核磁共振陀螺技术研究进展

核磁共振陀螺是基于量子操控技术的前沿研究新进展。具有高精度、微小型、对加速度不敏感、纯固态等特点,是未来发展高精度、微小型陀螺的主要技术发展方向之一。围绕核磁共振陀螺技术的最新研究进展,重点介绍了核磁共振陀螺的基本工作原理及其硬件构成,分析了核磁共振陀螺在上个世纪的主要技术发展路线与面临的技术发展瓶颈,综述了核磁共振陀螺近年来取得的研究进展及实现的技术突破,最后对核磁共振陀螺技术的未来发展进行了展望。     

复杂地形在不同大气条件下流场显示实验研究

在拖曳式水槽中利用不同密度分层的盐水来模拟不同的大气条件。对香港岛铜锣湾地带的污染情况进行了不同大气条件下的流场显示实验。从该地区在常年风作用下流场的变化,找出污染物不易扩散的原因。     

卫星真空热试验有机分子污染计算软件开发

文章介绍了卫星真空热试验有机分子污染计算软件的物理模型、数学模型及相关的一些重要公式,并对其主体框架、计算流程和特征设计进行了说明。该软件可以进行卫星真空热试验容器内任意位置有机分子污染量的快速计算,对试验过程起到很好的监督作用。     

核热推进载人火星探测方案设计

针对载人火星探测任务,结合我国现有技术基础,提出我国载人火星探测方案,重点研究载人火星探测任务推进系统的设计。首先,综合考虑载人深空探测任务的约束,采用Pork-Chop图设计了适用于不同任务场景的转移轨迹;然后,参考我国空间站技术,基于核热推进系统设计了我国载人火星探测任务的飞船;最后,对核热推进系统的发动机台数和推力进行了优化,得到了适用于不同任务场景的最优推进系统组合方案。本文所研究内容为我国未来载人火星探测任务提供了有益参考。     

A novel wireless light sensing device for planetary and astronomical observations

A novel and versatile wireless light sensing device has been designed and tested for stellar and planetary photometric observations. The device weighing few 10 s of grams finds a number of potential applications in the fields of astronomy and in situ planetary exploration. A Wireless Sensor Network (WSN) using a number of these devices has been deployed to successfully carry out simultaneous photometric observations under different conditions viz. sunlight, twilight, moonlight etc. Observation of a star of known magnitude for flux calibration at low intensity has been carried out by coupling the device to a 1.2 m telescope which demonstrates its sensitivity. A WSN using these devices is further capable of spatio-temporal investigations of sky background intensities. Such a network can also be used to effectively monitor certain astronomical events (lunar eclipse, asteroid occultation etc.) simultaneously from several locations. The capability of the device, level of miniaturization and its versatility makes it a potential tool for many photometric applications.     

Influence of nuclear de-excitation on observables relevant for space exploration

The composition of the space radiation environment inside spacecrafts is modified by the interaction with shielding material, with equipment and even with the astronauts’ bodies. Accurate quantitative estimates of the effects of nuclear reactions are necessary, for example, for dose estimation and prediction of single-event-upset rates. To this end, it is necessary to construct predictive models for nuclear reactions, which usually consist of an intranuclear-cascade or quantum-molecular-dynamics stage, followed by a nuclear-de-excitation stage.     

液压传动系统综合污染分析与控制方法研究

详细分析了工作油液中的固体颗粒、水、气、氯污染物的特征及其对系统的影响.通过多年污染控制实践,以及在汲取国内外先进的污染控制技术的基础上,阐述了各种污染物的控制方法及测试技术,提出了全面污染控制的设想.     

含水率对电动修复Cr（Ⅵ）污染高岭土的影响

实验选用重铬酸钾作为污染物，配制高岭土中Cr（Ⅵ）初始质量分数为500mg·kg^-1。实验研究了不同含水率对电动修复效率的影响程度。实验结果表明：含水率极低时，由于电迁移和电渗流作用都很小，去除效率很低，需要其它的方式提高去除效率；在达到饱和状态时，含水率对去除效率影响很小，几乎为零。在一般含水率情况下，含水率对去除效率影响很大，在以后的中试或现场试验中，建议通过改变含水率的大小来提高去除效率，还需进一步研究。     

Identification of a debris cloud from the nuclear powered SNAPSHOT satellite with haystack radar measurements

Data from the Massachusetts Institute of Technology Lincoln Laboratory Long Range Imaging Radar (known as the Haystack radar) have been used in the past to examine families of objects from individual satellite breakups or families of orbiting objects that can be isolated in altitude and inclination. This is possible because, for some time after a breakup, the debris cloud of particles can remain grouped together in similar orbit planes. This cloud will be visible to the radar, in fixed staring mode, for a short time twice each day, as the orbit plane moves through the field of view. There should be a unique three-dimensional pattern in observation time, range, and range rate which can identify the cloud. Eventually, through slightly differing precession rates of the right ascension of ascending node of the debris cloud, the observation time becomes distributed so that event identification becomes much more difficult.     

Atmospheric electrical conductivity measurements and modeling for application to air pollution studies

The experimentally measured ground level atmospheric electrical conductivity is validated from a simplified ion–aerosol model for which the inputs are ionization rate from surface radioactivity, aerosol density and meteorological parameters. Also estimated from the model is the reduction in conductivity for assumed aerosol levels. It is seen that for an increase of ambient aerosols by threefold the percent reduction in conductivity is 7% and it is 10% for an increase by sixfold. Thus, the variations in the measured ground level conductivity can be used to examine the atmospheric pollution, if any.