基于绿色光源LED的开关型恒流驱动电路设计

针对LED的特点提出开关型恒流驱动电路,通过电流与电压负反馈技术的采用,将LED的输入电流控制在一个稳定的电流数值下,同时使电路防止过电压的能力提高,可靠性大为增强.     

星载激光遥感技术的发展及应用

文章简要介绍了星载激光遥感的技术原理与特性,并对几种星载激光雷达在大气探测、星体测绘、冰盖监测及全球高分辨率测绘等领域的应用做了介绍,最后分析了中国发展星载激光遥感现阶段的已有基础及对未来的发展展望。     

参考系选择对Kepler广播星历参数拟合精度的影响

通过对MEO、IGSO、GEO三类导航卫星广播星历的开普勒轨道根数拟合方法及其拟合精度的分析研究,得出结论:开普勒轨道根数拟合导航卫星广播星历的方法,能很好吸收坐标变换过程中岁差、章动、极移、地球自转等因素对卫星星历拟合精度的影响。     

优化速差补偿方案的激光角反射器设计研究

在分析光学角反射器速差补偿两种经典方法的基础上，指出在实际工程设计中速差补偿方案的选取不是由某一种方法独立实现的，而是两种方法的综合体现。据此给出了适合工程设计特点的差速补偿方法考虑。     

载人航天器舷窗玻璃的强度特性

通过对玻璃强度理论的综述，分析了舷窗玻璃的强度特性。指出舷窗玻璃强度设计必须以玻璃的断裂机理为依据，而不能仅按传统上的杭张强度或抗折强度等指标作为选材标准。舷窗玻璃的强度受表面微裂纹影响很大，要保证舷窗玻璃强度达到设计和使用要求，必须对玻璃表面的裂纹进行严格的控制和检测。考虑到玻璃的亚临界裂纹生长，舷窗玻璃使用前应避免在大气环境中长时间受力。在舷窗结构设计时还应避免使处于张应力的表面与水分接触。     

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.     

Origin and Evolution of the Light Nuclides

After a short historical (and highly subjective) introduction to the field, I discuss our current understanding of the origin and evolution of the light nuclides D, ³He, ⁴He, ⁶Li, ⁷Li, ⁹Be, ¹⁰B and ¹¹B. Despite considerable observational and theoretical progress, important uncertainties still persist for each and every one of those nuclides. The present-day abundance of D in the local interstellar medium is currently uncertain, making it difficult to infer the recent chemical evolution of the solar neighborhood. To account for the observed quasi-constancy of ³He abundance from the Big Bang to our days, the stellar production of that nuclide must be negligible; however, the scarce observations of its abundance in planetary nebulae seem to contradict this idea. The observed Be and B evolution as primaries suggests that the source composition of cosmic rays has remained ∼constant since the early days of the Galaxy, a suggestion with far reaching implications for the origin of cosmic rays; however, the main idea proposed to account for that constancy, namely that superbubbles are at the source of cosmic rays, encounters some serious difficulties. The best explanation for the mismatch between primordial Li and the observed “Spite-plateau” in halo stars appears to be depletion of Li in stellar envelopes, by some yet poorly understood mechanism. But this explanation impacts on the level of the recently discovered early “⁶Li plateau”, which (if confirmed), seriously challenges current ideas of cosmic ray nucleosynthesis.     

轻型空间CCD相机模态分析及结构建模方法研究

文章以大型结构设计软件Pro/E、前后处理软件PATRAN及分析软件NASTRAN为基础 ,研究了轻型空间CCD相机的结构建模方法 ,建立了相机的超大规模有限元模型 ,并对该相机主要零部件及整机等多种状态进行模态分析 ,在验证该相机结构设计的合理性的同时有效地改进了设计。     

光抽运小铯束频率标准中光频移的测量

对光抽运小铯束管的光频移进行了测量 ,并对结果进行了简要的分析 ,估算了射入Ramsey腔的相应光强。导致光频移的光源是抽运光和检测光通过漫反射进入微波腔的部分和原子束中的铯原子自发辐射所产生的荧光。     

一种基于能量-灰度分布的图像清晰度评价方法

在分析了传统的清晰度评价函数后,提出了一种适用于评价光学滤波后成像质量好坏的图像清晰度评价算法。给出了该算法的原理和过程,该算法较之前的清晰度评价算法相比,更多的考虑了应用背景中光强对图像质量的影响。与其他几种清晰度评价函数的实验对比结果表明,该方法有效的克服了梯度平方函数的缺点,不仅适用于自动聚焦领域,对普通的图像清晰度评价也十分有效。