1.5MW风力机气动性能研究

研制了风力机专用试验平台并进行了验证试验,在此基础上,将该试验平台应用于1.5MW大型风力机1/16缩尺模型在12m×16m低速风洞的气动性能试验研究。通过对试验结果的分析,研究获得了桨距角对风能利用系数的影响规律,分析了不同叶尖速比下风轮转速急升和骤停现象与NH系列翼型气动特性的关系。论文还将试验结果与GH B laded软件计算结果进行了综合比较分析。研究表明,该风力机最大风能利用系数高于0.492。     

内置开孔隔墙的高速铁路隧道压力波数值模拟方法

基于一维可压缩非定常不等熵流动模型、薄壁孔口出流模型以及广义黎曼变量特征线法,发展了单列车通过内置开孔隔墙隧道的压力波数值分析方法.与国外试验结果比较验证本文建立的计算方法的正确合理性基础上,通过对不同开孔率的计算得出采用过大的开孔率将导致一维流动模型计算时出现较大的数值振荡,分析了计算结果震荡可能的—维流动模型适用性的原因.同时,通过对隔墙中开孔和不开孔的模拟计算,得出隔墙开孔可较大幅度的减缓压力波,为今后研究和隧道内设置开孔隔墙提供了有益的启示.     

乘波体构型飞行器的高超声速测压实验研究

乘波体构型是高超声速飞行器的重要气动布局之一。对某多目标优化设计的乘波体构型飞行器进行了高超声速测压实验,对其气动性能进行风洞实验验证。实验马赫数M=6和M=7,迎角α=-4°、-2°、0°、2°、4°、6°、8°。结果表明：该乘波体构型各部件气动性能良好。进气道唇口准确捕捉到压缩激波,激波位置与设计吻合。乘波体上表面流向压力变化不大,有利于减小乘波体飞行阻力。下表面经过进气口内压段时压力有明显的增大,后体膨胀效果显著。在设计状态下,该乘波体飞行器整体气动性能良好。     

面向过失速机动的风洞动态试验相似准则探讨

为进行更加准确的风洞试验,讨论了针对过失速机动的风洞动态试验的相似准则问题。从六自由度运动方程推导出了进行动态风洞试验需要满足的运动相似参数;从N—S方程中得到满足流动相似的相似参数。针对不同类型的风洞动态试验,提出了具体对应的相似参数作为主要的模拟量。得到的结论可以为风洞动态试验参数选择提供参考。     

Marangoni heat pipe: An experiment on board MIOsat Italian microsatellite

This article summarizes the activities in preparation of a microgravity experiment to be carried out by using a small technological payload onboard a microsatellite developed by the Italian Space Agency. A dedicated hardware will be developed to investigate innovative heat pipes filled with self-rewetting fluids, i.e. dilute aqueous alcoholic solutions with unique surface tension properties. After a general introduction of the scientific background, the paper is focused on the main activities in preparation of the flight experiment, on the design of the flight hardware and on the experimental planned procedure. The laboratory results achieved on ground in preparation of a flight experiment are also presented, including measurements of fluids physical properties and preliminary heat pipes performances characterization test. From the engineering point of view, the activities dealing with heat pipes filling and sealing are included. The activities for heat pipe characterization conclude the paper.     

Variations of the magnetosheath ion flux and geomagnetic activity

The magnetosheath plays a dominant role in the Sun–Earth connection because the magnetosheath field and plasma actually interact with the magnetosphere. The interactions change the magnetospheric magnetic field from its nominal value through a long chain of different processes. The change is usually described by geomagnetic indices and thus it can be expected that these indices would reflect changes in the magnetosheath. The present paper analyzes the relation between geomagnetic activity characterized by changes of the K_p, D_ST and AE indices and ion flux measured in the night-side magnetosheath. The results suggest a weak dependence of the D_ST index on the ion flux in the inner magnetosheath that is connected with a magnetopause displacement. On the other hand, fluctuations of the ion flux in the analyzed frequency range do not correlate with any of the indices.     

捕获轨迹系统并联机构地面标定方法

捕获轨迹系统（CTS）是一种先进的预测外挂物投放轨迹的试验系统，普遍采用六自由度（6-DoF）串联机构作为其运动机构，串联机构因惯性力大和关节累积误差大使其定位精准度不足。相比串联机构，并联机构具有惯性力小和关节误差不累积等优点。采用6-PTRT并联机构作为CTS试验系统的六自由度运动机构，在空间受限的风洞环境中对CTS并联机构进行地面标定：提出动平台位姿的测量和计算方法，建立包含直线驱动平台安装夹角修正的标定模型，并基于非线性最小二乘法辨识结构参数。辨识后CTS并联机构的位移定位准度优于0.1 mm，姿态定位准度优于0.05°，最后以CTS并联机构和常规攻角机构进行8#标模的对比风洞试验。风洞试验结果表明，CTS并联机构的风载定位准度满足测力试验精准度要求。     

带控制律CTS试验的实现

FL24风洞在国内首次进行了带控制律的CTS试验,这是改进捕获轨迹试验方式的一次探索。文中对国内外研究现状、试验技术原理、实现过程进行了阐述。试验结果表明在加控制律的CTS试验中导弹的滚转角和偏航角输出趋稳,呈有控状态。     

先进风洞气源系统的研制与运行

系统包括空气压缩、空气处理、储气、冷却水供应和中央监控等五个分系统,空压机的吸入流量为248m3 min,排气压力为2.4MPa,成品气常压露点达-38℃,可以满足一座0.6m量级的高速风洞对气源的需要。该系统在与800m3储气容积配套时,能保证在气体流量达140kg s、持续时间达40s的风洞试验中,其总温变化不超过1.5K。     

Substorms and Their Solar Wind Causes

Consequences of the solar wind input observed as large scale magnetotail dynamics during substorms are reviewed, highlighting results from statistical studies as well as global magnetosphere/ionosphere observations. Among the different solar wind input parameters, the most essential one to initiate reconnection relatively close to the Earth is a southward IMF or a solar wind dawn-to-dusk electric field. Larger substorms are associated with such reconnection events closer to the Earth and the magnetotail can accumulate larger amounts of energy before its onset. Yet, how and to what extent the magnetotail configuration before substorm onset differs for different solar wind driver is still to be understood. A strong solar wind dawn-to-dusk electric field is, however, only a necessary condition for a strong substorm, but not a sufficient one. That is, there are intervals when the solar wind input is processed in the magnetotail without the usual substorm cycle, suggesting different modes of flux transport. Furthermore, recent global observations suggest that the magnetotail response during the substorm expansion phase can be also controlled by plasma sheet density, which is coupled to the solar wind on larger time-scales than the substorm cycle. To explain the substorm dynamics it is therefore important to understand the different modes of energy, momentum, and mass transport within the magnetosphere as a consequence of different types of solar wind-magnetosphere interaction with different time-scales that control the overall magnetotail configuration, in addition to the internal current sheet instabilities leading to large scale tail current sheet dissipation.