坝陵河大桥桥位深切峡谷风剖面实测研究

用相控阵声雷达风廓线仪对坝陵河大桥桥址处深切峡谷中风剖面进行了实地观测,结果表明：在地形复杂的山区深切峡谷中,平均风剖面受峡谷地形影响较大,形态有时显得较为复杂而不规则,呈现锯齿形、正切变形或逆切变形等多样化。在峡谷的上半部,平均风速较大时其剖面相对较为规则,但不符合规范中描述平坦地貌平均风速剖面的幂函数形式,而具有e指数函数的变化规律。此外,统计显示,风向角在低空范围内受峡谷地形的影响要比在高空范围内严重,其在低空范围的变化幅度也要比在高空范围的变化幅度大。风迎角的散布范围和绝对值大小均随高度的增加呈减小的趋势。观测得到的峡谷湍流度大于平坦地貌湍流度的规范推荐值,同时峡谷湍流度具有一定的随机性,并且这种随机性随高度的增加而变大。     

双向梯度复合材料裂纹尖端应力强度因子研究

为了进一步改善梯度复合材料力学分析及设计水平,推导了一种适用于双向梯度复合材料断裂特性分析的梯度扩展单元法(XFEM).采用细观力学方法描述材料沿梯度方向变化的力学属性,通过线性插值位移场给出了4节点梯度扩展单元随空间位置变化的刚度矩阵,建立了结构的连续梯度有限元模型,并采用交互能量积分计算得到了裂纹尖端的应力强度因子(SIF).通过与已有文献结果对比验证了梯度扩展单元的优越性,并讨论了双向梯度结构中相关参数对SIF的影响规律,得到结论:梯度扩展单元能够提高梯度材料中裂纹尖端SIF的计算精度,其计算结果随着网格密度的增加迅速收敛于精确解;双向梯度结构的组份分布形式和属性梯度能够明显影响裂纹尖端的SIF;对于多裂纹双向梯度结构,裂纹间的相互作用增大了裂纹尖端的SIF,弹性模量大的一侧SIF较大.     

MSD对老旧飞机搭接结构完整性的影响

利用FRANC2D/L对含MSD某型飞机机翼蒙皮搭接接头进行了有限元分析,得到了不同分布钉载下MSD裂纹应力强度因子(SIF)随裂纹扩展历程变化的计算曲线,和已有的文献比较表明,本文数值结果精确,方法可靠。计算结果表明,孔壁受载方式对SIF影响不大,但对MSD裂纹扩展方向有明显的影响;相对于均匀分布和集中力,二次分布的钉载更接近于实际的孔壁受载方式,且在计算时,应考虑其它排钉孔的受载。最后探讨了基于力学的评估含MSD搭接结构完整性的方法。     

面向高轨目标的强度相干成像技术研究

强度相干成像技术是指利用地基强度相干阵列测量空间目标光强随机涨落的相干性,可获得目标的空间频谱模值,结合目标先验信息即可恢复目标光强分布图像.这种成像方法具有成像分辨力高、设备精度要求低、受大气湍流影响小等优点,目前已应用于恒星目标的成像观测领域,是一种有发展前景的地基光学成像手段.在综述强度相干技术原理与发展历程基础上,分析了利用强度相干阵列对高轨目标成像的可行性,认为在利用强度相干阵列对高轨目标成像过程中,主要存在空间频谱探测信噪比低和相位恢复复杂2大难题,提出利用激光主动照明对目标进行探测,同时采用符合计数方法和正则化优化方法可提高探测信噪比与相位恢复质量,对实现高轨目标成像有一定参考.     

Cosmic ray variations of solar origin in relation to human physiological state during the December 2006 solar extreme events

There is an increasing amount of evidence linking biological effects to solar and geomagnetic disturbances. A series of studies is published referring to the changes in human physiological responses at different levels of geomagnetic activity. In this study, the possible relation between the daily variations of cosmic ray intensity, measured by the Neutron Monitor at the Cosmic Ray Station of the University of Athens (http://cosray.phys.uoa.gr) and the average daily and hourly heart rate variations of persons, with no symptoms or hospital admission, monitored by Holter electrocardiogram, is considered. This work refers to a group of persons admitted to the cardiological clinic of the KAT Hospital in Athens during the time period from 4th to 24th December 2006 that is characterized by extreme solar and geomagnetic activity. A series of Forbush decreases started on 6th December and lasted until the end of the month and a great solar proton event causing a Ground Level Enhancement (GLE) of the cosmic ray intensity on 13th December occurred. A sudden decrease of the cosmic ray intensity on 15th December, when a geomagnetic storm was registered, was also recorded in Athens Neutron Monitor station (cut-off rigidity 8.53 GV) with amplitude of 4%. It is noticed that during geomagnetically quiet days the heart rate and the cosmic ray intensity variations are positively correlated. When intense cosmic ray variations, like Forbush decreases and relativistic proton events produced by strong solar phenomena occur, cosmic ray intensity and heart rate get minimum values and their variations, also, coincide. During these events the correlation coefficient of these two parameters changes and follows the behavior of the cosmic ray intensity variations. This is only a small part of an extended investigation, which has begun using data from the year 2002 and is still in progress.     

弹道靶中球模型非平衡可见光辐射的测量

使用中国空气动力研究与发展中心(CARDC)再入物理弹道靶和双狭缝式辐射计测量了多个状态的高超声速无烧蚀钢球模型非平衡流场的可见光辐射强度,并对实验技术和方法进行了讨论和分析.测量波段中心波长位于可见光的绿光波段(517.8nm、519.8nm),半宽度为6.6nm.球模型飞行速度为4.8~5.7km/s,靶室压力1333~10666Pa.实验数据与文献和计算结果一致,并发现高靶压状态辐射强度峰值下降的拖尾现象,其原因尚待分析.     

可压缩流体热线探针校准方法研究

在可压缩流体中利用热线技术进行湍流度测量时,其输出不仅与脉动速度有关,而且也与流体温度、密度紧密相关。因此,需要在与高速可压缩流体特征相似的校准装置中,在使用前对热线探针进行准确校准。本文提出了可压缩流体热线探针校准方法,建立了热线校准(工作)数学模型,并利用自建的热线校准风洞开展了热线校准实验和湍流度测量风洞试验验证,结果表明:热线校准方法可行,校准数学模型合理可靠,热线探针校准精度较高,湍流度测量结果可信,基本可满足高速可压缩流体湍流度测量的工程需要。     

一种航天器太阳电池阵供电能力计算方法

太阳电池阵为航天器提供能源,在型号研制和在轨运营过程中需对其供电能力进行计算,为此提出了一种航天器太阳电池阵供电能力的计算方法。首先,利用太阳电池片的地面测试数据得到标准测试条件(STC)下的电池片伏安模型,并利用电池片在轨等效光强和温度修正电池片伏安模型的光生电流、串联电阻和并联电阻等参数,得到电池片在轨伏安模型,然后,根据基尔霍夫定律推导出电池阵中电池片工作电压、电流以及旁路二极管和隔离二极管的输出情况,从而得到太阳电池阵的伏安模型。仿真结果表明,本文方法可以精确计算航天器在任意光强、温度和遮挡下的太阳电池阵伏安模型,可以精确分析旁路二极管和隔离二极管对太阳电池阵供电能力的影响,较已有方法计算精度提高20%。     

The dynamic chromosphere: Pushing the boundaries of observations and models

The interface between the bright solar surface and the million-degree corona continues to hold the key to many unsolved problems in solar physics. Advances in instrumentation now allow us to observe the dynamic structures of the solar chromosphere down to less than $0_{.}^{″}1$ with cadences of just a few seconds and in multiple polarisation states. Such observational progress has been matched by the ever-increasing sophistication of numerical models, which have become necessary to interpret the complex observations. With an emphasis on the quiet Sun, I will review recent progress in the observation and modelling of the chromosphere. Models have come a long way from 1D static atmospheres, but their predictions still fail to reproduce several key observed features. Nevertheless, they have given us invaluable insight into the physical processes that energise the atmosphere. With more physics being added to models, the gap between predictions and observations is narrowing. With the next generation of solar observatories just around the corner, the big question is: will they close the gap?     

基于近海海面观测的台风黑格比风特性研究

根据在博贺海洋观测站测得的0814台风黑格比三维风速时程,首先探讨了实测数据质量的判别准则及处理方法,进而研究了平均风场特性:风剖面、风攻角、梯度风高度以及脉动风场特性:湍流强度、阵风因子、时间尺度、积分尺度、脉动风速谱等。研究结果表明:近海海面指数律风剖面指数a远小于建筑结构荷载规范推荐值;台风风场结构本身存在3°～7°正攻角;在近海海面上阵风因子均值为1.23;顺风向湍流强度平均值为0.10,三向湍流强度的比值为1∶0.80∶0.43;水平向时间尺度基本上均小于30s,竖向时间尺度均小于10s;纵向和横向积分尺度较为接近,大于竖向积分尺度;不同区域的实测风速谱与各经验风速谱均存在一定差异,与von Karman谱吻合相对较好。