等离子体天线的原理及特性

根据等离子体柱天线的系统构成,分析了等离子体柱天线的基本工作原理,讨论了表面波在等离子体柱天线中的传播特性、等离子体柱内的电子分布,以及天线的长度、噪声与辐射特性。分析表明：表面波能激发和维持等离子体柱,等离子体柱可构成等离子体天线,且具易隐身、可控性等优点。     

High energy radiation from the direction of the galactic black hole Sgr A

X-ray observations indicate that the Galactic black hole Sgr A^∗ is inactive now, however, we suggest that Sgr A^∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼10⁵² erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?10⁵ yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼10⁷ yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process.     

空间光学遥感器天然辐射效应数据库研究

空间环境是诱发卫星异常和故障的主要原因之一。光学遥感器作为卫星最重要的有效载荷之一,在空间会受到空间辐射环境的影响。因此在研制光学遥感器的同时,需要同时考虑空间辐射环境因素,文章就空间光学遥感器天然辐射效应数据库的设计和应用进行了介绍。     

SOI工艺抗辐照SRAM型FPGA设计与实现

为提升SRAM型FPGA电路块存储器和配置存储器抗单粒子翻转性能，本文提出一种脉冲屏蔽SRAM单元结构。该结构通过在标准的六管单元中加入延迟结构,增大单元对单粒子事件响应时间，实现对粒子入射产生的脉冲电流屏蔽作用。以64k SRAM作为验证电路进行单粒子翻转性能对比，电路的抗单粒子翻转阈值由采用标准六管单元的抗单粒子翻转阈值大于25 MeV·cm 2·mg -1 提升至大于45 MeV·cm 2·mg -1 ，加固单元面积较标准六管单元增大约21.3%。30万门级抗辐照FPGA电路通过脉冲屏蔽单元结合抗辐照SOI工艺实现，其抗辐照指标分别为：抗单粒子翻转阈值大于37.3 MeV·cm 2·mg -1 ，抗单粒子锁定阈值大于99.8 MeV·cm 2·mg -1 ，抗电离总剂量能力大于200 krad(Si)。     

Parallel algorithm and its convergence of spatial domain decomposition of discrete ordinates method for solving radiation heat transfer problem

To improve the computational efficiency and hold calculation accuracy at the same time,we study the parallel computation for radiation heat transfer. In this paper, the discrete ordinates method(DOM) and the spatial domain decomposition parallelization(DDP) are combined by message passing interface(MPI) language. The DDP–DOM computation of the radiation heat transfer within the rectangular furnace is described. When the result of DDP–DOM along one-dimensional direction is compared with that along multi-dimensional directions, it is found that the result of the latter one has higher precision without considering the medium scattering. Meanwhile, an in-depth study of the convergence of DDP–DOM for radiation heat transfer is made. Analyzing the cause of the weak convergence, we relate the total number of iteration steps when the convergence is obtained to the number of sub-domains. When we decompose the spatial domain along one-,two- and three-dimensional directions, different linear relationships between the number of total iteration steps and the number of sub-domains will be possessed separately, then several equations are developed to show the relationships. Using the equations, some phenomena in DDP–DOM can be made clear easily. At the same time, the correctness of the equations is verified.     

Charged particles on the Earth–Jupiter–Europa spacecraft trajectory

Charged particle fluxes on the trajectory of future Russian space research mission to Jupiter and its satellite Europa are investigated. The existing experimental data and models of Jupiter’s main magnetic field and radiation belts are summarized. Preliminary results of computations of energetic particle fluxes and radiation doses for each stage of the flight are given. Special attention is paid to estimation of radiation conditions in Europa’s orbit and on its surface; influence of the satellite on spatial distribution of the fluxes of charged particles of various energies is studied.     

烧蚀材料的多光谱真温测量法

应用棱镜分光式多波长光电高温计对氧乙炔焰烧蚀材料的真实温度进行了测量。精心地选择波段及处理方法使烧蚀材料剥离、水蒸汽及烟雾影响减至最小，采用一点标定技术解决了高温区标定问题。     

空间特定目标表面的双波段红外辐射特性调控方法

红外诱饵等空间特定目标是对抗红外探测的主要手段之一。随着双色制导技术的发展,红外探测灵敏度不断提升,目标识别能力不断增强,这对空间特定目标表面的双波段红外辐射的逼真性提出了要求。通过改变空间特定目标表面发射率控制其红外辐射强度的大小,使用数值仿真的方法进行计算,从而提出了对空间特定目标表面红外辐射特性的调控方法。此外根据所确定的表面发射率、可见光吸收及红外发射比例以及内热源功率,选择合适的表面材料以及热功率施加方法,在保证空间特定目标表面机械性能的同时,使空间特定目标满足光照及阴影区的双波段红外辐射特性要求,并进行模型的制作以及热真空实验,证明了理论计算的准确性。     

隔热层厚度和数量对太空多层光学窗口温度分布的影响

 航天器上常安装有用于科学观察的多层光学窗口,其温度分布的均匀性会影响成像质量。运用射线踪迹-节点分析法的任意多层镜反射辐射与导热耦合换热模型,研究了隔热层厚度及数量对太空中多层光学窗口温度分布的影响。光学窗口的吸收系数、折射率随波长的变化用一组矩形谱带来近似。研究显示太空中热辐射在光学窗口的冷却过程中起着非常重要的作用,在离玻璃层表面附近很薄的一层玻璃介质内,辐射与导热存在强烈的耦合作用。隔热层厚度越薄,其内的温度分布越均匀,有利于提高成像质量。隔热层数量越多,光学窗口各层玻璃的温度分布越均匀,有利于提高成像质量,但是隔热层最佳数量的确定还需综合考虑其它因素。     

气动加热下光学窗口传热特性的数值模拟

针对气动加热条件下光学窗口辐射导热耦合传热开展研究,以了解光学窗口的热辐射发射规律及热防护性能。采用有限体积法、蒙特卡罗法、谱带模型建立了具有镜反射界面的光学窗口辐射传输及辐射导热耦合传热计算模型,对具有两层SiO2玻璃的光学窗口传热特性进行了模拟。结果表明处于高温区玻璃向外发射热辐射,低温区玻璃吸收热辐射;除了加热面附近外的玻璃区域,辐射热流密度远大于导热热流密度,在2.9～4.2μm谱带内的辐射热流密度大于0.4～2.9μm谱带内的;在0.4～2.9μm谱带内,可见光波长内的出射辐射热流密度最小,中红外波长范围内出射辐射热流密度最大。在光学窗口总厚度一定的情况下,降低玻璃层厚度和玻璃夹层气体热导率能够有效降低光学窗口非加热面稳态温度。