一种有电压补偿电路的高性能低压CFOA及其小信号分析

提出了一种新型的电流反馈型运算放大器,该电路所具有的电压补偿电路克服了以往基于CMOS的CFOA两个输入端静态条件下不平衡的缺点,NMOS与PMOS互补的输入结构提高了电路的信噪比。采用0.6μm工艺参数(低阈值),1.5V电源电压,利用HSPICE进行了仿真,获得了4.95mW的功耗,4.5 kΩ的输入电阻,53.5°的相位裕度以及与增益无关的带宽和极大的转换速率。     

活动区新浮磁流和暗条的激活

用数值计算方法探讨了新浮磁流驱动下暗条运动的基本规律。计算表明,活动区新浮磁流是驱动暗条运动导致暗条激活的有效机制之一,这个过程是通过暗条电流和背景磁场的相互作用来实现的。当选取不同强度的浮现磁流时,暗条可出现周期性振荡、激活上升和闪烁;此外,对同极性磁流浮现,当浮现强度足够强时,暗条一开始就会下沉。      

太阳风中的Alfven波耗散与电子和质子温度分布问题

根据动力论Alfven波耗散机制,详细计算了动力论Alfven波衰减的能量分配给质子和电子的比率.初步解释了高速太阳风中质子温度比电子温度高的事实,定性说明了r＜10R_s时电子快速冷却的原因.      

太阳风与彗尾等离子体相互作用引起不稳定的一种讨论

本文讨论了在无力场情形下,太阳风与彗尾等离子体相互作用的二流不稳定问题。应用International Cometary Explorer(ICE)飞行器对彗星Giacobini-Zinner的探测数据,采用合理的等离子分布形式,得出的结论是在彗星内部存在着这种二流不稳定现象。      

发电-储能一体化柔性电源系统结构热特性仿真研究

基于柔性薄膜砷化镓(GaAs)太阳电池、全固态薄膜锂电池(TFB)和柔性管理电路组成的发电-储能结构一体化电源系统,可以用作便携式应急电源,也可与无人飞行器、便捷式电子设备、无线传感网络节点等结合,实现自身能源的闭合供给,满足相关装备对电能源全天候、长时间、模块化等多样化应用的需求。但在实际工作中,系统的电转化效率只有30%左右,大部分太阳光的能量经太阳电池吸收后会转化成热,TFB在充电过程中也会发热。电源系统中,柔性太阳电池和TFB采用键合的方式结合,由于薄膜各层材料的热膨胀系数不同,产生的热量会在电源系统内部导致热应力,造成键合材料的分离,甚至破坏整个电源系统。通过计算机模拟柔性电源系统在月球表面环境下的工作状态,建立电源系统结构模型以及热传递数学模型,仿真得到不同结构电源系统工作时的温度场和应力场分布情况,对发电-储能一体化柔性电源系统结构优化和工作状态的掌握具有指导意义。     

Semi-global leader-following consensus-based formation flight of unmanned aerial vehicles

In this paper, we investigate a formation control problem of multi-agent systems(specifically a group of unmanned aerial vehicles) based on a semi-global leader-following consensus approach with both the leader and the followers subject to input saturation. Utilizing the low gain feedback design technique, a distributed static control protocol and a distributed adaptive control protocol are constructed. The former solves the problem under an assumption that the communication network is undirecte...     

基于交互式多模型的红外／雷达低小慢目标跟踪算法研究

研究了基于交互式多模型（IMM）的低小慢目标跟踪问题。基于低小慢目标运动特征的分析,以及目标匀速（CV）直线、匀加速（CA）直线、曲线飞行航迹模型,给出了目标跟踪的IMM算法及其流程。仿真结果表明：该算法能稳定精确跟踪低空目标。     

Response of low latitude D-region ionosphere to the total solar eclipse of 22 July 2009 deduced from ELF/VLF analysis

Response of the D-region of the ionosphere to the total solar eclipse of 22 July 2009 at low latitude, Varanasi (Geog. lat., 25.27° N; Geog. long., 82.98° E; Geomag. lat. = 14° 55’ N) was investigated using ELF/VLF radio signal. Tweeks, a naturally occurring VLF signal and radio signals from various VLF navigational transmitters are first time used simultaneously to study the effect of total solar eclipse (TSE). Tweeks occurrence is a nighttime phenomena but the obscuration of solar disc during TSE in early morning leads to tweek occurrence. The changes in D-region ionospheric VLF reflection heights (h) and electron density (n_e: 22.6–24.6 cm⁻³) during eclipse have been estimated from tweek analysis. The reflection height increased from ∼89 km from the first occurrence of tweek to about ∼93 km at the totality and then decreased to ∼88 km at the end of the eclipse, suggesting significant increase in tweek reflection height of about 5.5 km during the eclipse. The reflection heights at the time of totality during TSE are found to be less by 2–3 km as compared to the usual nighttime tweek reflection heights. This is due to partial nighttime condition created by TSE. A significant increase of 3 dB in the strength of the amplitude of VLF signal of 22.2 kHz transmitted from JJI-Japan is observed around the time of the total solar eclipse (TSE) as compared to a normal day. The modeled electron density height profile of the lower ionosphere depicts linear variation in the electron density with respect to solar radiation as observed by tweek analysis also. These low latitude ionospheric perturbations on the eclipse day are discussed and compared with other normal days.     

基于三结太阳电池的透射率测量系统

在空间环境中太阳电池的涂层会发生退化,从而影响航天器的飞行寿命,因此研究能够测量涂层光学透射率变化的系统具有重要意义.使用三结太阳电池作为探测器接收光能量;设计光电流检测电路,对太阳电池输出电流进行电流-电压变换,放大,滤波和模数转换,最终输入上位机处理;运用双通道比对测量技术,比较有玻璃和无玻璃的三结太阳电池光电流测量值,计算出玻璃样片在三结太阳电池响应谱段内的整体透射率;使用热电阻传感器检测太阳电池工作温度以消除温度变化带来的误差.通过实验测得系统的测试相对误差约为0.1%,测量不确定度小于0.15%.     

Spiral eddies in the Baltic,Black and Caspian seas as seen by satellite radar data

Despite spiral eddies were first seen on the sea surface more than 40 years ago, there is still a lot of uncertainty concerning these eddies. The present paper is aimed to provide the comprehensive results on the occurrence and statistics of small-scale eddies in the three inner seas (the Baltic, Black and Caspian) using satellite synthetic aperture radar (SAR) images. The dataset used includes over 2000 medium resolution Envisat ASAR and ERS-2 SAR images obtained in 2009–2010 in the different parts of the seas mentioned. As a result of the analysis performed ∼14,000 vortical structures were detected. 71% of them were visualized due to surfactant films (“black” eddies), while 29% due to wave/current interactions (“white” eddies). Practically all the eddies detected were cyclonically rotating. Their diameter was within 1–20 km. Characteristic size of the “black” eddies in all the basins was discovered to be less than that of the “white” eddies. Characteristic eddy size for the Baltic, Black and Caspian seas proved to be strictly proportional to the values of the baroclinic Rossby radius of deformation typical for these basins. The “black” eddies did not demonstrate a significant connection with the basin- and meso-scale surface circulation of the seas. Most of the “white” eddies detected were attributed to the zones with the most intense drift currents, i.e. those along the western boundaries and (in the Baltic Sea only) in the elongated parts of the basin.