一种基于集成电路的旋翼转速调节器研制

在对直升机旋翼转速调节系统分析研究的基础上,提出了一种基于集成电路设计旋翼转速调节器的总体设计方案,完成了具体电路设计,采用Multisim仿真工具验证了模块电路设计的正确性.实际应用表明,旋翼转速调节器功能完备,各项性能指标满足直升机所提出的性能指标要求,可在直升机上推广使用.     

凸极式旋转变压器电气性能及设计方法的研究

凸极式旋转变压器是近几年刚出现的新型测角元件,本文详细分析了其工作原理、定子绕组、转子凸极特征和电气性能;本文的结论得到了样机验证,本文还给出了提高测角精度的研究途径.     

基于矢量网络分析仪的相对介电常数扫频测量

采用波导短路法对介质材料的相对介电常数进行扫频自动测量,通过VC＋＋开发了一套宽频带（8GHz~18GHz）复介电常数自动测量系统。用矢量网络分析仪对波导采样器进行扫频测量,不仅可以得到被测材料介电常数的频率特性,而且能够解决超越方程多值解的判断问题,并减少了测量中的误差。通过对介质样品的实际测量,可以发现,该自动测量系统操作简单、测量速度快,测量结果能够达到较高准确度,结果令人满意。     

离子推力器小功率正高压屏栅电源研究

为了设计一种适用于小功率离子推力器的小功率正高压屏栅电源,本文提出了一种前级降压斩波电路后级全桥LLC谐振及全波倍压整流的两级式拓扑结构。在该主电路的基础上,设计了控制电路,并开展了试验研究。试验结果表明：设计的正高压屏栅电源在输入电压42 V、输出负载12.52 kΩ时,输出电压和输出功率分别为1050 V、88 W,且输出电压误差范围控制在2%以内,屏栅电源效率为90.44%。对于输出正负极高压短路、瞬时加减载具有自恢复功能。研究证明了该两级式拓扑结构的可行性,从而提供了一种小功率正高压屏栅电源的设计方法,对小功率离子推力器的发展具有推动作用。     

一种行波型超声电机驱动器的研制

针对超声电机的工作原理和驱动要求,研制一套适用于行波型超声波电机的驱动器。对比分析驱动器与普通驱动电源对超声电机性能的影响,实验结果表明,驱动器的输出波形与参数均满足设计要求,超声电机的输出性能也基本一致。在超声电机长时间运行过程中,电机与驱动器的输出性能均稳定。     

大型整星无磁转台研制方案探讨

文章介绍了气浮、静压、水压、大滚子轴承式、滚轮式等5种转台方案,同时阐述了在设备研制中,优化设计、技术更新的重要性。     

Influence of the Interplanetary Magnetic Field on the Solar Wind Flow about Planetary Obstacles

The main effects caused by the interplanetary magnetic field (IMF) are analyzed in cases of supersonic solar wind flow around magnetized planets (like Earth) and nonmagnetized (like Venus) planets. The IMF has a relatively weak strength in the solar wind but it is enhanced considerably in the so-called plasma depletion layer or magnetic barrier in the vicinity of the streamlined obstacle (magnetopause of a magnetized planet, or ionopause of a nonmagnetized planet). For magnetized planets, the magnetic barrier is a source of free magnetic energy for magnetic reconnection in cases of large magnetic shear at the magnetopause. For nonmagnetized planets, mass loading of the ionospheric particles is very important. The new created ions are accelerated by the electric field related to the IMF, and thus they gain energy from the solar wind plasma. These ions form the boundary layer within the magnetic barrier. This mass loading process affects considerably the profiles of the magnetic field and plasma parameters in the flow region.     

某磁头抛光技术

根据硬盘磁头加工的特点,分析了抛光机的运动学特性及抛光盘、抛光液、磨粒在抛光过程中的摩擦学行为等对磁头表面质量的影响。     

Locating Current Sheets in the Solar Corona

Current sheets are essential for energy dissipation in the solar corona, in particular by enabling magnetic reconnection. Unfortunately, sufficiently thin current sheets cannot be resolved observationally and the theory of their formation is an unresolved issue as well. We consider two predictors of coronal current concentrations, both based on geometrical or even topological properties of a force-free coronal magnetic field. First, there are separatrices related to magnetic nulls. Through separatrices the magnetic connectivity changes discontinuously. Coronal magnetic nulls are, however, very rare. Second, inspired by the concept of generalized magnetic reconnection without nulls, quasi-separatrix layers (QSL) were suggested. Through QSL the magnetic connectivity changes continuously, though strongly. The strength of the connectivity change can be quantified by measuring the squashing of the flux tubes which connect the magnetically conjugated photospheres. We verify the QSL and separatrix concepts by comparing the sites of magnetic nulls and enhanced squashing with the location of current concentrations in the corona. Due to the known difficulties of their direct observation, we simulated coronal current sheets by numerically calculating the response of the corona to energy input from the photosphere, heating a simultaneously observed Extreme Ultraviolet Bright Point. We did not find coronal current sheets at separatrices but at several QSL locations. The reason is that, although the geometrical properties of force-free extrapolated magnetic fields can indeed hint at possible current concentrations, a necessary condition for current sheet formation is the local energy input into the corona.