平直地面对一类圆极化波的等效反射系数

本文研究了入射波电场为任意线极化时,平直地面反射波中左旋圆极化分量和右旋圆极化分量的数学描述,引入了地面对这类波的等效反射系数的概念,并给予了物理解释,讨论了应用的有关问题。     

组网数据处理探讨

讨论了测向定位中双站交会定位及定位误差分析、三站交会定位、多站交会定位若干问题，首次尝试将最小二乘法和递推最小二乘法用于多站测向定位，减少了大量的矩阵求逆，数据利用效率高，可以提高测向定位的精度和简化运算。特别是在存在多径效应的情况下，有利于发现和去除野值。在测向站组网数据的处理和应用上有较强的实用性和推广价值。     

柱形弹体引信天线布局与作用盲点分析

在单天线横截面方向图计算公式的基础上，计算了圆柱体导弹引信双天线、三天线和四天线布局的方向图。讨论了不同布局下引信载频、弹体直径及天线布局与作用盲点的关系。双天线布局的实际测试表明，测试值与计算结果较为吻合，所用的计算方法正确，可为引信天线布局与引信工作频率确定提供设计依据。     

A theoretical assessment of the feasibility of potential Lunar Reconnaissance Orbiter radio occultation observations of the lunar ionosphere

The existence of a “dense” lunar ionosphere has been controversial for decades. Positive ions produced from the lunar surface and exosphere are inferred to have densities that are $?$${10}^6$ – ${10}^7$ m^?3 near the surface and smaller at higher altitudes, yet electron densities derived from radio occultation measurements occasionally exceed these values by orders of magnitude. For example, about 4% of the single-spacecraft radio occultation measurements from Kaguya/SELENE were consistent with peak electron densities of $~$$3\times {10}^8$ m^?3. Space plasmas should be neutral on macroscopic scales, so this represents a substantial discrepancy. Aditional observations of electron densities in the lunar ionosphere are critical to resolving this longstanding paradox. Here we theoretically assess whether radio occultation observations using two-way coherent S-band radio signals from the Lunar Reconnaissance Orbiter (LRO) spacecraft could provide useful measurements of electron densities in the lunar ionosphere. We predict the uncertainty in a single LRO radio occultation measurement of electron density to be $~$$3\times {10}^8$ m^?3, comparable to occasional observations by Kaguya/SELENE of a dense lunar ionosphere. Thus an individual profile from LRO is unlikely to reliably detect the lunar ionosphere; however, averages of multiple ($~$10) LRO profiles acquired under similar geophysical and viewing conditions should be able to make reliable detections. An observing rate of six ingress occultations per day ($~$2000 per year) could be achieved with minimal impact on current LRO operations. This rate compares favorably with the 378 observations reported from the single-spacecraft experiment on Kaguya/SELENE between November 2007 and June 2009. The large number of observations possible for LRO would be sufficient to permit wide-ranging investigations of spatial and temporal variations in the poorly understood lunar ionosphere. These findings strengthen efforts to conduct such observations with LRO.     

离散事件动态系统的GSMP模型及扰动分析

对离散事件动态系统（ＤＥＤＳ）的仿真过程建立了包含中断事件集和驱动事件集的广义半马尔可夫过程（ＧＳＭＰ）模型，对参数的无穷小扰动所引起的系统状态转移时刻进行了扰动分析，最后，讨论了扰动分析所需要的可变换条件和样本性能函数的关系，并提出值得进一步研究的问题。     

浮栅ROM器件的质子辐射效应实验研究

给出了浮栅ROM器件的质子辐射效应实验结果.认为浮栅ROM28C256和29C256的质子辐射效应不是单粒子效应,而是质子及其次级带电粒子产生的累积剂量造成的总剂量效应.器件出现错误有个质子注量阈值.对于29C256,高温加电退火容易消除质子产生的辐射损伤;对于28C256,高温加电退火不易消除质子产生的辐射损伤.动态监测和静态加电的器件都出现数据错误,且不能用编程器重新写入数据.然而不加电的器件在更高的质子注量辐照下未出现错误.对于应用浮栅ROM器件的航天器电子系统,冷备份是提高其可靠性的有效手段之一.     

事项法:提升财务会计核心竞争力的利器

信息技术对会计有着直接的影响，使会计从传统的簿记转变为关系数据库管理，企业资源计划，但同时大量非财务计量的涌现也降低了会计信息的权威，使其核心竞争力面临信息不客观、计量不完整、报告不及时等挑战。事项会计由于其强调个性化、增加信息量、减少抽象性、增强及时性、提高透明度的优势，成为提升会计核心竞争力的利器。由于计算机和网络技术的发展，计量属性研究的深入，会计环境的优化，以及信息使用者素质的提高，事项会计应用条件日益成熟，会计要保持核心竞争力，就必须逐步推行事项会计。     

离散事件系统的Petri网图仿真

1.前言 离散事件动态系统DEDS(Discrete Event Dynamic System)的传统分析方法——应用排队论和随机过程理论为离散事件动态系统建立排队网络模型,在很多情况下已不适用。新的理论和研究方法相继提出。其中之一是“皮特里网”(Petri Nets)理论。另一种比较成熟的方法是仿真法,但是,仿真法要以高昂的计算机设备的大量计算时间为代     

Stellar flares

Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed.     

Global ionospheric scintillations revealed by GPS radio occultation data with FY3C satellite before midnight during the March 2015 storm

Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively.