographic GW momentum flux (GWMF) generation for the late 20th and 21st centuries in a downscaling using the Rossby Centre regional atmospheric model under the Intergovernmental Panel on Climate Change A1B emission conditions. We focus on one of the world’s strongest extra-tropical GW zones, the Andes Mountains at mid-latitudes in the Southern Hemisphere. The presence of two GCM sub-grid scale structures locally contributing to GWMF (one positive and one negative) is found to the East of the mountains. For the late 21st century the strength of these structures during the GW high season increases around 23% with respect to the late 20th century, but the GWMF average over GCM grid cell scales remains negative and nearly constant around −0.015 Pa. This constitutes a steady significant contribution during GW high season, which is not related to the GWMF released by individual sporadic strong GW events. This characteristic agrees with the fact that no statistically significant variation in GWMF at source level has been observed in recent GCM simulations of atmospheric change induced by increases in greenhouse gases. 相似文献
6.
7.
Non-thermal components are key ingredients for understanding clusters of galaxies. In the hierarchical model of structure
formation, shocks and large-scale turbulence are unavoidable in the cluster formation processes. Understanding the amplification
and evolution of the magnetic field in galaxy clusters is necessary for modelling both the heat transport and the dissipative
processes in the hot intra-cluster plasma. The acceleration, transport and interactions of non-thermal energetic particles
are essential for modelling the observed emissions. Therefore, the inclusion of the non-thermal components will be mandatory
for simulating accurately the global dynamical processes in clusters. In this review, we summarise the results obtained with
the simulations of the formation of galaxy clusters which address the issues of shocks, magnetic field, cosmic ray particles
and turbulence. 相似文献
8.
K. Dolag S. Borgani S. Schindler A. Diaferio A. M. Bykov 《Space Science Reviews》2008,134(1-4):229-268
Modern cosmological observations allow us to study in great detail the evolution and history of the large scale structure
hierarchy. The fundamental problem of accurate constraints on the cosmological parameters, within a given cosmological model,
requires precise modelling of the observed structure. In this paper we briefly review the current most effective techniques
of large scale structure simulations, emphasising both their advantages and shortcomings. Starting with basics of the direct
N-body simulations appropriate to modelling cold dark matter evolution, we then discuss the direct-sum technique GRAPE, particle-mesh (PM) and hybrid methods, combining the PM and the tree algorithms. Simulations of baryonic matter in the Universe often use hydrodynamic codes based on both particle
methods that discretise mass, and grid-based methods. We briefly describe Eulerian grid methods, and also some variants of
Lagrangian smoothed particle hydrodynamics (SPH) methods. 相似文献
9.
10.
利用线性稳定性理论和直接数值模拟研究了带有入射斜激波的、来流马赫数Ma=4.5条件下的平板边界层的失稳特性。重点考察了在由于激波边界层相互干扰,平板边界层上形成分离区,又进而产生激波、膨胀波和旋涡等复杂流动现象的流场上游,引入小扰动的TS波后,扰动波传播通过带有这些复杂流动现象的流场时,扰动波的发展变化特点。通过对流场中扰动波(包括基本波和衍生波)演化特征的分析,研究分离和激波等复杂流动现象对平板边界层稳定性的影响特点。数值模拟发现,激波的出现不同于一般的压缩波,在亚声速区与超声速区对扰动波演化的影响是不同的,此外,分离对扰动有稳定作用。 相似文献