三维流场的光学C.T技术

本文介绍了三维流场光学Ｃ．Ｔ技术的原理，实验方法和重建算法，给出了计算机模拟研究的方法和应用实例。     

微小卫星平台公共总线技术——CAN网络应用

对局域控制网络(CAN)协议在“清华一号”微小卫星平台上的应用作了描述。提出了微小卫星对平台公共总线的要求,介绍了CAN网络的特点,阐述了CAN协议的帧结构,并在此基础上提出了针对卫星子系统数据通讯所作的改进协议。还给出了微小卫星星载计算机子系统的CAN节点硬件设计结构和软件控制流程。     

双屏显示系统

双屏显示系统是地面测试发控系统的组成部分之一。这种系统提供了一个内容丰富、明了直现、实时性强的图形界面。有关它的组成、功能和实验方法在本文中作了介绍。     

轴对称矢量喷管的气膜冷却及红外辐射耦合计算分析

为考察喷管壁面气膜冷却以及红外辐射特性对高性能航空发动机壁温分布的影响,对燃气红外波带的光谱特性采用窄波段模型计算,对壁面-燃气辐射采用封闭腔模型计算,对喷管收敛段的气膜冷却采用绝热温比计算。对于包含喷管壁面、隔热屏、套筒的多层结构传热建立壁温-热流耦合的热平衡方程,用Newt on-Raphson求解得到喷管及内外结构的壁温。对NASA TN D-1988中试验台架发动机喷管扩张段的气膜冷却及壁温进行验证计算,并详细计算了收敛段采用多排缝槽气膜冷却的轴对称矢量喷管。结果表明:气膜冷却有效降低了喷管收敛段的壁温,使得喷管扩张段成为受热严峻的部位;扩张段偏转改变了扩张段壁面温度和红外辐射的圆周分布,沿偏转方向的壁温和红外辐射都明显低于偏转反方向的,2个方向上的平均壁温相差约4.8%,喷管在后半球的辐射沿偏转方向增强。数值模拟结果与试验测量值吻合良好,可用于发动机喷管壁温分布精确计算。     

飞机环控系统管道气流温度的测量

根据实际使用中出现的问题，对各种实用的管道气流温度传感器的误差进行了计算，对电阻式和热电偶式温度传感器的误差原因作了定量分析。由于带密封罩的温度传感器在实际使用中存在着明显的缺点，建议今后使用热电偶测量飞机环控系统管道气流温度，并提出了一种实用热电偶温度传感器的结构形式，同时也介绍了如何减小由于热传导和热辐射引起的误差。     

Improving DORIS geocenter time series using an empirical rescaling of solar radiation pressure models

Even if Satellite Laser Ranging (SLR) remains the fundamental technique for geocenter monitoring, DORIS can also determine this geophysical parameter. Gobinddass et al. (2009) found that part of the systematic errors at 118 days and 1 year can be significantly reduced by rescaling the current solar radiation pressure models using satellite-dependent empirical models. Here we extend this study to all DORIS satellites and propose a complete set of empirical solar radiation parameter coefficients. A specific problem related to SPOT-5 solar panel realignment is also detected and explained. New DORIS geocenter solutions now show a much better agreement in amplitude with independent SLR solutions and with recent geophysical models. Finally, the impact of this refined DORIS data strategy is discussed in terms of Z-geocenter monitoring as well as for other geodetic products (altitude of high latitude station such as Thule in Greenland) and Precise Orbit Determination. After reprocessing the full 1993.0-2008.0 DORIS data set, we confirm that the proposed strategy allows a significant reduction of systematic errors at periods of 118 days and 1 year (up to 20 mm), especially for the most recent data after 2002.5, when more DORIS satellites are available for geodetic purposes.     

Infrared radiation signature of exhaust plume from solid propellants with different energy characteristics

The infrared radiation signature of the plume from solid propellants with different energy characteristics is not the same. Three kinds of double-base propellants of different energy characteristics are chosen to measure the infrared spectral radiance from 1000 cm 1 to 4500 cm 1 of their plumes. The radiative spectrum is obtained in the tests. The experimental results indicate that the infrared radiation of the plume is determined by the energy characteristics of the propellant. The radiative transfer calculation models of the exhaust plume for the solid propellants are established. By including the chemical reaction source term and the radiation source term into the energy equation, the plume field and the radiative transfer are solved in a coupled way. The calculated results are consistent with the experimental data, so the reliability of the models is confirmed. The temperature distribution and the extent of the afterburning of the plume are distinct for the propellants of different energy characteristics, therefore the plume radiation varies for different propellants. The temperature of the fluid cell in the plume will increase or decrease to some extent by the influence of the radiation term.     

2010年后国外主要航天装备的辐射特性

介绍了2010年后的美国主要军事航天装备的主要发展状况，重点介绍了2010年后的美国军事航天装备工作过程中的空间辐射特性，以及主要采用的反空间信息对抗措施，为未来的空间系统的发展选择提供了参考。     

一种窄带辐射温度计智能标定及检定系统

文章描述了由串行电可改写擦除存储器（ＥＰＲＯＭ）、ＲＳ－２３２通讯口和个人计算机（ＰＣ）组成的窄带辐射温度计标定检定系统。系统除了能够在标定过程中自动完成仪器的标定，给出听输出误差分布、提高仪器的速度以外，在检定时还可以通过修改检定参数很容易地修正仪器的各种源移量，使被检测仪器无需作入动或调整即可重新使用。     

Plasma Waves in the Hermean Magnetosphere

The Hermean magnetosphere is likely to contain a number of wave phenomena. We briefly review what little is known so far about fields and waves around Mercury. We further discuss a number of possible phenomena, including ULF pulsations, acceleration-related radiation, bow shock waves, bremsstrahlung (or braking radiation), and synchrotron radiation. Finally, some predictions are made as to the likelihood that some of these types of wave emission exist.