原子氧与真空紫外线协同效应对有机涂层的降解作用

为研究真空紫外与原子氧的协同作用,进行了环氧树脂和有机硅树脂的原子氧/真空紫外交互的地面模拟实验,结果表明:在交互作用中,对有机涂层破坏的主导因素是原子氧,真空紫外线起到协同作用,在切断有机高分子材料化学键的同时,为原子氧提供了反应基,加速了原子氧的反应速率.对比真空紫外辐照和原子氧/真空紫外交互实验结果分析中可以发现,有机硅树脂是较好的耐真空紫外辐射和原子氧侵蚀的有机涂层材料.     

H+辐照前后C-SiC 涂层的红外吸收光谱研究

对在不锈钢基体上用离子束混合技术沉积的C－SiC涂层，进行了二次离子质谱（SIMS）及傅氏变换红外吸收光谱（FI－IR）的分析。研究了不锈钢基体涂覆H＋辐照前后的氢浓度分布以及H^ 辐照前后涂层的红外光谱振动吸收峰的变化，对SiC涂层阻氢的机理进行了探讨。     

激光辐照强化技术的实验研究

 本文介绍了激光辐照强化技术在材料、结构方面的研究概况。在材料激光辐照参数优选的基础上,对Y7机长桁接头进行了辐照处理,并进行了模拟疲劳实验,研究了辐照参量对疲劳寿命的影响。试验结果表明辐照强化处理能显著地提高构件的疲劳寿命。     

Ultraviolet 3D digital image correlation applied for deformation measurement in thermal testing with infrared quartz lamps

In thermal-structural testing of hypersonic materials and structures, deformation measurement on the front surface of an object directly heated by quartz lamps is highly necessary and very challenging. This work describes a novel front-surface high-temperature deformation measurement technique, which adopts ultraviolet 3D digital image correlation (UV 3D-DIC) to observe and measure the high-temperature deformation fields on front surfaces directly heated by quartz lamps. Compared with existing blue light DIC techniques, the established UV 3D-DIC, which combines UV CCD camera, active UV illumination and bandpass filter imaging, can effectively suppress the strong disturbing light emitted by the quartz lamps and the heated sample itself during heating process. Two experiments were carried out to verify the robustness and accuracy of the developed technique: (1) direct observation of front surfaces of a hypersonic thermal structure sample heated from room temperature to 1050 °C, and (2) front-surface thermal stain and coefficient of thermal expansion (CTE) measurement of an Inconel 718 sample up to 800 °C. The well matched strain and CTE results with literature data show that UV 3D-DIC system is an effective technique for front-surface deformation measurement and has great potential in characterizing deformation response of hypersonic materials and structures subjected to transient aerodynamic heating.     

均苯型聚酰亚胺薄膜在质子辐照下的力学性能退化试验研究

聚酰亚胺薄膜广泛应用于航天器热控结构和太阳帆等充气展开结构中,由于暴露在航天器表面,受到各种空间环境效应的影响,其力学性能会发生退化。文章对不同通量、注量和温度条件下质子辐照对均苯型聚酰亚胺薄膜力学性能的影响进行了模拟试验研究。研究发现,当质子通量较低时,质子通量的增加对薄膜力学性能的影响微弱;当质子通量持续增加,薄膜的抗拉强度和断裂伸长率呈近似线性下降;当质子注量增加到一定程度后,薄膜的抗拉强度和断裂伸长率下降速率变缓;薄膜在低温辐照下比在高温辐照下更容易发生脆性断裂。     

热控涂层GEO带电粒子辐射效应加速试验方法

文章研究热控涂层GEO带电粒子辐射效应加速试验的参数确定方法。根据轨道带电粒子辐射环境的特点,以效应等效为原则,建立了利用单一能量带电粒子产生的辐射效应模拟轨道带电粒子辐射效应时的等效注量率计算方法,称之为等效能谱模拟技术;并建立了利用高注量率来提高加速试验效率的加速因子计算方法,称之为加速试验的加速因子确定技术。利用这两项技术,研究设计了防静电Kapton二次表面镜GEO电子辐射效应模拟试验的参数。     

The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less than half a pc in these galaxies, and from GALEX far-UV and near-UV wide-field, low-resolution imaging of the entire galaxies. Both datasets allow us to study the hierarchical structure of star formation: the youngest stellar groups are the most compact, and are often arranged within broader, sparser structures. The derived recent star-formation rates are rather similar for the two galaxies, when scaled for the respective areas. We show how uncertainties in metallicity and type of selective extinction for the internal reddening may affect the results, and how an appropriate complement of UV filters could reduce such uncertainties, and significantly alleviate some parameter degeneracies.     

The status and future of EUV astronomy

The Extreme Ultraviolet wavelength range was one of the final windows to be opened up to astronomy. Nevertheless, it provides very important diagnostic tools for a range of astronomical objects, although the opacity of the interstellar medium restricts the majority of observations to sources in our own galaxy. This review gives a historical overview of EUV astronomy, describes current instrumental capabilities and examines the prospects for future facilities on small and medium-class satellite platforms.     

Luminous star-forming galaxies in the SDSS-GALEX database

We use the combined photometric GALEX + SDSS database to look for populations of luminous blue star-forming galaxies. These were initially identified from such a sample at redshifts near 0.4, using SDSS spectra. We make use of the NUV, g, and i colour index previously defined in our previous paper, to separate stars and QSOs, to locate more of these unusual galaxies, to fainter limits. They are found in significant numbers in two different regions of the related colour-magnitude plot. Within these regions, we use the ensemble 7-colour photometry (FUV, NUV, u, g, r, i, z) to postulate the populations of blue star-forming galaxies at redshifts near 0.4 and 1.0, from a full photometric sample of over half a million.     

S781白漆电子辐照后光学性能退化的恢复与保护

为了深入认识和抑制航天器材料空间辐照损伤在地面环境中的恢复,在模拟的空间环境下对S781白漆进行了90keV电子辐照试验。研究了电子辐照后,试样分别在真空环境下、真空室注入空气后和空气中储存几小时后辐照诱发的光谱反射系数和太阳吸收比的变化。结果表明,S781白漆光学性能退化的恢复主要发生于与空气接触的数分钟内。此外,液氮环境对S781白漆的电子辐照损伤和光学性能退化具有保护作用。液氮的保护机制不仅在于它抑制了氧在材料表面的化学吸附,还在于它对辐照诱发缺陷的冻析效应。