仿生毛细芯平板热管性能研究

为解决电子设备热管理问题,根据亲水性植物叶片表面微观凸起结构,以颗粒直径为75μm的电解铜粉为材料烧结制备了锥形毛细芯,制造了3种平板热管:普通蒸发段（No.1）、超亲水蒸发段（No.2）、超亲水蒸发段与超疏水冷凝段匹配（No.3）。以去离子水为工质,研究了加热功率、角度等因素对3种平板热管热性能的影响。结果表明:角度对3种平板热管的热性能影响不大,3种平板热管均具有较好的抗重力特性。超亲水蒸发段与超疏水冷凝段匹配的平板热管热性能最佳,当倾斜角为0°、加热功率为140.4W时,蒸发段中心点温度仅为67.0℃。超亲水蒸发段与超疏水冷凝段匹配的平板热管不仅具有最小蒸发热阻,最小值可达0.05K/W,而且具有最小冷凝热阻,最小值可达0.02K/W。      

高能电子对地球同步轨道卫星的影响分析

为了厘清在轨GEO(Geosynchronous Earth Orbit,地球同步轨道)卫星不时出现异常的原因,提高卫星执行任务的可靠性,首先从机理上介绍了空间环境中的地球辐射带及高能电子的情况,引出GEO卫星所处恶劣空间环境的现实;其次基于我国SEPC(Space Environment Prediction Center,国家空间环境预报中心)以及NSMC(National Satellite Meteorological Center,国家卫星气象中心)的空间环境月报资料,结合某GEO环境业务卫星故障的实际数据,经统计归纳,分析得出了地球辐射带中的高能电子是导致GEO卫星发生故障的主要原因;最后按照事例技术分析、常规按需预报和特殊情况下的实时预报等3个层次对高能电子预报方法进行了初步探讨。通过分析可以看出,为提高卫星完成任务的可靠性、降低长期管理风险,需要加强GEO卫星所处空间环境高能电子的预报工作。     

无筒空射运载火箭重力出舱机箭耦合动力学

研究了以运输机为平台的内装式空射运载火箭重力出舱载机-火箭两体动力学。根据火箭受力条件和相对运动自由度,将其出舱运动顺次分为5个阶段。给出了各阶段过渡的力学条件,基于牛顿-欧拉法分别建立了前4个阶段的机-箭两体动力学模型。定义了火箭出舱过程可能发生危险的多种异常情况,给出了发生异常的力学或几何条件。然后对火箭出舱全程作了数值仿真。若发射初始条件合理,仿真将顺次经历前4个或3个正常阶段,直至火箭离舱。如果异常情况的条件满足,火箭出舱将发生危险,仿真失去意义,故中止,需要调整发射初始条件后进一步仿真验证。本文给出的系统动力学模型和仿真数据可为工程部门设计空射型火箭的本体参数,以及设置空射初始条件提供参考。     

The use of Gaussian equations of motions of a satellite for local gravity anomaly recovery

The orbital elements of a low Earth orbiting satellite and their velocities can be used for local determination of gravity anomaly. The important issue is to find direct relations among the anomalies and these parameters. Here, a primary theoretical study is presented for this purpose. The Gaussian equations of motion of a satellite are used to develop integral formulas for recovering the gravity anomalies. The behaviour of kernels of the integrals are investigated for a two-month simulated orbit similar to that of the Gravity field and steady-state ocean circulation explorer (GOCE) mission over Fennoscandia. Numerical investigations show that the integral formulas have neither isotropic nor well-behaved kernels. In such a case, gravity anomaly recovery is not successful due to large spatial truncation error of the integral formulas. Reformulation of the problem by combining the orbital elements and their velocities leads to an integral with a well-behaved kernel which is suitable for our purpose. Also based on these combinations some general relations among the orbital elements and their velocities are obtained which can be used for validation of orbital parameters and their velocities.     

风洞模型投放试验轻模型法重力效应影响

风洞模型投放试验是研究超声速机弹分离问题的一种有效手段，相似参数的选取是影响试验准度的关键因素。有初始弹射速度的超声速机弹分离研究中，通常采用"轻模型法"得到模型的运动学及动力学相似参数，但该相似参数中模型重力模拟不足。为了研究重力效应对投放试验结果的影响，采用CTS试验技术对全尺寸真实参数与缩比尺寸轻模型法相似参数条件下得到的结果进行了对比研究。研究结果表明：在载弹与载机分离过程中，载弹位姿相互耦合，垂直下落位移的快慢会影响载弹姿态角的变化；轻模型法相似参数条件下，载弹垂直下落位移较慢，虚拟重力的修正方法只能近似修正下落位移，不能对导弹姿态角进行修正，而姿态角会影响下落的位移；机弹分离安全性方面，轻模型法相似参数条件下的试验结果较真实参数偏危险。     

Response of the EIA ionosphere to the 7-8 May 2005 geomagnetic storm

In this paper, response of low latitude ionosphere to a moderate geomagnetic storm of 7–8 May 2005 (SSC: 1920 UT on 7 May with Sym-H minimum, ∼−112 nT around 1600 UT on 8 May) has been investigated using the GPS measurements from a near EIA crest region, Rajkot (Geog. 22.29°N, 70.74°E, Geomag.14°), India. We found a decrease in total electron content (TEC) in 12 h after the onset of the storm, an increase during and after 6 h of Sym-H deep minimum with a decrease below its usual-day level on the second day during the recovery phase of the storm. On 8 May, an increase of TEC is observed after sunset and during post-midnight hours (maximum up to 170%) with the formation of ionospheric plasma bubbles followed by a nearly simultaneous onset of scintillations at L-band frequencies following the time of rapid decrease in Sym-H index (−30 nT/h around 1300 UT).     

Physical mechanism of the vertical electric field generation over active tectonic faults

The concept of the Global Electric Circuit (GEC) provides an explanation of the existence of a vertical atmospheric electric field and coupling between the ground and ionosphere. Presently, ionospheric physics pays more attention to electric fields and coupling processes in the polar and auroral regions, whereas in other areas the potential difference between the ground and ionosphere usually is not taken into account. Regional processes exist, however, that are able to significantly affect the GEC parameters and through modification of the ionospheric potential to create plasma density irregularities of different scales within the ionosphere. One such source of ionosphere modification is air ionization in the vicinity of active tectonic faults, which takes place due to increased radon emanation. This paper considers the process of local modification of the GEC and corresponding ionospheric variability due to tectonic activity.     

三维数模随动下的机翼结构重量优化

目前,基于快速建模下的重量重心估算系统得到了快速发展。为了进一步提高结构重量估算精度,研究了如何在重量重心快速分析(WCGA)系统环境中构建优化模块。以机翼结构重量优化为例,提出优化流程,对优化模块功能进行分解,给出模型简化要求。以A320飞机机翼为例,对梁和长桁进行优化,结果显示,经过优化,有效减轻了结构重量,且相比于传统的减重优化设计方法,极大提高了计算效率。     

捷联式移动平台重力仪地面测试结果

自主研制移动平台重力仪对我国矿产资源勘探及测绘等领域具有重要意义。研制了一种基于激光捷联惯导的移动平台重力仪,根据移动平台重力测量应用需求及激光捷联惯导系统特点,采用高精度石英挠性加速度计作为重力测量传感器,安装于系统垂向通道,既可作为导航用垂向加速度计,又用于实现标量重力测量。介绍了工程样机系统的组成。利用重力场随高度升高衰减的原理,以相邻楼层间的重力测量差值评价了系统的静态精度;通过地面跑车试验,获得了系统动态测量内符合精度。     

低成本多小天体并行交会技术

小天体资源开发方兴未艾,为降低开发风险和成本,需要发射无人探测器交会观测多个待选目标小天体。传统多目标探测方案存在无法多次交会、成本高,周期长等不足。提出的低成本多小天体并行交会技术,能够对多小天体探测任务进行解耦,实现基于微纳飞行器的低成本多目标并行交会勘查,从而降低探测成本,缩短探测周期。该技术结合行星借力与不变流形机制构建了低能量星际转移方案。然后引入扰动流形思想,使微纳飞行器能够实现与目标小天体的快速交会。进一步,提出了一种多目标小天体探测全局搜索方法,该方法基于在日地halo轨道上停泊的微纳飞行器集群,逐次确定小天体探测目标,并利用上述方法完成了多微纳飞行器与多小天体的交会。数值仿真结果表明,该方案能够大幅度降低转移过程的燃料消耗,并缩短转移时间。