基于累积损伤的双基推进剂强度准则及实验

国内在对固体火箭发动机装药结构完整性分析时,强度判断准则基本采用传统的结构强度准则,这些强度准则并不能很好地反映固体推进剂材料的强度破坏过程。该文对双基推进剂试件进行了若干不同拉伸速率下的等速率拉伸破坏试验,结合试验数据获得损伤方程参数,建立了基于累积损伤的结构强度准则。并利用损伤方程预测试件破坏情况,和试验值吻合较好,说明该基于累积损伤的强度准则能够较好地判断双基推进剂材料的破坏。     

观察者模式及Word自动化技术在信息分析软件中的应用

介绍了试验信息质量分析软件的设计与实现,重点阐述了系统涉及的主要技术问题,包括观察者模式以及Word自动化技术的应用。观察者模式的应用提高了软件的可维护性和可重用性,Word自动化技术的应用使得为用户提供可定制的分析报告成为可能。     

RFID技术在军事试验装备管理中的应用

针对传统军事试验装备管理在效率、实时性、可靠性等方面存在的问题,本文提出了一种基于RFID技术设计和实现智能化试验装备管理系统的方法。在对此系统组成与功能进行总体设计的基础上,着重对系统的硬件模块、软件模块进行了详细设计。实际工程应用结果表明,该管理系统能够实现军事试验装备的自动识别和管理,显著提高装备管理的效率和水平,从而实现装备管理智能化。     

COTS星载双模测控应答机基带设计与实现

提出了一种星载双模测控应答机基带设计方案,采用COTS（商用现货）器件实现,能较好解决星载功率受限和空间辐射效应引起的相关问题。测控应答机主处理器由反熔丝FPGA（现场可编程门阵列）实现,可在低功耗条件下保证最基本测控需求,解调上行DPSK（差分相移键控）信号,调制下行扩频信号;协处理器受主处理器控制,由SRAM（静态存储器）FPGA来实现,对上行扩频信号进行解扩解调。测控应答机可根据星载电源功率情况和不同测控任务切换模式,具有成本低、可靠性高、使用灵活等优势。     

原点误差对发射方位角及弹道精度的影响分析

发射原点是飞行器试验中非常重要的参数,在某些特殊试验中,发射原点往往是不能准确给出的,为此,本文详细推导了发射原点误差对发射方位角和弹道精度的影响公式。仿真计算结果证明,原点误差对发射方位角影响较大,而原点误差和发射方位角误差的共同作用对发射系下的弹道精度影响很大,对于此类高精度的飞行器试验必须考虑原点误差对弹道精度的影响。     

电波折射误差实时修正方法研究

目前的实时弹道处理过程中,由于获得探空气象数据比较困难,电波折射误差均采用各种简化方法进行计算,因而大气折射误差计算的精度不高,修正效果不佳。针对这种现状,本文提出了基于双指数模型的射线瞄迹法计算大气折射误差。试算结果表明,该方法的计算精度与事后数据处理所采用的电波折射误差修正方法相当,且能够满足实时处理的时间要求。     

Electron density retrieval from occulting GNSS signals using a gradient-aided inversion technique

In the coming years, opportunities for remote sensing of electron density in the Earth’s ionosphere will expand with the advent of Galileo, which will become part of the global navigation satellite system (GNSS). Methods for accurate electron density retrieval from radio occultation data continue to improve. We describe a new method of electron density retrieval using total electron content measurements obtained in low Earth orbit. This method can be applied to data from dual-frequency receivers tracking the GPS or Galileo transmitters. This simulation study demonstrates that the method significantly improves retrieval accuracy compared to the standard Abel inversion approach that assumes a spherically symmetric ionosphere. Our method incorporates horizontal gradient information available from global maps of Total Electron Content (TEC), which are available from the International GNSS Service (IGS) on a routine basis. The combination of ground and space measurements allows us to improve the accuracy of electron density profiles near the occultation tangent point in the E and F regions of the ionosphere.     

Imaging interplanetary CMEs at radio frequency from solar polar orbit

Coronal mass ejections (CMEs) represent a great concentration of mass and energy input into the lower corona. They have come to be recognized as the major driver of physical conditions change in the Sun–Earth system. Consequently, observations of CMEs are important for understanding and ultimately predicting space weather conditions. This paper discusses a proposed mission, the Solar Polar Orbit Radio Telescope (SPORT) mission, which will observe the propagation of interplanetary CMEs to distances of near 0.35 AU from the Sun. The orbit of SPORT is an elliptical solar polar orbit. The inclination angle between the orbit and ecliptic plane should be about 90°. The main payload on board SPORT will be an imaging radiometer working at the meter wavelength band (radio telescope), which can follow the propagation of interplanetary CMEs. The images that are obtained by the radio telescope embody the brightness temperature of the objectives. Due to the very large size required for the antenna aperture of the radio telescope, we adopt interferometric imaging technology to reduce it. Interferometric imaging technology is based on indirect spatial frequency domain measurements plus Fourier transformation. The SPORT spacecraft will also be equipped with a set of optical and in situ measurement instruments such as a EUV solar telescope, a solar wind ion instrument, an energetic particle detector, a magnetometer, a wave detector and a solar radio burst spectrometer.     

Ionospheric heating due to solar flares as measured by SROSS-C2 satellite

The data on thermal fluctuations of the topside ionosphere have been measured by Retarding Potential Analyser (RPA) payload aboard the SROSS-C2 satellite over the Indian region for half of the solar cycle (1995–2000). The data on solar flare has been obtained from National Geophysical Data Center (NGDC) Boulder, Colorado (USA) and other solar indices (solar radio flux and sunspot number) were download from NGDC website. The ionospheric electron and ion temperatures show a consistent enhancement during the solar flares. The enhancement in the electron temperature is 28–92% and for ion temperature it is 18–39% compared to the normal day’s average temperature. The enhancement of ionospheric temperatures due to solar flares is correlated with the variation of sunspot and solar radio flux (F10.7cm). All the events studied in the present paper fall in the category of subflare with almost same intensity. The ionospheric electron and ion temperatures enhancement have been compared with the IRI model values.     

The Radio Observatory on the Lunar Surface for Solar studies

The Radio Observatory on the Lunar Surface for Solar studies (ROLSS) is a concept for a near-side low radio frequency imaging interferometric array designed to study particle acceleration at the Sun and in the inner heliosphere. The prime science mission is to image the radio emission generated by Type II and III solar radio burst processes with the aim of determining the sites at and mechanisms by which the radiating particles are accelerated. Specific questions to be addressed include the following: (1) Isolating the sites of electron acceleration responsible for Type II and III solar radio bursts during coronal mass ejections (CMEs); and (2) Determining if and the mechanism(s) by which multiple, successive CMEs produce unusually efficient particle acceleration and intense radio emission. Secondary science goals include constraining the density of the lunar ionosphere by searching for a low radio frequency cutoff to solar radio emission and constraining the low energy electron population in astrophysical sources. Key design requirements on ROLSS include the operational frequency and angular resolution. The electron densities in the solar corona and inner heliosphere are such that the relevant emission occurs at frequencies below 10 MHz. Second, resolving the potential sites of particle acceleration requires an instrument with an angular resolution of at least 2°, equivalent to a linear array size of approximately 1000 m. Operations would consist of data acquisition during the lunar day, with regular data downlinks. No operations would occur during lunar night.