The population of massive stars in R136 from HST/FOC UV observations

New ultraviolet (1300 A, 3400 A),HST FOC observations have been used to derive the UV color-magnitude diagram (CMD) of R136, with the main scientific goal of studying the upper end of the stellar mass function at ultraviolet wavelengths where the color degeneracy encountered in visual CMDs is less severe. The CMD has been compared to a set of theoretical isochrones, which have been computed using the latest generation of evolutionary models and model atmospheres for early type stars. Wolf-Rayet stars are included. Comparison of theTheoretical andobserved CMD suggests that there are no stars brighter than M₁₃₀–11. We use the observed main sequence turn-off and the known spectroscopic properties of the stellar population to derive constraints on the most probable age of R136. The presence of WNL stars and the lack of red supergiants suggests a most likely age of 3±1 Myr. A theoretical isochrone of 3±1 Myr is consistent with the observed stellar content of R136 if the most massive stars have initial masses around 50 M.Bases on Observations with the NASA/ESA Hubble Space Telescope, obtained at the STScI, which is operated by AURA, Inc., under NASA contract NAS5-26555.Astrophysics Division, Space Science Department, ESA     

扩张管和燃料部分填充对PDE效能的影响

采用基于有限速率基元化学反应模型的网格自适应有限体积方法,数值模拟以脉冲爆轰发动机为背景的爆轰波通过扩张喷管的流场,研究了喷管形状及喷管充气状况对脉冲爆轰发动机推进性能的影响。结果表明,氢-氧混合物产生爆轰波的等截面爆轰管冲量在某一比例合适的部分填充时达到最大,而对较大扩张角的喷管来说,其冲量一般随喷管内可燃气体填充比例的增加而增加,比冲通常随可燃气体填充比例的减少而增加;合适的喷管和燃料填充系数能使比冲显著提高。     

气动谐振管加热振荡流动过程数值研究

为了了解气动谐振管加热现象的振荡流动过程，利用显式TVD－MacCormark格式数值求解二维轴对称雷诺平均N－S方程，获得了一个谐振循环中完整的喷嘴－谐振管系统的振荡流动湍流流场，结果表明，欠膨胀声速冲击喷流固有的流场不均匀性和不稳定性是谐振管加热现象产生的内在原因，激波耗散是谐振管主要的加热机理。     

Experimental Aspects of Mid-Frequency Pulsations (f≈10–100 mHz) in the Southern Polar Cap

We review the results obtained in the frequency range of Pc3 (22-100 mHz) and Pc4 (7-22 mHz) pulsations at Italian Antarctic stations in the southern polar cap (“Mario Zucchelli”, at Terra Nova Bay, TNB, 80^˚.S; “Concordia”, the Italian/French base at Dome C, DMC, 89^˚.S). The absence of a midnight enhancement in the pulsation power suggests a negligible substorm influence at extreme latitudes, while the sharp noon enhancement, which appears only at TNB, is determined by the closer proximity of the station to cusp related phenomena. The relationship between the frequency of the band-limited signals and the interplanetary magnetic field strength, the cone angle influence, and the higher correlation of the Pc3 power with the solar wind speed in the morning hours suggest a global scenario in which upstream waves would be mainly responsible for the mid-frequency activity in the polar cap. However, the polarization pattern is odd with respect to the predictions for tailward propagating modes.     

新型固态纳米团簇NaXe在核磁共振中的量子尺寸效应

介绍了从体材料、薄膜(面材料)至量子点材料的发展。讨论了纳米材料中量子尺寸效应的重要意义。在实验中,用Xe离子注入NaCl微晶的方法,获得了尺寸小于80 nm的新型固态纳米团簇NaXe,测得了这种新型纳米材料在核磁共振中化学位移的量子尺寸效应。     

雾化槽燃油雾化机理研究

本文从雾化槽的雾化过程、流场特点、档板结构以及油膜在翻越运动中的分布,来研究雾化槽的雾化机理。     

一种改进的Turbo码Log-MAP译码算法

在传统Turbo码Log-MAP译码算法的基础上,借鉴已有的简化算法,提出了一种改进的Log-MAP译码算法。仿真结果表明,新的算法在大大降低译码复杂度的同时较好地保持了译码性能,使其非常接近Log-MAP算法的译码性能;同时也非常有利于硬件实现。     

角速度波动率测量的数据处理和不确定度分析

本文在对角速度波动率测量技术研究的基础上，提出了一些自己的看法，并对一些相关术语进行了定义，同时，对角速度波动率测量方法的不确定度评定进行了分析。最后，通过数据处理软件对实验数据进行了分析和验证。     

混合移频静刚度法和直接扰动迭代法

本文对混合移频动柔度法的失代式进行等价变换，从而得到一个“变种”，该变种不包含混合移频系统的动柔度式F^△（λ*），这便消除了F^△（λ*）带来的近似性，另外，对直接扰动法也进行等价变换，引出可以省时地用于许多特征向量导数计算的直接扰动迭代法。最后，为了供读者参数，本文还导出了三种混合移频动柔度法的非迭代式，其中有两种恰好是另外两种动柔度法经混合移频后的非迭代式，这实际上已将另两种动柔度法也扩展到密集根情况了。