LENS风洞试验返回器模型气动热特性模拟

国家数值风洞高超声速流动模拟软件HyFLOW的研制对打破国外同类软件的技术壁垒具有重要意义。与国外DPLR软件进行了对比研究，同时系统介绍了HyFLOW软件求解器的数值方法、物理化学模型以及壁面催化特性计算模型等主要方法，采用典型算例对有限催化模型进行了数值验证，最后基于LENS风洞试验146 mm返回器标模外形开展了高超声速气动热特性数值模拟。研究结果表明，HyFLOW软件在高超声速热化学非平衡流动模拟与评估方面的气动力计算精度高，与国外同类软件DPLR相当，同时其壁面催化条件下的气动热计算精度可靠，可信度高。     

飞翼模型高速风洞PIV试验研究

对小展弦比飞翼标模在2.4米跨声速风洞中创新开展了PIV试验。对空风洞进行了测速校核,并对小展弦比飞翼标模开展了二维、三维涡迹PIV测试,试验马赫数为0.4~0.9。测试结果表明,2.4m风洞PIV试验数据具有较高的准确度,M≤0.8时空风洞测速结果与理论值相差不超过1%,M=0.9时相差不超过2%。小展弦比飞翼标模测试结果显示,M数增大使机翼尾涡涡量和切向速度增大,涡核向内展向方向移动。前缘涡与上翼面分离具有密切关系:当M=0.8、α≤12°时,翼梢测试截面的前缘涡尚未破裂,上翼面未发生显著的流动分离;当α≥13°时,前缘涡破碎时机提前,当地后1/2弦长区域产生了比较明显的流动分离。     

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.     

Effects on winter circulation of short and long term solar wind changes

Indices of the North Atlantic Oscillation and the Arctic Oscillation show correlations on the day-to-day timescale with the solar wind speed (SWS). Minima in the indices were found on days of SWS minima during years of high stratospheric aerosol loading. The spatial distribution of surface pressure changes during 1963–2011 with day-to-day changes in SWS shows a pattern resembling the NAO. Such a pattern was noted for year-to-year variations by Boberg and Lundstedt (2002), who compared NAO variations with the geo-effective solar wind electric field (the monthly average SWS multiplied by the average southward component, i.e., negative Bz component, of the interplanetary magnetic field). The spatial distribution of the correlations of geopotential height changes in the troposphere and stratosphere with the SWS; the geo-effective electric field (SWS∗Bz); and the solar 10.7 cm flux suggests that solar wind inputs connected to the troposphere via the global electric circuit, together with solar ultraviolet irradiance acting on the stratosphere, affect regional atmospheric dynamics.     

Electron density inversed by plasma lines induced by suprathermal electron in the ionospheric modification experiment

Incoherent scatter radar (ISR) is the most powerful ground-based measurement facility to study the ionosphere. The plasma lines are not routinely detected by the incoherent scatter radar due to the low intensity, which falls below the measured spectral noise level of the incoherent scatter radar. The plasma lines are occasionally enhanced by suprathermal electrons through the Landau damping process and detectable to the incoherent scatter radar. In this study, by using the European Incoherent Scatter Association (EISCAT) UHF incoherent scatter radar, the experiment observation presents that the enhanced plasma lines were observed. These plasma lines were considered as manifest of the suprathermal electrons generated by the high-frequency heating wave during the ionospheric modification. The electron density profile is also obtained from the enhanced plasma lines. This study can be a promising technique for obtaining the accurate electron density during ionospheric modification experiment.     

用于BVI噪声试验的新型涡发生器设计与分析

针对直升机特有的旋翼桨/涡干扰(Blade vortex interaction,BVI)噪声计算精度低且试验数据缺乏问题,也为了开展旋翼气动噪声特性分离方法的验证试验研究,本文设计了一种能够用于BVI噪声试验的新型多段翼型组合式涡发生器。首先通过CATIA软件建立涡发生器出口端翼型段在不同迎角下的试验模型,再使用FLUENT软件建立涡发生器的流场仿真计算模型,比较分析了不同翼型段迎角下的涡流流场。随后用粒子图像测速法(Particle image velocimetry,PIV)技术系统测量了不同翼型段迎角、距离涡发生器出口端的长度及流速等参数变化下的涡流流场,对不同试验状态下的涡核、涡强等参数进行了对比分析。针对涡量偏弱的缺点,对传统单级涡发生器进行了改进,设计研发了双级涡发生段。试验证明其能产生更强且稳定的涡,为BVI噪声试验提供了模拟的桨尖涡,试验结果表明了涡发生器的有效性。     

海上双馈电机开路故障容错性能评估

海上风电机组面临故障率高、停运损失大等问题,迫切需要及早发现运行故障、及时提供容错机制。构建基于西蒙决策理论的双馈风力发电机开路故障容错设计方案,选取电能质量和风力发电机组可靠性作为典型评估指标。结合双馈风力发电机组机侧变流器单相开路故障容错案例,给出量化的容错性能指标。结果表明及时有效的故障容错机制能够提高海上风电场的可用率,避免故障恶化,降低故障带来的经济损失。     

An experimental system for release simulation of internal stores in a supersonic wind tunnel

Aerodynamic parameters obtained from separation experiments of internal stores in a wind tunnel are significant in aircraft designs. Accurate wind tunnel tests can help to improve the release stability of the stores and in-flight safety of the aircrafts in supersonic environments.A simulative system for free drop experiments of internal stores based on a practical project is provided in this paper. The system contains a store release mechanism, a control system and an attitude measurement system. The release mechanism adopts a six-bar linkage driven by a cylinder, which ensures the release stability. The structure and initial aerodynamic parameters of the stores are also designed and adjusted. A high speed vision measurement system for high speed rolling targets is utilized to measure the pose parameters of the internal store models and an optimizing method for the coordinates of markers is presented based on a priori model. The experimental results show excellent repeatability of the system, and indicate that the position measurement precision is less than0.13 mm, and the attitude measurement precision for pitch and yaw angles is less than 0.126°, satisfying the requirements of practical wind tunnel tests. A separation experiment for the internal stores is also conducted in the FL-3 wind tunnel of China Aerodynamics Research Institute.     

扩压叶栅剪敏液晶试验与图像处理

基于剪敏液晶涂层(SSLCC)材料的光学特性,发展了适合于内流场狭小空间环境下的SSLCC边界层流动显示技术:设计并加工了微型摄像头-发光二极管(LED)组合式图像采集设备解决拍摄光路问题;基于二维SSLCC图像与三维模型的空间映射关系,建立了真实模型的三维重构方法;通过SSLCC图像光谱Hue色相值转化,实现了液晶图像信息的定量分析。以西北工业大学高亚声速平面叶栅风洞为平台,开展了某扩压叶栅吸力面边界层流态的剪敏液晶流动显示试验。结果表明:所发展的剪敏液晶显示技术可进行叶栅内流场边界层的流态测量;所建立的图像处理方法可为边界层流动特征的辨识及其特征位置确定提供技术支撑;在来流马赫数为0.12、攻角为0°的条件下,叶片吸力面边界层沿流向依次经历了层流边界层分离、再附着及转捩为湍流状态的过程,且边界层的发展受叶栅角区分离流动影响,造成其前缘分离区减小,再附着点和边界层转捩位置向前缘移动。     

张力腿漂浮式风力机的运动响应计算

漂浮式风力机与近海桩基式风力机、陆上风力机差异很大,特别是漂浮平台设计复杂,对仿真工具要求更高。海上风力机除受气动载荷之外,还需进一步考虑海洋环境所施加的各种其他载荷。采用自由涡尾迹方法计算风力机气动性能,分别采用线性波和PM频谱模拟波浪运动并应用Morison方程计算波浪载荷。构建张力腿漂浮平台结构动力学方程,以气动载荷和波浪载荷为激励,得到平台响应,并反馈至气动计算,从而完成气动、结构和水动的耦合计算。最后以大型风力机NH1500为例,对张力腿式海上风力机进行仿真模拟,对比分析来流风速、浪高和波浪入流角对漂浮平台运动和风力机气动性能的影响,采用PM频谱模拟真实海况并计算漂浮式风力机动态响应,为漂浮式风力机设计提供了依据。