钛合金表面抗激光涂层损伤特性及热效应影响研究

实验研究了钛合金和高反射型陶瓷涂层材料抗连续型激光烧蚀的损伤及温度分布特性，并从热效应影响角度对比分析了二者在抗激光损伤效果方面的差异性。研究结果表明：相比于钛合金，高反射型陶瓷涂层材料能有效增强钛合金基底抗激光损伤的能力；在同等激光功率密度辐照下，陶瓷涂层材料能有效提升钛合金基底耐受激光辐照的时间长度。实验结果表明该陶瓷涂层材料的激光损伤阈值比钛合金高约5.8倍。实验发现陶瓷涂层温升速率高于钛合金，但由于陶瓷材料具有较高的反射特性，以及良好的热吸收和热传导特性，因此能使由激光辐照产生的热量在其表面较快地扩散，而降低向基底方向传导的程度，最终提升陶瓷涂层的抗激光损伤阈值。     

Modeling the effects of green alternative on heat island mitigation of a meso level town,West Bengal,India

Urban heat island (UHI) is emerged as a ubiquitous phenomenon that affects the outdoor thermal comfort. Hence urban microclimatic studies using numeric simulation software to find out adaption strategies are attracting the great attention of researchers and policymaker. Number of scientists carried out their research on this topic using different tools and technique whereas ENVI-met model is the most widely used simulation tools. The present study intended to examine the implication of green infrastructure of the town on enhanced microclimatic condition and to evaluate the best suitable mitigation strategy modelling cool city with ENVI-met software (V4). Five greening condition such as existing UHI condition (C1), 100% greening of roof (C2), 100% greening of roof and walls (C3), 50% greening of roof and walls (C4) and: Plantation at suitable area with 50% greening of roof and walls (C5) have been taken into consideration for the microclimate simulation for all three selected sites. Among these five conditions, C3 for the open mid-rise and compact low-rise, C5 for the open low-rise are identified as one of the most suitable strategies which can reduce the air temperature of peak hours by 2.6 °C, 1.33 °C and 1.87 °C respectively. These models are validated by simple linear regression between simulated and existing air temperature in case of existing UHI condition (C1) and in all the cases coefficient of determination value is high such as for open mid-rise, compact low-rise and open low-rise, it is 0.92, 0.92 and 0.75 respectively. Therefore it can be concluded that the application of those strategies can improve the urban thermal environment as well as the outdoor thermal comfort of English bazaar Town and its surroundings.     

Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton

We present an analysis of seven clusters observed by XMM-Newton as part of our survey of 17 most X-ray luminous clusters of galaxies at z  0.2 selected for a comprehensive and unbiased study of the mass distribution in massive clusters. Using the public software FTOOLS and XMMSAS we have set up an automated pipeline to reduce the EPIC MOS and pn spectro-imaging data, optimized for extended sources analysis. We also developped a code to perform intensive spectral and imaging analysis particularly focussing on proper background estimate and removal. XMM-Newton deep spectro-imaging of these clusters allowed us to fit a standard β-model to their gas emission profiles as well as a standard MEKAL emission model to their extracted spectra, and test their inferred characteristics against already calibrated relations.     

低轨道带可变翼的平板型极高真空分子屏

本文计算了在低轨道自由飞行的平板型分子屏（ＷａｋｅＳｈｉｅｌｄＦａｃｉｌｉｔｙ）加了可变翼后，分子屏后实验区的压力分布。计算中考虑了分子屏和翼材料出气对实验区压力的影响。本文并对加可变翼和不加可变翼、考虑出气和不考虑出气几种情形进行了计算和比较。我们的结果表明：给轨道分子屏加上可变翼后，其实验区的压力可比不加可变翼降低一个数量级以上，压力达１０－１３Ｐａ。本文的研究表明，这种给轨道分子屏加可变翼的模型对更好的利用分子屏环境是非常有利的。     

费率受制于位相半马氏过程的风险模型

对带马氏链的线性和非线性系统，经过众多学者近20多年的努力，已取得一系列重要成果。然而，由于马氏链状态逗留时间服从负指数分布，使得这些成果在应用中有很大的局限性。本文首先探讨了位相半马氏过程的性质，然后以位相半马氏过程代替马氏过程，研究风险模型的相关问题，取得了与马氏链相同的研究成果，从而说明了位相半马氏过程在克服由马氏过程带来的局限性中的作用。     

螺旋桨滑流对飞机绕流影响的试验研究

在国产双涡桨支线飞机发展过程中，曾专门研究过螺旋桨滑流对飞机表面压力分布的影响。本文以此为基础，从滑流对飞机绕流影响出发，研究了螺旋桨滑流引起飞机气动特性的变化，重点讨论了气动特性变化的机理。     

热惯性对热冲击半无限体热应力影响非傅立叶效应研究

考虑超快速加热引起传热过程的非傅立叶效应,基于线性热弹性理论和表面热惯性特性,建立了带惯性第一类边界条件的半无限体的动态温度场、热应力场方程组。用拉普拉斯变换法对方程组进行求解。结果表明,快速加热在半无限体内产生温度场和应力场,且热和应力呈波动输运机制。讨论了温升率或热惯性对半空间温度场和应力场的影响,比较弹性波波速与热波波速之比动态热应力的影响。     

正态分布可靠寿命经典近似限的改进

本文给出了正态分布可靠寿命的又一个经典近似下限，经验证，本文所给出的结果的精度比已有的结果精度要高，可提供给可靠性工程人员使用。     

基于信息流电路可测试性的度量

准确地度量电路的可测试性是数字系统测试的重要问题之一。本文提出了一种基于信息流度量电路可测试性的方法,它表明可以将一个数字电路看成是一个信息处理系统。因此,电路的可测试性的度量值定义为电路输出的平均信息量与输入的平均信息量的最大值之比。文中给出了如何应用逻辑模拟软件来计算电路可测试性的度量值。对于由模块组成的电路,可以通过模块之间的一些特殊操作求得整个电路可测试性的度量值,本文也给出了方法及实例。文中还给出了应用本文提出的方法进行电路可测试性度量的实例,并与文[1,5]的方法得到的结果进行了比较,从而说明了本文方法的特点。