增强氟塑料干法制备工艺研究

对生产增强氟塑料的原材料P202和FR104两种聚四氟乙烯树脂性能进行了对比,采用“干法”制备工艺并对工艺参数进行改进,生产出FS-20d和FS-35d增强氟塑料。生产制品测试结果表明：“干法”制备工艺配方稳定、生产工艺稳定,制品的耐磨性能、耐高温性能、致密性、均匀性和相分散性均优于“湿法”制备工艺制品。     

Late stages of stellar evolution – Herschel’s contributions

Cool objects glow in the infrared. The gas and solid-state species that escape the stellar gravitational attraction of evolved late-type stars in the form of a stellar wind are cool, with temperatures typically ?1500 K, and can be ideally studied in the infrared. These stellar winds create huge extended circumstellar envelopes with extents approaching 10¹⁹${10}^{19}$ cm. In these envelopes, a complex kinematical, thermodynamical and chemical interplay determines the global and local structural parameters. Unraveling the wind acceleration mechanisms and deriving the complicated structure of the envelopes is important to understand the late stages of evolution of ∼97% of stars in galaxies as our own Milky Way. That way, we can also assess the significant chemical enrichment of the interstellar medium by the mass loss of these evolved stars. The Herschel Space Observatory is uniquely placed to study evolved stars thanks to the excellent capabilities of the three infrared and sub-millimeter instruments on board: PACS, SPIRE and HIFI. In this review, I give an overview of a few important results obtained during the first two years of Herschel observations in the field of evolved low and intermediate mass stars, and I will show how the Herschel observations can solve some historical questions on these late stages of stellar evolution, but also add some new ones.     

Dark Matter Particle Explorer:The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

The Dark Matter Particle Explorer (DAMPE) mission is one of the five scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Science (CAS) approved in 2011. The main scientific objective of DAMPE is to detect electrons and photons in the range of 5GeV-10TeV with unprecedented energy resolution (1.5% at 100GeV) in order to identify possible Dark Matter (DM) signatures. It will also measure the flux of nuclei up to above 500TeV with excellent energy resolution (40% at 800GeV), which will bring new insights to the origin and propagation high energy cosmic rays. With its excellent photon detection capability, the DAMPE mission is well placed for new discoveries in high energy-ray astronomy as well.      

带缘板阻尼块涡轮叶片减振特性研究

以某型带缘板阻尼块涡轮叶片为对象,采用二维整体-局部统一滑动模型,编制涡轮叶片振动响应分析程序。在此基础上系统地计算不同参数时带缘板阻尼块叶片的振动响应,分析了正压力、外激励对减振效果的影响。算例分析表明:同一外激励下,存在一最佳正压力可以使系统减振效果比较好;正压力不变时,外激励幅值大小的变化对叶片减振效果有较大影响;另外阻尼块对叶片起到调频作用。     

带弹支干摩擦阻尼器的转子振动控制 策略和方法

根据弹支干摩擦阻尼器的特点,提出弹支干摩擦阻尼器控制转子振动的方案,建立了基于主动弹支干摩擦阻尼器的比例积分控制(PI控制)和连续增益调度比例积分控制(连续GSPI控制)方法,对两种控制方法控制转子通过临界转速的振动进行了理论分析、数值仿真和试验验证,并分析了其特点.      

Status and Perspectives of Dark Matter Searches in China

In this paper, we give a review of direct detection searches reported by the DAMA (China as a Co-I), and indirect detection searches reported by the ATIC (China as a Co-I). We also outline the future plans of dark matter search in China.      

Dark matter in very poor galaxy groups

We have analyzed a sample of 7000 galaxies in the Local Supercluster (LS) (V < 3100 km/s) selected from the LEDA database [Makarov, D.I., Karachentsev, I.D. A new catalogue of multiple galaxies in the local supercluster small galaxy groups. Small Galaxy Groups ASP Confer. Ser. 209, 40–46, 2000]. We have derived physical properties of poor LS groups selected by dynamical and 3D-Voronoi tessellation methods. Median values of mass-to-luminosity ratios for poor LS groups selected by these methods are 50 M_⊙/L_⊙ and 34 M_⊙/L_⊙, respectively. Physical parameters of LS galaxy triplets in comparison with other samples were evaluated. We suggest that the Dressler effect is present even in such poor groups as galaxy triplets. The data suggest that dark matter haloes are associated with the individual galaxies for LS triplets, which we find are dynamically younger systems. This contrasts with the properties of the Interacting and Northern & Southern triplet samples. For these two samples, the data suggest that the dark matter resides in a common halo. The median values of the mass-to-luminosity ratios for LS triplets, Northern & Southern triplets, and Interacting triplets are 35 M_⊙/L_⊙, 47 M_⊙/L_⊙, and 13 M_⊙/L_⊙, respectively.     

多谐波法研究带有叶间干摩擦阻尼失谐叶盘系统的共振特性

提出一种高效的多谐波分析方法,以用于研究失谐对带有叶间干摩擦阻尼的叶盘系统共振特性的影响规律.该方法可准确预测叶盘系统在频域的受迫响应,其有效性用数值积分法进行了验证.利用该方法对带有叶间干摩擦阻尼的叶盘受迫振动响应进行了仿真计算,分析了叶盘系统在谐调和失谐两种情况下受耦合强度、黏性阻尼和干摩擦阻尼等系统参数影响下的共振特性.结果表明,提出的多谐波分析法能够高效地研究失谐对带有叶间干摩擦阻尼的叶盘系统共振响应的影响特征,尤其适合考虑各种系统参数的综合影响.