Coronal plumes and fine scale structure in high speed solar wind streams

We present a solar wind model which takes into account the possible origin of fast solar wind streams in coronal plumes. We treat coronal holes as being made up of essentially 2 plasma species, denser, warmer coronal plumes embedded in a surrounding less dense and cooler medium. Pressure balance at the coronal base implies a smaller magnetic field within coronal plumes than without. Considering the total coronal hole areal expansion as given, we calculate the relative expansion of plumes and the ambient medium subject to transverse pressure balance as the wind accelerates. The magnetic flux is assumed to be conserved independently both within plumes and the surrounding coronal hole. Magnetic field curvature terms are neglected so the model is essentially one dimensional along the coronal plumes, which are treated as thin flux-tubes. We compare the results from this model with white-light photographs of the solar corona and in-situ measurements of the spaghetti-like fine-structure of high-speed winds.     

新型碳基复合吸波材料的制备及性能研究

在聚丙烯腈(PAN)聚合液中分别加入Fe,nano-Fe和FeC2O4.2H2O,经热处理后制备了三种新型的电磁损耗型碳基复合吸波材料.通过X射线衍射仪(XRD)对复合材料分别进行物相分析,三种复合材料中,Fe元素主要以Fe3O4的形式存在.根据所测得的介电常数和磁导率比较分析了三种碳基复合材料和纯碳材料的吸波性能,结果表明加入Fe和nano-Fe制备的碳基复合材料有效改善了纯碳材料的输入波阻抗匹配程度,提高了微波吸收性能.结果表明,加入Fe和nano-Fe制备的碳基复合材料,涂层厚度分别为1.9和2.2mm时,在12.7～ 18GHz频段内,反射损失值都小于- 10dB,有效吸收带宽为5.3GHz.涂层厚度均增至2.5mm,最小反射损失值分别达到- 46和- 29.8dB,有效改善了纯碳基体输入波阻抗匹配程度,提高了微波吸收性能.     

飞机射频隐身表征参量及其影响因素分析

 随着军事装备的不断发展,无源探测器（电子支援系统、雷达告警接收机和电子情报接收机）对飞机的探测能力大大提高。为了避免机载雷达设备辐射的射频(RF)信号被截获,要求飞机具有良好的射频隐身性能。综合考虑机载雷达探测距离和无源截获接收机截获距离之间的关系以及天线空域扫描方式发生捷变对飞机射频隐身性能的影响,指出了用施里海尔(Schleher)截获因子评价飞机射频隐身性能的不足,并提出用信号截获率来表征飞机射频隐身特性的方法。最后,对影响信号截获率的因素进行分析与计算,在此基础上给出飞机实现射频隐身的途径与方法。该评价方法综合了飞机在时域、频域和空域上的射频隐身特性,对飞机的射频隐身设计具有参考价值。     

Radio Wave Emission from the Outer Planets Before Cassini

We review observations and theories of radio wave emissions from the outer planets. These include radio emissions from the auroral regions and from the radiation belts, low-frequency electromagnetic emissions, and atmospheric lightning. For each of these emissions, we present in more details our knowledge of the Saturn counterpart, as well as expectations for Cassini. We summarize the capabilities of the radio instrument onboard Cassini, observations performed during the Jupiter flyby, and first (remote) observations of Saturn. Open questions are listed along with the specific observations that may bring responses to them. The coordinated observations (from the ground and from space) that would be valuable to perform in parallel to Cassini measurements are briefly discussed. Finally, we outline future missions and perspectives.     

复合固体推进剂无烟化述评

综述了复合固体推进剂烟雾成因、消烟途径和国内外无烟(少烟)推进剂的研究情况,指出了今后我国复合固体推进剂无烟化研究的努力方向。     

太阳质子事件与微波爆发的某些特征

选用NOAA提供的太阳质子事件表以及SGD发表的与其相关的射电多波段的观测资料进行了统计分析,试图从厘米波,毫米波爆发与质子事件的关系上寻找规律,从而获得一些有意义的结果.      

基于HEMT的单片微波集成放大器设计

 介绍了S波段单级单片微波集成放大器的设计方法,电路核心为高电子迁移率晶体管(High Electron Mobility Transistor, HEMT).针对在该波段高电子迁移率晶体管稳定性较差、噪声性能优秀的特点设计电路拓扑,在HEMT的输入端并联一个200Ω电阻,用HP-EESOF公司的Libra2.1软件进行了小信号电路仿真与设计.仿真结果表明设计的放大器是绝对稳定的,在2~3GHz频带内增益为14.2dB,纹波小于0.4dB,噪声系数约2.7dB,满足实用要求.     

LA-CDMA蜂窝移动通信系统的无线定位技术

讨论了蜂窝移动通信系统中无线定位技术在智能交通系统(ITS)中的应用.特别针对了在我国具有自主知识产权的第三代移动通信系统,LA-CDMA系统中附加无线定位功能的原理与方法,提出了在正向链路和反向链路中分别实现定位服务方法,并指出各自的优点和缺点,同时分析了在CDMA蜂窝网络中定位所遇到的各种问题.     

1998年5月2日日冕亮度观测图的数值研究

采用数值手段模拟了1998年5月2日日冕亮度观测图，计算模式改进为球坐标下系下特殊的二维理想磁流体（MHD）模型，即把（r,φ）坐标建立在SOHO观测日冕亮度的子午面上，消除了子午面极区的几何奇异性，根据SOHD日冕观测布置磁极子得到初始磁场位形，内边界条件采用自治的投影特征边界条件，计算迭代出稳态的多 磁场结构，得得到了与观测基本一致的亮度图，计算结果表明在太阳表面附近磁场位形对太阳凤等离子参数分布起控制作用。     

X-ray bursts associated with envelope expansion

The precursor associated with a long X-ray burst is interpreted in terms of the stellar envelope expansion. The mass flow driven by the radiation pressure in excess of the local Eddington limit and the grey atmosphere model correctly describe the burst profiles in different energy ranges.