电路模拟吸波材料带宽拓展方法探索

电路模拟吸波材料有一定的频率选择特性,电磁波有效损耗的带宽通常比较窄,通过多层电路屏、掺杂电损耗介质、磁损耗介质层组合、磁电损耗组合的方法,对电路模拟结构吸波材料在2~18GHz区间电磁损耗带宽的拓展进行了初步探索。结果证明:四种方法都能够提高电路模拟吸波材料的有效吸波带宽,并能够不同程度地提高材料的吸波效率。多层电路屏、掺杂电损耗介质的多层电路屏、组合磁损耗介质层的多层电路屏、组合磁损耗介质层和电损耗介质的多层电路屏,其反射率≤-5dB的带宽较单层电路屏的1.2GHz分别增加了6.4、10.6、9.6、10.6GHz,最小反射率分别达到-8、-10、-12、-25dB。     

民用客机座舱温、湿度限制等效安全研究与应用

受低纬度区域低空空气高湿度影响,民用客机对适航条款FAR/CCAR25.831(g)的符合性验证非常困难。以FAA的MSHWG报告为指导,通过验证座舱温、湿度限制等效安全规则间接验证某型民用客机对适航条款FAR/CCAR25.831(g)的符合性,即采用热分析方法计算民用客机通风系统失效时座舱内部乘员人体核心温度的变化,并将其与MSHWG报告规定的人体核心温度标准值对比,说明某型民用客机对适航条款FAR/CCAR25.831(g)的符合性。     

激光等离子体微推力器的发展及热点问题

激光微推力器在航天器的轨道调整、引力补偿、位置保持、轨道机动和姿态控制等方面存在巨大的潜在优势。对近年来激光等离子体微推力器的研究和发展进行了较全面介绍,并详述了激光等离子体微推力器发展过程中的几个热点问题,包括激光等离子体微推力器的工作模式和工质的选择、推力单元结构设计、微型激光器和微推力测试方法的研究与发展现状。通过对比分析,给出了目前所研究的激光等离子体微推力器的优缺点,为国内研制激光等离子体微推力器提供了一些有益参考。     

固体药柱的超声特征扫描成像检测

研究了固体火箭发动机药柱的声传播特性。介绍了超声特征扫描成像方法的原理、扫描系统的设计。采用研制的低频组合探头,提高了声波在粘弹介质中的穿透能力。试验表明,设计的超声特征扫描系统可采用幅度成像、深度成像成功检测药柱的缺陷。     

The isotopic composition of anomalous cosmic rays from sampex

Measurements of the anomalous cosmic ray (ACR) isotopic composition have been made in three regions of the magnetosphere accessible from the polar Earth orbit of SAMPEX, including the interplanetary medium at high latitudes and geomagnetically trapped ACRs. At those latitudes where ACRs can penetrate the Earth's magnetic field while fully stripped galactic cosmic rays (GCRs) of similar energies are excluded, a pure ACR sample is observed to have the following composition: ¹⁵N/N < 0.023, ¹⁸O/¹⁶O < 0.0034, and ²²Ne/²⁰Ne = 0.077(+0.085, –0.023). We compare our values with those found by previous investigators and with those measured in other samples of solar and galactic material. In particular, a comparison of ²²Ne/²⁰Ne measurements from various sources implies that GCRs are not simply an accelerated sample of the local interstellar medium.     

概括原则与悖论研究的进展

悖论的出现与概括原则中的造集的任意性有很大关系。然而,历史上各种排除悖论的方案要么修改概括原则而过多地限制了概括原则的合理内容,要么修改与之配套的逻辑系统而导致失败。近年来,这些问题的研究又取得了新的进展,有必要历史地加以评介,本文从类型论、ZFC公理系统、BG公理系统、多值逻辑系统和中介数学系统五个方面综述逻辑数学悖论之解释方法的研究情况。     

Ion relaxation processes in the heliospheric interface: how perturbed are ion distribution functions?

Charge-exchange processes between interstellar H-/O-atoms and protons of the bulk of the interstellar plasma flow downstream of the outer bowshock in the heliospheric interface induce secondary ions leading to non-relaxated velocity distribution functions. The relaxation of these freshly induced ions towards an equilibrium distribution occurs due to Coulomb interactions and wave–particle interactions with the background turbulence. Since Coulomb interactions are of low relevance, we study here in detail the effect of wave–particle interactions. To find the turbulence levels in the interface we consider the MHD-wave transformation at the outer shock surface between the interface and the local interstellar plasma. The turbulence in the outer interface region is shown to be dominated by incompressible Alfvén waves both for cases of quasiparallel and quasiperpendicular shocks. Also we show that waves propagating towards the shock are more intensive than those propagating away from it. The level of Alfvén turbulence in the interface is estimated using the recent data on local interstellar turbulence deduced from observations of interstellar scintillations of distant radiosources. Two proton relaxation processes are considered: quasilinear resonant interactions with Alfvén waves and non-linear self-induced wave–particle scattering. The corresponding diffusion coefficients are estimated, and typical time periods for protons and oxygen ions relaxation are shown to be of the same order of magnitude as H-/O-atoms passage time over the extent of the interface. This indicates that perturbed ion distribution functions must be expected there.     

Coupling of the interstellar and interplanetary magnetic fields at the heliospheric interface: The effect of neutral hydrogen atoms

We present numerical results showing the effect of neutral hydrogen atoms on the solar wind (SW) interaction with the local interstellar medium (LISM), where the interstellar magnetic field (ISMF) is coupled to the interplanetary magnetic field (IMF) at the surface of the heliopause. The IMF on the inner boundary surrounding the Sun is specified in the form of a Parker spiral and self-consistently develops in accordance with the SW motion inside the heliopause. The model of the SW–LISM interaction involves both plasma and neutral components which are treated as fluids. The configuration is chosen where the ISMF is orthogonal to the LISM velocity and tilted 60° to the ecliptic plane. This orientation of the magnetic field is a possible explanation of the 2–3 kHz emission data which is believed to originate ahead of the heliopause. It is shown that the topology of the heliospheric current sheet is substantially affected by the ISMF. The interaction pattern dependence on the neutral hydrogen density is analyzed.     

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．     

我国中小企业发展中存在的问题与对策

近几年我国中小企业发展比较迅速，但是中小企业目前所面临的困难也很多。要改变中小企业的生存环境和促进中小企业快速发展，除了企业加强自身能力外，社会尤其是政府应当在政策上给予扶持，在各方面给予中小企业提供帮助，使中小企业快速、健康地发展。