The Surface of Mercury as Seen by Mariner 10

The Mariner 10 spacecraft made three flyby passes of Mercury in 1974 and 1975. It imaged a little less than half of the surface and discovered Mercury had an intrinsic magnetic field. This paper briefly describes the surface of Mercury as seen by Mariner 10 as a backdrop to the discoveries made since then by ground-based observations and the optimistic anticipation of new discoveries by MESSENGER and BepiColombo spacecraft that are scheduled for encounter in the next decade.     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.     

一种新型的双圆环形印刷天线设计

提出了一种新型圆极化天线形式——双圆环形印刷天线。通过提出一种异形巴伦,解决了圆极化天线与馈电网络严重失配的技术难题,从而使得该天线具有较高的增益和较宽的波束,且工作频率范围内驻波在1．5以下。天线的实测结果与仿真结果能够较好地吻合。     

小型氢原子频标微波腔本征值问题的计算机仿真分析

使用Ansoft HFSS软件分别仿真计算了氢原子频标中标准尺寸微波腔、蓝宝石部分介质充填微波腔和不同金属极片间距的磁控管微波腔,并分析了储存泡对谐振频率的影响,得到极片间距和储存泡对谐振频率的影响趋势,对于实际工作时主要影响谐振频率的极片间距的选择给出了建议。     

EB-PVD热障涂层对IC10合金高温持久性能的影响

采用电弧离子镀技术在IC10合金基体上制备NiCrAlYSi粘结层,采用电子束物理气相沉积(EB-PVD)技术在粘结层上制备YSZ陶瓷面层,研究TBCs涂层对IC10合金高温持久性能的影响.结果表明,IC10合金沉积TBCs涂层后,980℃高温持久寿命高于IC10合金,持久塑性略高于基体合金,IC10合金沉积TBCs涂层后,对高温持久性能无不良影响,满足使用要求.     

基于IRIG106 Chapter 10标准的数据记录系统

IRIG106 chapter 10是一种数据获取与记录标准,用较经济的方法实现多种数据的数字化和有效组合。本文探讨了IRIG106 chapter 10标准、STANAG4575文件系统的关键特征,针对机载数据记录系统的需求,提出了一种基于IRIG106 chapter 10标准的数据记录系统设计架构,对于机载数据记录系统的设计和研究有一定的价值。     

涂层厚度对AZ91D镁合金WC涂层性能影响研究

采用JP-5000超音速火焰喷涂技术在AZ91D镁合金表面喷涂WC-10Co4Cr涂层。利用扫描电子显微镜、X射线衍射仪、显微硬度计等设备和浸泡腐蚀实验来分析WC涂层的组织结构和性能。结果表明：WC涂层均匀、致密,孔隙较少,涂层与基体结合紧密,无裂纹,无剥离;WC发生分解形成W2C,分解率与火焰作用时间有关;随涂层厚度的增加,涂层的显微硬度有增大的趋势;WC涂层提高了镁合金的耐腐蚀性。     

高水压环境下机械位移机构设计

介绍了一套用于辅助计量测试的高水压环境下机械位移机构设计实例,详细讨论了10MPa水压环境下电机密封装置设计,水下位移机构导向传动机构的设计方案等。电机密封装置是为某型号步进电机专门设计的密封外壳,它采用车氏密封标准产品为基础设计动密封结构,采用O型橡胶圈解决静密封问题;水下位移机构的设计以光轴为位移导向,以万向滚珠为回转导向,以齿轮齿条和梯形丝杠为位移传动方式,细节上采用了一些非常规的设计结构和处理方式。     

基于JP-10与RP-3燃烧的数值模拟

基于标准肛￡二方程湍流模型、EDM湍流燃烧模型以及DO辐射模型,对JP-10与RP-3燃料在某型弹用涡喷发动机燃烧室中的燃烧过程分别进行了数值模拟。结果表明,在保持燃料质量流量不变的条件下,采用JP-10替代RP-3后,燃烧室内的温度分布、组分浓度分布变化不大,引起的发动机结构的热负载差异也不大,但对于同等体积的燃油,燃油持续燃烧的时间却增加20％左右。     

促进剂对高碳数碳氢燃料点火特性的影响

在JP-10和煤油点火特性激波管实验基础上,进行了促进剂CH3NO2、CH2Cl2对JP-10和煤油点火特性影响的实验.在预加热激波管上采用缝合运行技术,获得了近7ms的实验时间.采用单色仪和光电倍增管记录点火过程中OH自由基在306.5nm发射谱强度变化作为点火发生的判据.当促进剂加入量约为JP-10的10%~20%(摩尔比),质量比为5%~12%时,实验观测到明显的点火促进作用.在1100K时,添加10%(摩尔比)CH3NO2使JP-10的点火延时时间缩短了70%.当CH3NO2的加入量占煤油的10%~15%(摩尔比),质量比约为5%~6%时,对煤油点火有明显的促进作用,在1000K时使煤油点火延时时间缩短了50%.