空间能量粒子探测方法研究

阐述了空间能量粒子探测的原理和方法。介绍了国外在能量粒子探测方面所采用的半导体望远镜测量法、电场加速法、磁偏转法等方法，分析了它们各自的优缺点。就制约能量粒子探测技术发展的关键因素进行了讨论。并以此为基础，结合我国实际情况提出了一种新的探测方法。     

Space-Wise,Time-Wise,Torus and Rosborough Representations in Gravity Field Modelling

The decade of the geopotentials started July 2000 with the launch of the German high-low SST mission CHAMP. Together with the joint NASA-DLR low-low SST mission GRACE and the ESA gradiometry mission GOCE an unprecedented wealth of geopotential data becomes available over the next few years. Due to the sheer number of unknown gravity field parameters (up to 100 000) and of observations (millions), especially the latter two missions are highly demanding in terms of computational requirements. In this paper several modelling strategies are presented that are based on a semi-analytical approach. In this approach the set of normal equations becomes block-diagonal with maximum block-sizes smaller than the spherical harmonic degree of resolution. The block-diagonality leads to a rapid and powerful gravity field analysis tool. Beyond the more-or-less conventional space-wise and time-wise formulations, the torus approach and Rosborough's representation are discussed. A trade-off between pros and cons of each of the modelling strategies will be given. This revised version was published online in August 2006 with corrections to the Cover Date.     

Reconstructed 3-d magnetic field structure and hard X-ray two ribbons for 2000 Bastille-day event

The Bastille-day event in 2000 produced energetic 3B/X5.6 flare with a halo CME, which had great geo-effects consequently. This event has been studied extensively and it is considered that it follows the two-ribbon flare model. The flare/CME event was triggered by an erupting filament and TRACE observations showed formation of giant arcade structures during the flare process. Hard X-ray (HXR) two ribbons revealed for the first time in this flare event (Masuda et al., 2001). The reconstruction of 3-D coronal magnetic fields revealed a magnetic flux rope structure, for the first time, from extrapolation of observed photospheric vector magnetogram data and the flux rope structure was co-spatial with portion of the filament and a UV bright lane (Yan et al., 2001a, 2001b). Here we review some recent work related to the flux rope structure and the HXR two ribbons by comparing their locations and the flux temporal profiles during the flare process so as to understand the energy release and particle accelerations. It is proposed that the rope instability may have triggered the flare event, and reconnection may occur during this process. The drifting pulsation structure in the decimetric frequency range is considered to manifest the rope ejection, or the initial phase of the coronal mass ejection. The HXR two ribbons were distributed along the flux rope and the rope foot points coincide with HXR sources. The energy dissipation from IPS observations occurred within about 100 R _⋅ is consistent with the estimate for the flux rope system. This revised version was published online in August 2006 with corrections to the Cover Date.     

滑阀稳态液动力的计算和分析

以液氧/煤油补燃循环火箭发动机中流量调节器中滑阀为例,介绍了滑阀稳态液动力的一种计算方法,分析了不同结构参数下稳态液动力的变化规律,得出了滑阀的稳态液动力与滑阀位移、液流出口处的流道形状以及刃边厚度关系的一些初步结论。     

一个简单有效的磁记录纠错系统

介绍一种简单有效的纠错编码方法 ,用于资源卫星高密度数字磁记录器 ,使误码率由 10 -6降低到 10 -11,同时介绍它的基本工作原理、实现方案及试验结果。     

铝合金定向凝固过程枝晶生长的相场法模拟

本文基于Wang等人提出的熵函数公式。在假定平衡时同液界面处固、液相的化学势相同而溶质浓度不同的基础上。推导了一个新的二元合金相场模型。并利用该相场模型与溶质场进行耦合计算，以Al-4．5％Cu合金为例模拟了二元台金等温凝固定向凝固的枝晶生长过程。研究了在正温度梯度情况下二元合金过冷熔体中的等轴枝品和柱状晶的生长过程及其溶质场的分布情况。     

月食过程月表太阳辐照和温度变化模拟

月食对月球轨道探测器的温度有重要的影响,分析月食时月表的太阳辐照和温度,具有重要意义。文章给出了通用的月表温度模型和月食时月表太阳辐照模型,根据某次月食的天文参数,用太阳辐照模型可求出月表任一点在月食时的太阳直接辐照变化过程,代入温度模型可求出任一点的温度变化过程。此模型和方法可用于对任何一次月食的分析,并以2007年8月28日的月食为例,模拟了该次月食的表面太阳直接辐照和温度的变化过程。     

冲压发动机点火前内流场数值仿真研究

冲压发动机在点火前由于燃烧室的压力较低,内通道流场状态与发动机正常工作时的差别很大。因此,在发动机设计时,必须要考虑形成正常点火条件对发动机结构的约束。本文利用有限体积法对N-S方程进行空间离散,对发动机点火前的不同内通道结构下的冷流场进行了数值模拟,结果表明稳定器和喷油装置对形成合理的点火条件很重要,稳定器的布局对点火状态有很大影响。     

一种新型级间分离技术研究

本文对一种含固体燃气发生器的级间分离技术进行了研究。首先给出了分离的总体方案，建立了级间段气体压强瞬变的数学模型和导弹两级的运动模型，并利用流体动力学软件对级间段充气过程进行了模拟。简要介绍了固体燃气发生器的设计，并给出燃气发生器装药的选取原则。最后通过对某型号导弹的计算，证明这种级间分离方案是可行的。     

航天飞行器防热部件烧蚀行为的数值模拟

对航天飞行器防热部件在氧－煤油发动机火焰喷吹下的烧蚀行为进行了有限元数值模拟。利用“杀死”单元的方法建立防热部件瞬态温度场的有限元模型，实现了烧蚀边界的退缩，从而完成了对烧蚀尺寸变化的定量描述。烧蚀开始于4．59s，到12s时线烧蚀量为1．47mm。计算结果与试验的实测结果一致。