SMESE (SMall Explorer for Solar Eruptions): A microsatellite mission with combined solar payload

The SMESE (SMall Explorer for Solar Eruptions) mission is a microsatellite proposed by France and China. The payload of SMESE consists of three packages: LYOT (a Lyman α imager and a Lyman α coronagraph), DESIR (an Infra-red Telescope working at 35–80 and 100–250 μm), and HEBS (a High Energy Burst Spectrometer working in X- and gamma-rays).     

Evolution of solar wind structures from 0.72 to 1 AU

Understanding the evolution of solar wind structures in the inner heliosphere as they approach the Earth is important to space weather prediction. From the in situ solar wind plasma and magnetic field measurements of Pioneer Venus Orbiter (PVO) at 0.72 AU (1979–1988), and of Wind/Advanced Composition Explorer (ACE) missions at 1 AU (1995–2004), we identify and characterize two major solar wind structures, stream interaction regions (SIRs) and interplanetary coronal mass ejections (ICMEs). The average percentage of SIRs occurring with shocks increases significantly from 3% to 24% as they evolve from 0.72 to 1 AU. The average occurrence rate, radial extent, and bulk velocity variation of SIRs do not change from 0.72 to 1 AU, while peak pressure and magnetic field strength both decrease with the radial evolution of SIRs. Within the 0.28 AU distance from the orbit of Venus to that of Earth, the average fraction of ICMEs with shocks increases from 49% to 66%, and the typical radial extent of ICMEs expands by about a fraction of 1.4, with peak pressure and magnetic field strength decreasing significantly. The mean occurrence rate and expansion velocity of ICMEs do not change from 0.72 to 1 AU.     

Hydrodynamic atmosphere models for hot luminous stars II. Method and improvements over unified models

In a paper submitted to A&A we present the first line blanketed hydrodynamic models of spherically expanding atmospheres of hot stars. This paper is complementary to the submitted paper. Here, we emphasize the advantages and the weak points of our approach and we present additional technical aspects.The models are characterised by a simultaneous solution of the equation of motion, the non-LTE populations of H and He, and radiation transfer in a line blanketed atmosphere. The entire domain from the optically thick photosphere out to the terminal velocity of the wind is treated. The radiative forces are evaluated consistently with the depth-dependent radiation field, taking into account multiple scattering by metal lines and line overlap.     

液体火箭发动机对单级入轨运载器的影响

对给定的飞行任务，计算了推进系统采用国外现有、改型以及新型液体火箭发动机时，主推进系统发动机的组成方式对单级入轨运载器干质量的影响。对推进系统采用改进SSME的单级入轨运载器，计算了在运载器起飞质量不变的情况下，发动机比冲和质量对运载器有效载荷的影响，以及在有效载荷不变的情况下，发动机比冲和质量对运载器子质运的影响。计算结果表明，推进系统采用双燃料双膨胀发动机的单级入轨运载器具有最小的干质量。     

广义质量的空间算子代数描述

应用空间算子代数理论，研究机械多体系统广义质量的结构特点，研究表明广义质量可初步表示为：M＝HφMφ*H*，并进一步表示为：M＝[I＋HφK]D[I HφK]^*，其逆矩阵可表示为：M^-1＝[I－HψK]^*D^-1[I-HψK]。这种表示与牛顿第二运动定律和欧拉定律相互对应，具有简洁的数学表达和明确的物理意义，广义质量是正，反向动力学的重要参量，是联系旋量力和旋量加速度的桥梁，其理论依根源自通过旋量整合的牛顿第二运动定律和欧拉定律，即d^2β/dt^2=M^tT′，旋量加速度等广义质量的逆左乘旋量力，据此可形成对旋量加速度的高效递推算法，并为下一时刻的φ，H，P，D，G，K等参数的正向动力学计算作准备。     

空间碎片质量分布模型建模方法研究

利用空间碎片环境演化模型的建模思想，对碎片环境建模的过程进行了分析与研究，通过分析1999年以前空间环境中碎片产生，衰减及在未来时间中的演化因素，建立了质量分布模型，并利用可得到的碎片数据进行了仿真研究，所得结果可供有关研究人员参考。     

大质量飞行器质心测量方法

详细介绍了大质量飞行器质心测量的多支点称重法,针对某大质量飞行器,提出了径向测量的改进方法,算例表明,改进方法极大地提高了系统的测量准确度,可以满足大质量飞行器高准确度质心的测量要求。     

一种双功能谐振传感器──谐振式质量流量／密度传感器

详细地讨论了一种双功能谐振式质量流量/密度传感器的测量原理,为我国迅速研制成这种新型的谐振传感器提供了一定的理论依据。     

太阳电池阵的铰链副刚度参数识别

为正确识别太阳电池阵铰链副的刚度参数,用形状简单、建模相对容易的有机玻璃板列阵不同状态下模态试验结果估计待识别参数的初始值,通过线性化目标函数,将参数识别归为易求解的数学规划问题,最终直接用商用有限元分析程序和数学软件实现参数识别。识别结果表明,理论计算值与试验结果基本吻合。     

用飞行时间质谱仪研究固体推进剂催化燃烧行为

介绍了使用飞行时间质谱仪对高氯酸铵(Ap)、Ap加附加物、草酸铵加附加物、含与不含附加物的推进剂热分解进行的实验研究.结果表明XTC-02是Ap热分解的有效催化剂,它不仅能加速Ap的热分解,而且能加速氨的氧化;另外还能加速推进剂的凝聚相反应,改变Ap分解历程.