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191.
大多数航天器单机产品都要求进行冲击响应谱试验,试验量级普遍为1000g~2000g,甚至超过3000g。对于较大质量(如50 kg以上)产品高量级的冲击试验,振动台、传统的摆锤式或跌落式冲击试验台均很难满足相关要求。文章研究并设计了一套能够进行大质量受试产品高量级冲击响应谱试验的气动冲击试验系统。该系统利用压缩空气瞬间释放膨胀推动质量块加速撞击具有多阶固有频率的谐振板,通过谐振板被激起的响应模拟复杂的衰减正弦波。测试结果表明,系统空载时冲击谱量级达8000g,负载200 kg时可达5000g,时域曲线为振荡衰减波,持续时间小于10 ms。文章提出的气动式冲击响应谱试验系统设计方法可为此类冲击试验系统的设计提供参考和理论依据。 相似文献
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194.
Xi Lin Xiaohua Deng Zhigang Yuan Meng Zhou Shiyou Li Ye Pang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We study the structure and kinetic properties of slow-mode shocks near the plasma sheet boundary layer (PSBL) associated with magnetic reconnection by Cluster observation. The presence of slow-mode shocks is confirmed by traditional Rankine–Hugoniot (RH) analysis and Monte-Carlo shock fitting method. The Walén analysis, applied to the tailward flow associated with slow-mode shocks, also supports that plasma was accelerated across a Petschek-type slow-mode shock connected to the diffusion region. Back-streaming ions were observed on the shock layer, and cold ions were accelerated and heated by slow-mode shocks. In addition, whistler and electrostatic solitary waves were observed around the slow-mode shocks. These waves might be excited by the observed field-aligned electron beams near the shocks. 相似文献
195.
采用边界层理论与斜激波/膨胀波精确算法,建立一种结合Eckert参考温度法和Illingworth-Stewartson变换法优势的边界层权重算法,用于研究超声速黏性楔面边界层位移厚度对斜激波极值规律的影响。分别应用层流Navier-Stokes方程和湍流Navier-Stokes方程的CFD解算器对边界层新模型进行了算例精度评估。在来流马赫数为1.2~2.4和楔面角为3°~20°的范围内,压强比的相对误差小于0.1%。计入层流与湍流边界层影响的理论模型研究表明,边界层影响使得最优马赫数增加;对于层流边界层,最优马赫数增量约为0.001 5~0.003 3;对于湍流边界层,最优马赫数增量约为0.002 8~0.006 1。 相似文献
196.
Chin-Chun Wu R.P. Lepping 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(2):335-338
Using nine years (1995–2003) of solar wind plasma and magnetic field data, solar sunspot number, and geomagnetic activity data, we investigated the geomagnetic activity associated with magnetic clouds (MCs), magnetic cloud-like structures (MCLs), and interplanetary shock waves. Eighty-two MCs and one hundred and twenty-two MCLs were identified by using solar wind and magnetic field data from the WIND mission, and two hundred and sixty-one interplanetary shocks were identified over the period of 1995–2003 in the vicinity of Earth. It is found that MCs are typically more geoeffective than MCLs or interplanetary shocks. The occurrence frequency of MCs is not well correlated with sunspot number. By contrast, both occurrence frequency of MCLs and sudden storm commencements (SSCs) are well correlated with sunspot number. 相似文献
197.
J. Amrico Gonzlez-Esparza S. Jeyakumar 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1815-1820
We study the heliocentric evolution of ICME-like disturbances and their associated transient forward shocks (TFSs) propagating in the interplanetary (IP) medium comparing the solutions of a hydrodynamic (HD) and magnetohydrodynamic (MHD) models using the ZEUS-3D code [Stone, J.M., Norman, M.L., 1992. Zeus-2d: a radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. i – the hydrodynamic algorithms and tests. Astrophysical Journal Supplement Series 80, 753–790]. The simulations show that when a fast ICME and its associated IP shock propagate in the inner heliosphere they have an initial phase of about quasi-constant propagation speed (small deceleration) followed, after a critical distance (deflection point), by an exponential deceleration. By combining white light coronograph and interplanetary scintillation (IPS) measurements of ICMEs propagating within 1 AU [Manoharan, P.K., 2005. Evolution of coronal mass ejections in the inner heliosphere: a study using white-light and scintillation images. Solar Physics 235 (1–2), 345–368], such a critical distance and deceleration has already been inferred observationally. In addition, we also address the interaction between two ICME-like disturbances: a fast ICME 2 overtaking a previously launched slower ICME 1. After interaction, the leading ICME 1 accelerates and the tracking ICME 2 decelerates and both ICMEs tend to arrive at 1 AU having similar speeds. The 2-D HD and MHD models show similar qualitative results for the evolution and interaction of these disturbances in the IP medium. 相似文献
198.
WANG Chi FENG Xueshang 《空间科学学报》2008,(5)
This brief report summarized the latest advances of the interplanetary physics research in China during the period of 2006—2007,made independently by Chinese space physicists and through international collaboration.The report covers all aspects of the interplanetary physics,including theoretical studies,numerical simulation and data analysis. 相似文献
199.
M. Tátrallyay G. Erdős A. Balogh I. Dandouras 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1537-1544
Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations. 相似文献
200.
航迹关联(TTTA)是多传感器数据融合系统的核心模块之一,是系统误差估计和航迹融合的前提和基础。传感器存在的固有系统误差使得目标位置状态估计与真值发生偏离,容易诱发TTTA错误。传统的基于全局最小距离准则的TTTA算法,需要获得较高精度的系统误差估计,来对航迹数据进行误差补偿。针对传感器具有系统误差环境下的TTTA问题,在对TTTA进行间接评估的基础上,定义了一致关联数的概念,提出了一致关联数最大化的TTTA准则,并在稳健交替迭代的框架下完成算法设计。与距离函数不同,一致关联数是一个离散量,放松了对系统误差估计精度的要求。最后,仿真实验验证了所提算法的有效性。 相似文献