地球同步轨道相对论电子微分通量的动态预报模型

地球同步轨道区域充满能量高达MeV的高能电子,其对航天器威胁极大.电子微分通量预报有助于及时有效地预警高能电子事件,降低高能电子对航天器造成的危害.本文以此为背景提出了一种基于经验正交函数（EOF）方法的地球同步轨道相对论电子微分通量预报模型.该模型利用太阳风参数及地磁指数拟合后一天的电子通量EOF系数,结合EOF基函数给出后一天中大于2MeV电子微分通量预报.对2003年1月至2006年6月的样本测试结果表明,该模型可以重构出电子微分通量的真实变化,给出较好的5min微分通量预报,其平均预报效率达到67%左右.     

球形压头压入中摩擦对材料参数识别的影响

利用量纲分析原理和有限元方法,研究了球形压头压入中摩擦对于幂强化材料塑性材料参数识别的影响.通过定义一种基于能量的表征应变,根据识别的两个压入深度的表征应变和表征应力,得到材料的塑性特性;最后研究了摩擦对压入响应、表征应力及材料参数提取的影响.研究结果表明,摩擦对压入的影响与材料的应变硬化指数、弹性模量与屈服极限的比值及弹性功与总功的比值密切相关,弹性功与总功的比值越大,摩擦的影响越小;摩擦对材料参数提取的影响不可忽略,当摩擦系数未知时,对于压入过程中弹性功与总功的比值较大的材料,近似取摩擦系数为0.15,能得到较合理的材料参数识别的结果.      

星载大型反射面天线的刚-柔-姿控一体化在轨振动分析方法

随着大型可展开环形天线在航天器上的应用,口径越来越大,指标更加严格,卫星姿控、轨控、太阳翼驱动等导致的机械运动必然会引起大型反射面天线的振动,从而造成电性能降低,影响任务完成质量。提供了一种获取大型环形天线在轨振动影响的刚–柔–姿控一体化分析方法,建立了集扰动源、整星刚柔耦合动力学模型、姿态控制系统、天线振动影响分析的一体化仿真分析模型,实现了在典型扰动模式下的环形天线的振动响应计算、环形天线整体指向和变形计算。分析结果为天线在轨振动影响分析、性能指标预示、振动传递机理及抑制措施提供支持。     

A comprehensive numerical model investigating the thermal-dynamic performance of scientific balloon

The increase of balloon applications makes it necessary for a comprehensive understanding of the thermal and dynamic performance of scientific balloons. This paper proposed a novel numerical model to investigate the thermal and dynamic characteristics of scientific balloon in both ascending and floating conditions. The novel model consists of a dynamic model and thermal model, the dynamic model was solved numerically by a computer program developed with Matlab/Simulink to calculate the velocity and trajectory, the thermal model was solved by the Fluent program to find out the balloon film temperature distribution and inner Helium gas velocity and temperature field. These models were verified by comparing the numerical results with experimental data. Then the thermal and dynamic behavior of a scientific balloon in a real environment were simulated and discussed in details.     

Determination of land surface temperature using precipitable water based Split-Window and Artificial Neural Network in Turkey

Land surface temperature (LST) calculation utilizing satellite thermal images is very difficult due to the great temporal variance of atmospheric water vapor in the atmosphere which strongly affects the thermal radiance incoming to satellite sensors. In this study, Split-Window (SW) and Radial Basis Function (RBF) methods were utilized for prediction of LST using precipitable water for Turkey. Coll 94 Split-Window algorithm was modified using regional precipitable water values estimated from upper-air Radiosond observations for the years 1990–2007 and Local Split-Window (LSW) algorithms were generated for the study area. Using local algorithms and Advanced Very High Resolution Radiometer (AVHRR) data, monthly mean daily sum LST values were calculated. In RBF method latitude, longitude, altitude, surface emissivity, sun shine duration and precipitable water values were used as input variables of the structure. Correlation coefficients between estimated and measured LST values were obtained as 99.23% (for RBF) and 94.48% (for LSW) at 00:00 UTC and 92.77% (for RBF) and 89.98% (for LSW) at 12:00 UTC. These meaningful statistical results suggest that RBF and LSW methods could be used for LST calculation.     

Characterization of ionospheric amplitude scintillations using wavelet entropy detrended GNSS data

The extensive monitoring networks of Global Navigation Satellite System (GNSS) ionospheric scintillation have been established to continuously log observation data. Further, the amplitude scintillation index and the phase scintillation index, which are derived from scintillation observations, are anticipated to accommodate the accuracy requirement of both the user level and the monitoring station level. However, raw scintillation observations essentially measure superposed waveform impairments of GNSS signals propagating through ionosphere and troposphere. It implies that fluctuations of raw scintillation observations are caused by multiple factors from the entire radio propagation environment. Hence, it is crucial to characterize ionospheric scintillations from GNSS observation data. And the characterization is implemented through extracting fluctuations of raw observations merely induced by ionospheric scintillations. Designed to address this problem by means of Fourier filtering detrending, the present work investigates the influence of varying detrending cutoff frequencies on wavelet statistical energy and wavelet entropy distributions of scintillation data. It consequently derives criteria on the optimum detrending cutoff frequency for three types of raw amplitude scintillation data, which are classified by their wavelet energy distributions. Results of the present work verify that detrending with specific optimum cutoff frequencies rather than the fixed and universally applicable one renders the validity and credibility of characterizing ionospheric scintillations as the part of GNSS observation fluctuations purely induced by ionosphere electron density irregularities whose scale sizes are comparable with or smaller than the Fresnel scale.     

现代微波测量的发展动态

从微波测量仪器、测量技术及测量分析出发 ,简单地阐述了现代微波测量发展的趋势。供微波测量人员参考     

板料成形的数值分析及程序系统

本文讨论了板料成形的数值分析方法,并介绍一个能在微机上运行的程序系统——CASF(Computer Aided Sheetmetal Forming)01系统。 CASF01系统采用参数三次样条描述板金零件的几何外形,按弹-塑性流动理论用完全拉格朗日有限元法计算成形过程中的应力应变分布。由于参数样条的插值性和分段描述特点与有限元法的结构离散在基本思想和处理方法上的相似性,系统内曲面描述和力学分析程序间数据传递迅速方便。圆板胀形及其汽车零件的计算实例表明了CASF01系统的可靠性和实用性。     

飞秒激光系统图像调焦装置以及方法

飞秒激光直写技术在复杂三维微结构加工领域具有显著优势,而调焦是否精准直接影响了所加工结构的完整度.提出了在光路中临时置入调焦光源和物的图像调焦技术,通过调节物的位置使其成像面与激光聚焦面一致,从而通过清晰可分辨的成像状态间接反映激光聚焦状态.利用Zemax软件模拟分析了原飞秒激光光路与加入调焦光源和物的调焦光路,二者可实现相同加工物镜后工作距离与良好成像质量,证明了该方法的可行性.通过分析得到该过程的成像误差主要由成像镜头焦深(3.9 μm)引起,我们获得的理想调焦精度可达到1/2焦深以内.设计了单层高度为5 μm的二层圆柱结构,通过多次实验验证了所加工元件高度误差在1.5 μm范围以内,与理论分析一致,满足飞秒激光系统的调焦要求.