Neutral Atmospheres of the Giant Planets: An Overview of Composition Measurements

Measurements of the chemical composition of the giant planets provide clues of their formation and evolution processes. According to the currently accepted nucleation model, giant planets formed from the initial accretion of an icy core and the capture of the protosolar gas, mosly composed of hydrogen and helium. In the case of Jupiter and Saturn (the gaseous giants), this gaseous component dominates the composition of the planet, while for Uranus and Neptune (the icy giants) it is only a small fraction of the total mass. The measurement of elemental and isotopic ratios in the giant planets provides key diagnostics of this model, as it implies an enrichment in heavy elements (as well as deuterium) with respect to the cosmic composition. Neutral atmospheric constituents in the giant planets have three possible sources: (1) internal (fromthe bulk composition of the planet), (2) photochemical (fromthe photolysis ofmethane) and(3) external (from meteoritic impacts, of local or interplanetary origin). This paper reviews our present knowledge about the atmospheric composition in the giant planets, and their elemental and istopic composition. Measurements concerning key parameters, like C/H, D/H or rare gases in Jupiter, are analysed in detail. The conclusion addresses open questions and observations to be performed in the future.     

切向流与偏流相互干扰对穿孔板声阻抗的影响

对切向流和偏流相互干扰如何影响穿孔板声阻抗进行了细致的实验研究,结果表明:切向流削弱了偏流对穿孔板声阻的调控,但在较高偏流速度下,偏流对穿孔板声阻的影响仍起主导作用;此外,不同的偏流方式(吹气或吸气)与切向流干扰对穿孔板声阻抗的影响有明显区别。最后,尝试通过有效流量系数把不同实验条件下的数据关联起来。     

用于阻抗变换层的Li2O-Al2O3-SiO2玻璃陶瓷制备及其微波介电特性

 采用热压和凝浇注无压烧结的方法制备了Li₂O-Al₂O3-SiO₂ 玻璃陶瓷阻抗变换层,研究表明烧结的工艺方法和参数对该玻璃陶瓷的致密度和复介电常数有很大的影响。在较高烧结温度和压力下,该玻璃陶瓷的复介电常数保持不变。降低烧结温度和压力时,能够得到一系列复介电常数在较小范围内变化的Li₂O-Al₂O₃-SiO₂ 玻璃陶瓷,但复介电常数不随频率发生变化。将该玻璃陶瓷作为吸波材料的阻抗变换层后,大幅度提高了材料的吸波性能,而且其制备工艺对吸波性能也有一定的影响,可以通过改变该玻璃陶瓷的烧结条件来满足不同吸波材料设计对阻抗匹配层的多种要求。     

住宅电力线通信电路的阻抗特性

本文是在加拿大期间的工作总结之一。论述了电力线作为通信媒质时住宅电力电路的阻抗测量结果，并对这些结果进行了分析。     

Comparative Study of the Dynamics of the Outer Planets

The two classes of outer planets, Gas Giants and Ice Giants, have distinctly different global circulation patterns and internal structure. Ongoing ground-based observations of the Ice Giants provide clues to better understanding and Galileo and Cassini data will generate constraints for Gas Giant modeling. The composition below the cloud levels, the depths to which the winds penetrate and the processes that sustain the zonal winds and weather systems are not understood. Basic questions concerning the structure, composition and atmospheric dynamics that are sustained on the four giants could be answered by a combination of orbiters and probes. Future missions that could answer these questions are not currently under development.     

OPTIMIZATION OF ACOUSTIC IMPEDANCE，GEOMETRIC STRUCTURE AND OPERATING CONDITION OF LINERS MOUNTED IN ENGINE DUCT

ＯＰＴＩＭＩＺＡＴＩＯＮＯＦＡＣＯＵＳＴＩＣＩＭＰＥＤＡＮＣＥ，ＧＥＯＭＥＴＲＩＣＳＴＲＵＣＴＵＲＥＡＮＤＯＰＥＲＡＴＩＮＧＣＯＮＤＩＴＩＯＮＯＦＬＩＮＥＲＳＭＯＵＮＴＥＤＩＮＥＮＧＩＮＥＤＵＣＴＬｕＹａｄｏｎｇ；ＷａｎｇＱｉｎｇｋｕａｎ（Ｉｎｓｔｉ...     

大功率晶体管最优驱动电路研究

大功率晶体管深度饱和以降低功率损耗与管子快速关断之间的矛盾并非不可调和。文中针对通常的抗饱和驱动，提出了一种新型驱动电路，很好地解决了这个矛盾。一方面在功率管饱和导通时，比例驱动管子工作于深饱和状态，使功率管的损耗达到最小；另一方面在功率管关断时，驱动电路通过低阻抗抽流回路及高反压辅助抽流的引入，在功率管的基极提供很强的基极反抽电流，使管子快速关断。实验表明与通常的抗饱和驱动相比，本方案由于功率管深度饱和，从而使管子的通态饱和压降降低了0.5V，损耗亦降低了63.4W；另一方面由于关断时基极反抽电流增大了三倍，存储时间增加权0.1us，实现了大功率晶体管的最佳驱动。     

涡流环及其阻抗计算

本文将空心放置式线圈在平面异体中激发的涡流等效成一个环形涡流区域，计算该涡流环的尺寸，分析涡流环对检测线圈阻抗的影响以及计算涡流环的阻抗。     

利用ADS和Serenade设计S波段压控振荡器

简介设计 S波段压控振荡器 ( VCO)的理论基础 ,阐述利用 Agilent公司的 ADS软件进行 S波段 VCO的初步设计过程及如何通过 Ansoft公司的 Serenade软件快速改进 VCO性能 ,使其达到实际要求     

巨磁阻抗微型磁强计技术研究

针对未来微卫星、纳卫星及皮卫星平台的应用需求,介绍了一种基于巨磁阻抗（GMI）效应的微型化三轴磁强计。微型化三轴磁强计采用非线性非对角化巨磁阻抗效应原理制备敏感元件;采用相敏检波方式设计信号处理电路,并对磁强计电路进行了集成化芯片工艺的设计研发。研制的样机在±500mGs磁场下的输出为0~5V。0.1~10 Hz频率范围内的噪声小于RMS 200 pT;频谱密度噪声小于20pT/√("Hz" )@1Hz。