Sunspot activity and cosmic ray modulation at 1 a.u. for 1900–2013

The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u.     

舰载直升机理论风限图飞行模拟获取方法

获取舰载直升机实用风限图,仅依靠实装飞行试验或建模仿真都是非常困难的。通过起降飞行模拟试验获取理论风限图,结合少量的海上实装飞行验证试验是一种综合较优的方法。起降飞行模拟试验需要真实飞行员和高等级飞行模拟器参与,飞行模拟器中的母舰气流场数据、母舰运动可由建模仿真或试验测试得到,且必须考虑母舰气流场的非定场特性;只有当飞行员视景或视觉反馈受限时(如能见度降低时),飞行模拟器基座的六自由度运动才是必需的;用DIPES或Bedford方法量化飞行员主观操纵负担,结合记录的客观操纵数据,评判起降难度;典型的飞行模拟试验程序包含了不同风况下的进近和甲板着舰,通常每隔15°和5kn一个风况。通过起降飞行模拟试验得到的理论风限图,可以更加有效和安全地指导海上实装飞行验证试验,最终获得实用风限图。     

帆板控制系统设计

该帆板控制系统采用塑料薄膜电位器作为传感器检测角度信号,检测到的角度信号经信号处理电路送12位的串行接口A/D转换器ADS7818进行数字化转换,转化结果由Cortex-M3处理器LM3S615进行处理产生PWM控制信号,该控制信号经功率VMOS驱动电路实现轴流电扇的速度调节,从而实现帆板角度定位闭环控制。通过按键可以实现帆板角度的设定及运行控制,设置六位LED数码管显示实现角度及其它运行状态的显示。经过实际测试该系统完全达到了设计要求的各项指标要求。     

基于循环平稳性的噪声调频干扰高分辨测向方法

根据噪声调频信号循环平稳特性分析,提出了基于阵列接收信号循环均值-空域处理的波达方向(DOA)估计算法。仿真结果表明:该算法的角度估计性能明显高于比幅比相单脉冲测角法,且在高信噪比环境中,该法的估计性能更好、运算量较小。     

基于LabVIEW的通信系统的构建

本设计基于LabVIEW仿真软件完成了基本通信系统和通信综合系统的构建。该系统涵盖了模拟调制,数字调制,模拟信号数字传输,信道编码,最佳接收系统几部分内容。通过系统仿真,实现了系统输入输出波形的直观显示,解决了教学中实验效果不理想,理论内容不好理解的问题。同时通过内置的Web Server进行网页发布后,用户可以在客户...     

椭球台高杆灯风荷载的实验研究

通过风洞实验研究了多钝体高杆灯在不同水平风向角和竖向风向角下的力与力矩系数。实验结果表明在一定的风向角下，法向阻力系数Cdmax=1.030,法向弯曲力矩系数Cmmax=-0.940,轴向力系数Camax=0.504和Camin=-0．600。     

重量的一种遥测式监测系统

本文提出一种重量信号的无线传输和测量方法。重量信号经传感顺转换成电信号，再经Ｖ／Ｆ变换后调频发射，接收信号解调后单片机处理。单片机的信号处理采用电子计数器测频方法，经过计算送显示单元，实现重量信号的遥测。     

Multisim在高频电子技术课程中的应用

使用multisim软件对普通调幅和抑制载波的双边带调幅电路制作和仿真,阐述multisim软件对学习和理解高频电子技术课程有很大的帮助。     

基于LabVIEW的通信系统的构建

本设计基于LabVIEW仿真软件完成了基本通信系统和通信综合系统的构建。该系统涵盖了模拟调制,数字调制,模拟信号数字传输,信道编码,最佳接收系统几部分内容。通过系统仿真,实现了系统输入输出波形的直观显示,解决了教学中实验效果不理想,理论内容不好理解的问题。同时通过内置的Web Server进行网页发布后,用户可以在客户端通过web浏览器远程调用并运行本系统,提高效率,节约成本。     

飞机电气系统参数测试标准实施中问题分析

结合本标准宣贯、研讨会上所提供的信息,分析了飞机电气系统参数测试标准在实际应用中存在的一些问题,并对瞬态电压和频率调制率等重点问题进行了详细的讨论和分析.