Sharp boundaries of solar wind plasma structures and their relationship to solar wind turbulence

Sharp (<10 min) and large (>20%) solar wind ion flux changes are common phenomena in turbulent solar wind plasma. These changes are the boundaries of small- and middle-scale solar wind plasma structures which can have a significant influence on Earth’s magnetosphere. These solar wind ion flux changes are typically accompanied by only a small change in the bulk solar wind velocity, hence, the flux changes are driven mainly by plasma density variations. We show that these events occur more frequently in high-density solar wind. A characteristic of solar wind turbulence, intermittency, is determined for time periods with and without these flux changes. The probability distribution functions (PDF) of solar wind ion flux variations for different time scales are calculated for each of these periods and compared. For large time scales, the PDFs are Gaussian for both data sets. For small time scales, the PDFs from both data set are more flat than Gaussian, but the degree of flatness is much larger for the data near the sharp flux change boundaries.     

Galactic Wind: Mass Fractionation and Cosmic Ray Acceleration

The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×10¹⁸ eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall Cosmic Ray spectrum.     

某型工程车多功能检测仪的硬件设计

设计的检测仪用于检测某型工程车的电控系统,以51单片机作为中央处理单元,以MAX392多路选择器实现多路选通,以CPLD扩展外围接口,可较好地实现信号的采集、存储和信息显示等功能。检测仪还具有代用功能,在紧急情况下可代替原车电控系统进行工作。     

0.1米低温风洞的设计

本文阐述了我国首次设计和建造的低温风洞的设计特点及共性能。这是一座以风扇驱动的闭口回流式风洞,用氮气作试验气体。试验段为0.1米的方形截面。计运转参数范围为:M=0.04～0.40,P_t=101.2 kPa～202.6kPa,T_t=79K～320K。试验时间为半小时。风洞壳体是用铝合金制造的,外部用超细玻璃棉绝热。风扇用交流电机拖动,转速用变频控制。     

八十年代风工程

本文扼要地回顾了推动风工程发展成为一门新兴独立学科以来的重大事件,并介绍了八十年代在该学科领域内取得的主要进展和研究动向。     

风洞天平不回零校正及修正方法研究

本文报告了一台典型的六分量天平在瑞典航空研究院 MK6校正架上进行回零校正与不回零校正的比较,弄清了不回零校正与回零校正的差别,然后用三种修正方法对不回零校正的载荷进行修正,发现直接投影法修正的效果最好,此方法已用到 FFA 新建的1.5米跨音速风洞的校正架上。     

对B2C领域两种营销渠道形式的比较探析

在B2C领域,传统营销渠道与网络营销渠道是一对相互竞争的矛盾。网络营销渠道是新生事物,凭借低成本优势得以迅速成长。传统营销渠道根基雄厚,且更贴近消费者的需求,因此仍吸引着大多数的消费者。网络营销渠道如何进一步发展,传统营销渠道如何吸收新的元素,不对两种营销渠道进行比较,是不能获得满意的答案的,而比较这两者之间的相对劣势比比较它们的优势更能引发思考。     

大型飞机高速气动力关键问题解决的技术手段及途径

大型飞机采用超临界机翼,并具有尺度大、飞行雷诺数高等特点,其研制中必须解决好高升阻比机翼、翼身组合体设计,推进系统/机体一体化设计,抖振特性、静气动弹性特性预测及超临界机翼流动控制等高速气动力问题。要解决这些关键气动力问题,必须进行一系列相关的大型高速风洞试验,以及解决相应的试验技术问题。     

国外风洞试验的新机制、新概念、新技术

风洞是空气动力学研究的重要地面试验设备,是保证一个国家航空航天处于领先地位的基础研究设施。面对新世纪航空航天领域的激烈竞争,世界发达国家加强了新概念风洞研制,改革风洞运行机制,一些新技术也在大型生产性风洞得到应用。     

海沧大桥气动弹性特性风洞试验研究

位于东南沿海台风多发地区的厦门海沧大桥是一座中跨达648m的三跨悬索桥，主梁断面采用流线型钢箱梁。通过气动弹性模型风洞试验，研究了该桥在运营及五个典型施工状态的颤振稳定性和抖振特性。