振动电容式介质内部电荷测量仪研制

内带电效应是引起航天器飞行故障的主要原因之一。为满足对内带电效应进行地面模拟试验研究的需求,文章提出了一种基于振动电容法的内带电电荷测量方法,设计了物理探头和信号处理器,完成了原理样机的研制,并对原理样机进行了标定测量试验。结果表明,该自主研发仪器线性度和准确度高,工作性能稳定。     

一种用于动物黏附运动机制研究的多参数同步测量传感器

在长期生存竞争中,包括壁虎在内的许多动物演化出了与其运动表面间形成黏附力的器官.已有研究发现:生物黏附力与接触面积密切相关,基于范德华力的干黏附可能受包括摩擦接触电荷导致的电场在内的外电场调控.壁虎运动过程接触/摩擦电的存在已得到证实,反力、实际接触面积两个参数的单独测量和表征工作也取得一定成果,但由于不同参数测试技术...     

422E03型In-Line电荷转换器的校准

主要介绍了使用B&K公司的振动传感器校准系统9610A校准PCB公司的422E03型的In-Line电荷转换器的方法及不确定度评定。     

DSP便携式陀螺仪智能寻北系统

介绍了基于CCD图像传感器与DSP技术的陀螺仪智能寻北系统的结构与工作原理,重点介绍了与DSP有关的电子硬件和软件部分,寻北方法在DSP特定环境下的应用,给出了系统的硬件原理图和软件流程图,最后总结了这套系统在陀螺仪寻北中的优点。     

Linear Shaped Charge Cutting Property and Charge Cutting Mechanism of Mg-Gd-Y-Zn Alloy

The linear shaped charge cutting technology is an effective technology for aircraft separation. It can separate invalid components from aircrafts timely to achieve light-weight. Magnesium alloy is the lightest metal material, and can be used to cast effective light-weight components of an aircraft construction. However, the application study of the linear shaped charge cutting technology on magnesium alloy components is basically blank. In response to the demand for the linear separation of magnesium alloys, the Mg-12Gd-0.5Y-0.4Zn alloy is selected to carry out the target shaped charge cutting test. The effects of the shaped charge line density, cutting thickness, and mechanical properties on the cutting performance of the alloy are studied. The shaped charge cutting mechanism is analyzed through the notch structure. The results show that the linear shaped charge cutting performance is significantly affected by the penetration and the collapse. The higher the linear density is, the stronger the ability of the linear shaped charge cutter is, and the greater the penetration depth is, which is advantageous. However, the target structure will be damaged when it is too large (e.g., 4.5 g?m-1). Within 12 mm, when the cutting thickness of the target increases, the penetration depth increases. The lower the tensile strength is, the greater the penetration depth is, and the more conducive the penetration depth to the shaped charge cutting is. When the elongation (EL) increases to 12%, the collapse of the target is incomplete and the target cannot be separated. When the tensile strength of the Mg-Gd-Y-Zn alloy is less than 350 MPa, the EL is less than 6.5%, the cutting thickness is less than 12 mm, and the linear shaped charge cutting of the magnesium alloy can be achieved stably.     

X-Rays From Mars

X-rays from Mars were first detected in July 2001 with the satellite Chandra. The main source of this radiation was fluorescent scattering of solar X-rays in its upper atmosphere. In addition, the presence of an extended X-ray halo was indicated, probably resulting from charge exchange interactions between highly charged heavy ions in the solar wind and neutrals in the Martian exosphere. The statistical significance of the X-ray halo, however, was very low. In November 2003, Mars was observed again in X-rays, this time with the satellite XMM-Newton. This observation, characterized by a considerably higher sensitivity, confirmed the presence of the X-ray halo and proved that charge exchange is indeed the origin of the emission. This was the first definite detection of charge exchange induced X-ray emission from the exosphere of another planet. Previously, this kind of emission had been detected from comets (which are largely exospheres) and from the terrestrial exosphere. Because charge exchange interactions between atmospheric constituents and solar wind ions are considered as an important nonthermal escape mechanism, probably responsible for a significant loss of the Martian atmosphere, X-ray observations may lead to a better understanding of the present state of the Martian atmosphere and its evolution. X-ray images of the Martian exosphere in specific emission lines exhibited a highly anisotropic morphology, varying with individual ions and ionization states. With its capability to trace the X-ray emission out to at least 8 Mars radii, XMM-Newton can explore exospheric regions far beyond those that have been observationally explored to date. Thus, X-ray observations provide a novel method for studying processes in the Martian exosphere on a global scale.     

Ionic Charge States of Solar Energetic Particles: A Clue to the Source

The ionic charge of solar energetic particles (SEP) as observed in interplanetary space is an important parameter for the diagnostic of the plasma conditions at the source region and provides fundamental information about the acceleration and propagation processes at the Sun and in interplanetary space. In this paper we review the new measurements of ionic charge states with advanced instrumentation onboard the SAMPEX, SOHO, and ACE spacecraft that provide for the first time ionic charge measurements over the wide energy range of ∼0.01 to 70 MeV/nuc (for Fe), and for many individual SEP events. These new measurements show a strong energy dependence of the mean ionic charge of heavy ions, most pronounced for iron, indicating that the previous interpretation of the mean ionic charge being solely related to the ambient plasma temperature was too simplistic. This energy dependence, in combination with models on acceleration, charge stripping, and solar and interplanetary propagation, provides constraints for the temperature, density, and acceleration time scales in the acceleration region. The comparison of the measurements with model calculations shows that for impulsive events with a large increase of Q _Fe(E) at energies ≤1 MeV/nuc the acceleration occurs low in the corona, typically at altitudes ≤0.2 R _S .     

Experimental discrimination of electrostatic and magnetic forces in particle–particle aggregation

The aggregates formed in low gravity are generally fractals. The fractal dimensions and the site growth probability measures of the resulting fractal structures strongly depend on the properties of the forces that cause the aggregation. Using some approximations, we solved the equation of motion and obtained the relation giving the particles separation as a function of time. The electric force between two charged particles and the magnetic force between two particles with a magnetic moment were considered. The two relations are different and it is shown that one can identify and separate these two interactions by analysing the recording of the aggregation. The apparatus used to record the aggregation has a resolution in the order of one micrometer per pixel and has the possibility of recording simultaneously two views at right angles. From a three dimensional recording of an aggregation, it will be possible to obtain the product of the two charges or magnetic moments causing the aggregation.     

含氧杂环丁烷基叠氮粘合剂的可回收固体推进剂研究进展

综述了3，3′－双叠 甲基氧杂环丁烷（BAMO）／3－叠氮甲基－3′－甲基氧杂环丁烷（AMMO）共聚物Poly-BAMO/AMMO的合成及在含能配方中的应用和回收研究进展，Poly-BAMO／AM－MO是未来高能、“绿色”固体推进剂及发射药粘合剂的最佳候选。     

空间尘埃的充电过程及与等离子体参数的关系

考虑了地球附近的彗星、行星环、行星际介质等空间尘埃等离子体环境中尘埃颗粒的充电问题．应用典型的空间尘埃等离子体参数，计算了不同种类的尘埃颗粒，以及不同等离子体成分下等离子体中尘粒的平衡电势，得到了尘埃颗粒的平衡电势与尘埃等离子体成分、温度，及其他等离子体参数之间的相互关系．