钝体入水时的水下声场的测量

对钝体入水时的水下声场进行了深入研究。在水中大约30个不同的测点上，测量了入水时产生的水中激波(声波)的压力，从而获得了激波的空间能量分布及其传播速度的实验数据。     

Relative ion Fe,C and O abundances in quiet time particle fluxes in the 23 SC

Using ACE and SOHO data the origin of quiet-time low-energy particle fluxes at 1 AU is studied in the 23rd solar cycle. One of the selection criteria of quiet-time periods is to demand that H/He < 10 provided that periods with noticeable contribution of remnants of gradual events have been excluded from consideration. Our results suggest different origin of 0.03–3 MeV/nucleon particles – different seed populations accelerated and different acceleration processes. During the ascending, maximum and descending phases of solar activity quiet-time ions consist of coronal particles accelerated to suprathermal energies in about a half of the quiet periods, the rest of quiet-time fluxes originates from particle acceleration in processes similar to those in small impulsive solar flares rich in Fe. At solar minimum the bulk solar wind particles serve as seed population.     

Use of principal component analysis in the identification of the spatial pattern of an ionospheric total electron content anomalies after China’s May 12, 2008, M = 7.9 Wenchuan earthquake

This paper uses principal component analysis (PCA) to determine the spatial pattern of total electron content (TEC) anomalies in the ionosphere post the China’s Wenchuan Earthquake of 12 May, 2008 (UTC) (M_w = 7.9). PCA and image processing are applied to the global ionospheric map (GIM) with transforms conducted for the time period 08:00–10:00 UT on 12 May 2008. Results show that at a height of approximately 200 km the anomaly is widespread and less intense; however, it becomes more localized with height reaching maximum intensity and localization at an altitude of 300 km. The spatial distribution is remarkably similar to that reported for a TEC anomaly previously identified as a precursor anomaly on May 9, 2008 for the same time period. Potential causes of the results are discussed with emphasis given to vertical acoustic gravity waves based on the spatial pattern identified.     

高声强混响室噪声试验典型声谱控制方案

不同的运载火箭其整流罩内的噪声声压级有较大差异。在进行卫星的整星噪声试验时,需要分析声谱条件、选取不同的参试设备、优化控制系统的参数设置,最后通过系统调试找到最佳的试验方案。文章以3种不同的声谱条件为例,根据试验设备的条件和能力,结合试验效果、技术上的可靠性、试验成本等因素综合考虑,选定最有效和可行的试验方案。既保证了试验能达到预定的目的,检验卫星经受高声强环境的能力,提高其可靠性,又能使试验易于实现且成本较低。     

“风云二号”卫星噪声试验高频段控制问题研究

文章对“风云二号” 04卫星噪声试验进行了回顾,其声谱控制未能完全满足试验大纲要求的原因主要有硬件配置、控制系统参数设置等方面。经过理论分析和调试检验,决定从3个方面来解决,即:高频电气换能器EPT-200作为必须参试的设备;试验过程中电气换能器的工作介质（液氮汽化并升温后的氮气）压力不能太低;控制参数可根据试验前调试的情况作适当的修正。最终圆满完成了该型号05卫星以及06卫星的噪声试验。     

On the early phase of relativistic solar particle events: Are there signatures of acceleration mechanism?

Many physical processes precede and accompany the solar energetic particles (SEP) occurrence on the Earth’s orbit. Explosive energy release on the Sun gives rise to a flare and a coronal mass ejection (CME). X-ray and gamma emissions are believed to be connected with flares. Radio emission is signature of disturbances traveling through the corona and interplanetary space. Particles can gain energy both in the flare and the accompanying wave processes. The beginning of the SEP events has the advantage of being the phase most close to the time of acceleration. Influence of interplanetary transport is minimal in the case of first arriving relativistic solar protons recorded by ground based neutron monitors in so called ground-level enhancements (GLE). The early phase of the SEP events attracts attention of many scientists searching for the understanding of particle acceleration. However, they come to the opposite conclusions. While some authors find arguments for coronal mass ejections as a sole accelerator of SEPs, others prove a flare to be the SEP origin. Here, the circumstances of SEP generation for several GLEs of the 23rd solar cycle are considered. Timing of X-ray, CME, and radio emissions shows a great variety from event to event. However, the time of particle ejection from the Sun is closer to maximum of X-ray emission than to any other phenomena considered. No correlation is found between the particle fluxes and the CME characteristics.     

The dust content of clusters of galaxies

We have statistically investigated the infrared luminosity of clusters of galaxies in comparison with the known tracers of the cluster mass like the X-ray luminosity and the cluster richness (e.g. the number of member galaxies). Our results show that there is a clear positive correlation of the infrared luminosity with the cluster mass. Quantitatively speaking, the infrared luminosity is on average 20 times higher than the X-ray luminosity. Moreover, the infrared luminosity increases with the redshift. This probably shows that a major part of this infrared luminosity is due to star formation in the member galaxies. Another possible contribution would be the thermal emission from dust particles in the diffuse intracluster medium. However our method does not allow us to infer conclusions about this second hypothesis. Depending on their size and abundance, such particles would contribute to the infrared luminosity of galaxy cluster and have an impact on the cooling function of the baryons and thus on the formation of the large scale structures. This is an important cosmological question which still remains open.     

悬停状态倾转旋翼噪声试验及数值计算

结合消声室试验和数值计算研究了悬停状态倾转旋翼气动噪声特性。消声室试验采用孤立倾转旋翼模型,测试了不同总距角和桨尖马赫数状态的气动噪声数据。数值计算基于CFD(computational fluid dynamic)结合FW-H(Ffowcs Williams-Hawkings)声学方程的方法,采用试验数据验证了计算模型的可靠性。分析了倾转旋翼的噪声传播特点以及拉力系数和桨尖马赫数对噪声总声压级的影响,并对比了孤立旋翼和双旋翼状态的气动噪声特性。结果表明:倾转旋翼噪声随着拉力系数和桨尖马赫数的增加均有所增加,维持旋翼拉力不变时降低桨尖马赫数虽然使得拉力系数增加,旋翼噪声水平仍然降低;倾转双旋翼噪声相对纵向平面对称分布,在多个方位角区域存在着局部最大值,这和双旋翼噪声传播时的相互叠加以及双旋翼间气动干扰相关。      

飞翼布局飞机武器舱综合流动控制技术研究

 针对飞翼布局飞机武器舱高强度气动噪声、内埋武器分离安全性和全机开舱附加阻力问题,以高速风洞气动噪声及气动力测量为研究手段,开展了基于前缘扰流片激励的武器舱综合流动控制技术试验研究。试验结果表明:对于飞翼布局飞机,武器舱开启对飞机气动性能有较大影响,巡航状态下,武器舱打开后使全机阻力增加了60%~110%;武器舱气动噪声高达185 dB;内埋武器分离过程中存在较大的抬头力矩,不利于武器分离。通过在武器舱前缘布置扰流片对剪切层施加激励,可以有效改善武器舱流动特性。巡航状态下武器舱开舱附加阻力最多降低20%;武器舱噪声降低5~8 dB;同时可以有效改善内埋弹分离特性。     

环形腔室径向宽度对加力燃油泵内流及性能影响

对某加力燃油泵内部非定常流动开展了系统的数值模拟,研究了不同环形腔室径向宽度条件下泵的外特性和内流特征.计算结果表明,缩小径向宽度可有效提高泵在不同流量下的扬程,且小流量工况增幅显著高于大流量,明显改善了小流量工作的不稳定性.对于大流量工况,环形腔室截面变小导致腔室内循环流量降低、沿程损失明显减小,是泵出口扬程提高的主要因素;而对于小流量工况,环形腔室截面变小使得扩散管主流贴近环形腔室,显著降低了叶轮流道扬程损失,有效提升了泵出口扬程.