First millimetric detections of AE Aquarii

We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.     

Navier—Stokes（NS）方程组差分计算中的物理和网格尺度效应及NS方程组的简化

对于高Re数流动计算，在通常二阶精度NS差分格式和网格数条件下，存在某些粘性项落入修正微分方程截断误差项的问题。这类NS方程组计算实际是计算某种简化NS方程组，而且重复计算误差物理粘性项既浪费机时和内存，误差积累又会对数值解产生不可预测的影响，避免外述缺陷的办法一个提高NS差分格式的精度，另一个是丢掉可能落入截断误差项的物理粘性项，把NS方程组简化为广义NS方程组，广义NS计算避免了误差物理粘性项误差积累对数值解的不可知影响，又可节省内存和机时，对高Re数流体工程计算很有好处。利用广义NS方程组计算超声速绕前向和后向台阶流动的结果表明：广义NS方程组与NS方程组的数值结果很好相符符。     

INFLUENCE OF DWELL TIME ON HIGH TEM-PERATURE LOW CYCLE FATIGUE (HTLCF) BEHAVIOR IN AN Nd-BEARING NEAR-α TITANIUM ALLOY

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全球导航卫星系统的测高研究

以美国全球定位系统为代表的全球导航卫星系统具有广泛的应用领域，特点是能够在全球范围和近地空间，全天候地提供飞行器的位置、速度和时间信息。     

高速数据采集和CCD数据变换技术

本文讨论的是高速数据采集技术问题,其中重点阐明利用 CCD(电荷耦合器件)作为模拟一数字变换器(ADC)的中间暂存器,把高速变化信号采样后的信息按顺序快速输入 CCD 中暂存起来,供给低速的 ADC 变换,变成二进制数字量。这种利用 CCD 器件采用快入慢出(FISO)工作方式是解决高速模拟量变换成相应数字量的最新技术。它可以把 ADC 变换率提高到100MHz,而成本却提高很小。     

GaInP_2外延薄膜的成份调制与超结构间的关联

用自制的具有极高分辨率的微机控制的三晶体x-射线衍射仪测量了用MOCVD方法生长的Ga_(0.52)In(0.48)P外延薄膜的超结构。我们发现,在Ga_(0.52)In(0.48)P外延薄膜内由In平面和Ga平面交替组成的(?)平面中,存在着交替的In丰与Ga丰平面。对此,我们定义了有序因子,并首先精确地测定了有序因子值。由此导出了成份调制的表达式。这样,我们就可用成份调制表示式来表达GaInP_2外延薄膜中存在的部分有序相的超结构特征。     

Current dissipation within the chromosphere-corona transition

Studies of sporadic outbursts, ranging from flares to nano-flares, invariably endow the solar corona with steady plasma conditions, prior to seeking a current-flow (or the associated magnetic structure) which induces instability. Such an approach does not incorporate a crucial feature of the natural configuration, namely, that the material is of chromospheric origin, and only resides at coronal altitudes for as long as it can acquire adequate energy. There is clearly a feedback loop involved, which allows plasma to moderate the transfer of energy from the field while making use of this heat to permeate coronal altitudes. An examination of the whole procedure is necessary if the location and threshold-conditions for the energy-conversion mechanism are to be identified.A critical step in the feedback procedure mentioned involves the supply line which links the corona to the chromosphere. Because the solar atmosphere has such large vertical dimensions, even a modest change in average temperature and/or density can place heavy demands on this artery: the problem is that a conventional conduction-dominated transition layer cannot readily accommodate a rapid increase in current-density or plasma-flow. (Restructuring of the temperature gradient, to provide the carriers with extra heat, is a very slow process.) A transition layer of this type is unable to endure for long at the base of a sporadically-heated atmosphere in any case, since it becomes the target for plasma falling in the gravitational field during each intermediate cooling phase. As a result, the gap between the chromosphere and corona is more abrupt than is usually considered, endowing the region with thermo-electric characteristics which allow energy to be extracted when modest current-densities arise. Energy-conversion at this region fulfills two rôles: it supplies at least part of the heat required by the overlying corona, and maintains contact between the chromosphere and corona via non-thermal transport processes.     

星载毫米波反射面天线结构

“神舟4号”飞船的多模态微波辐射计天线的工作频率跨到毫米波段．这在我国过去的航天器天线中尚未遇到．采用了计算机机电热一体化设计手段，从材料的选择入手，把最佳的电性及结构设计、先进有效的制造、检测与装配技术有机地融为一体之后，保证了天线最终的高精度指标．本文从高精度反射面天线的要求出发，从设计、分析、实现以及验证多方面说明星载反射面天线形面高精度的控制与实现．     

大气重力波引起的突发钠层的模拟研究

应用钠原子和中性大气分子的质量连续性方程来模拟突发纳层（SSL），垂直风场采用接近实际大气重力波的正弦行波模式，结果较好地反映了SSL的形成过程。SSL的形成时刻在5－15min之间并可持续到30min之后，形成高度大约在90－100km之间，峰宽为0.5-2km之间，这些都与实际观测SSL的特点相符，同时还进一步地研究了当重力波参数（主要指垂直波长和周期）、风速以及常态钠层半宽度发生变化时SSL的变化趋势。     

武装直升飞机雷达散射截面的估算方法

讨论了在预告不知道武装直升飞机详细外形数据的情况下，根据三视图及少量外形数据，对其外形进行拟合，对雷达散射截面进行估算的方法，并对一武装直升飞机进行了理论计算和实验测试，结果吻合较好。