核磁共振陀螺高精度磁场驱动技术

核磁共振陀螺（NMRG）是利用激光与核磁共振气室中的碱金属原子和惰性气体原子的相互作用使核子以拉莫尔频率进动,并通过磁场驱动技术对气室磁场实现闭环控制和对剩磁进行补偿来维持核子的共振状态,进而能够检测载体的角速度信息。磁场驱动技术作为磁场闭环控制的重要部分,直接影响核磁共振陀螺的磁场控制精度和稳定性。为了解决核磁共振陀螺磁场控制精度和稳定性不足的关键问题,采用交直流分离设计的压控电流源方案改善磁场驱动问题,基于噪声分析理论对电路进行建模和噪声分析,并通过实验验证对三轴线圈的横向磁场控制精度达±0.046 2 nT,纵向磁场控制精度为±0.003 1 nT,实验证明该技术方案具有较强的工程应用价值。      

“嫦娥4号”中继星任务轨道确定问题初探

"嫦娥4号"任务将采用着陆器、巡视器和绕飞地月拉格朗日L2点中继星进行月球背面的探测,中继星已先期发射,进入环绕地月L2点的晕(Halo)轨道。在中继星使命轨道动力学模型的基础上,通过相关仿真工作,开展了中继星在Halo轨道上的摄动源量级及影响定轨预报的主要因素分析,结果表明:太阳光压摄动是其主要影响因素。为降低其相关影响,提高定轨精度,在太阳光压球模型的基础上,结合中继星在轨运行特点及其星体结构特点,提出了一种求解光压等效面积的方法。经仿真分析,使用修正后的太阳光压球模型进行定轨求解,速度精度可提升约一个量级。     

黑板框架的知识表达方法

本文介绍了黑板框架知识表达方法的设计思想和技术。黑板框架是由框架、知识源和黑板模型组成,是产生式规则、谓词、框架等多种知识表达功能的组合形式,它将知识表达和知识处理结合成一体,既能表达静态的知识,又能表达动态的知识;既能方便地表达断言性知识,又能自然地表达结构性知识。表达功能强、灵活性大;方便知识调度,加快推理速度,提高推理效率;方便知识获取并有利于机器学习。 黑板框架是一种能表达特定领域复杂知识结构的良好的方法,具有表达充分、推理充分、推理效率和获取效率高的特点。 文中还对目前各种知识表达方法进行了评价,对黑板模型、知识源、黑板框架的概念进行了描述,并对黑板框架给出了严格的BNF定义。 黑板框架的知识表达方法,已在医学专家系统开发工具BFBEST中获得了成功的应用,并取得满意的效果。     

小波聚类算法在本科招生生源质量分析中的应用

招生是高校人才培养工作的首要环节,生源质量的好坏直接关系到高校的人才培养质量.随着我国高等教育招生制度的改革、发展和完善,自主招生越来越受到高校的重视,优质生源的竞争日趋激烈.本文将小波阈值方法引入到数据的聚类分析中,建立了一种新的数据挖掘模型并应用到在校学生学习成绩信息的分析研究中,对建立科学的本科招生生源质量评价体系进行了初探,分析结果对高校招生管理工作起到了科学指导和辅助决策作用.     

面向地震应急响应的松耦合研判模型管理机制

由于面向地震应急响应系统(EERS)的研判模型有其自身特点,传统决策支持系统中模型管理方法并不能较好地满足其管理需求。提出一种面向地震应急响应的松耦合研判模型管理机制(LC-MM),包括3个部分:(1)研判资源建模环境,由研判模型描述/控制语言(MDCL)和数据源描述/控制语言(DSDCL)组成;(2)研判资源协同交互框架,该框架分为4层,主要包括应用环境上下文App_Context、模型调用者Model_Invoker和数据通道Data_Channel 3个Agent组件;(3)研判资源协同交互协议,该协议将研判任务、研判模型和数据源的紧耦合关系分解为上述Agent组件之间的协同交互关系。实际应用表明,LC-MM能够有效屏蔽研判资源的异构性,提高EERS的可扩展性、动态适应性以及平台无关性,能够较好地满足EERS中研判模型的管理需求。     

ADI-FDTD在激励源和完纯导体边界处的精确格式

证明了当采用交替方向隐式时域有限差分法(AD I-FDTD)计算时,完纯导体和激励源处的算法格式与无源空间的算法格式不同,并推导了AD I-FDTD算法在源和完纯导体所在网格处的精确格式。利用常规的FDTD、无源空间的AD I-FDTD以及在源和导体处采用精确格式的AD I-FDTD,分别计算了点源激励的在自由空间传播的二维TE波、TM波垂直入射于金属条带FSS的散射场。计算结果表明,如果计算域中包含导体或激励源,直接采用通常的AD I-FDTD格式会带来很大的计算误差,而采用该精确格式后,计算结果与FDTD的计算结果吻合,从而证明了本文导出的AD I-FDTD在导体和激励源处的精确格式的正确性和使用的必要性。     

全位置自动焊管机TIG焊电源研制

本文介绍了一种适用于管－管、管－板对接的全位置自动TIG焊晶体管电源，该电源采用可编程控制器控制，具有直流／脉冲功能，焊接参数在4个区间内可分别预测，试验表明，该电源区间过渡时电弧稳定，抗干扰能力强，焊缝均匀、连接。     

旋转热源传热特性的理论研究

研究了旋转热源的热传导问题，并将其简化为一维、旋转的周期性脉冲热源传热问题。类似于流体流动，一组新的由旋转角速度ω、热物性参数和几何尺寸组合而成的无量纲拟贝克数Pe1，Pe2．毕奥数Bi被导出。结果表明．它们对传热过程起决定性作用。尤为重要的是，数值仿真对每周转的温度分布给出了微观的“精细”结构和宏观的“粗糙”结构，两的差别取决于上述无量纲数的不同组合，显示了上述几个无量纲准则数的相对关系对传热特性的影响。     

A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements

With a network of ground-based ionosondes distributed around the world, the ionospheric peak electron density and its height measured by FORMOSAT-3/COSMIC satellites in terms of GPS radio occultation technique are extensively examined in this article. It is found that, in spite of the latitude, the mean values of the peak electron density measured by COSMIC satellites are systematically smaller than those observed by ground-based ionosondes. The discrepancy between them is dependent on the latitude, namely, it is small in low and mid-latitudes and large in high-latitude region. Moreover, statistical analysis shows that the slopes of the regression line that is best fitted to the scatter diagram of occultation-retrieved peak electron density (ordinate axis) versus ionosonde-observed peak density (abscissa axis) are universally less than one. This feature is believed to be the result of path average effect of non-uniform distribution of the electron density along the GSP ray during the occultation. A comparison between COSMIC-measured peak height and ionosonde-derived peak height hmF2 indicates that the former is systematically higher than the latter. The difference in the two can be as large as 20% or more in equatorial and low-latitude regions. This result implies that the peak height hmF2 derived from the virtual height through true height analysis based on Titheridge method seems to underestimate the true peak height. The correlation between COSMIC and ionosonde peak electron densities is analyzed and the result reveals that correlation coefficient seems to be dependent on the fluctuation of the occultation-retrieved electron density profile. The correlation will be higher (lower) for the electron density profiles with smaller (larger) fluctuations. This feature suggests that the inhomogeneous distribution of the electron density along the GPS ray path during the occultation plays an important role affecting the correlation between COSMIC and ionosonde measurements.     

Latitudinal variation of the topside electron temperature at different levels of solar activity

A database of electron temperature (T_e) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature T_e at different latitudes, altitudes, local times and seasons. The T_e data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general T_e changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, T_e increases with increasing solar activity. But this increase is not linear as assumed in most empirical T_e models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward.