Response of photosynthetic systems to salinity stress in the desert cyanobacterium Scytonema javanicum

The present study investigated the physiological and biochemical characteristics of Scytonema javanicum, a pioneer species isolated from desert biological crusts, under salinity stress. Pigment analysis showed that salinity decreased chlorophyll a and phycocyanin content, while low salinity increased carotenoid concentration and high salinity decreased carotenoid concentration. Salinity also inhibited CO₂ assimilation rate and photosynthetic oxygen evolution in this cyanobacterium. Chlorophyll a fluorescence transient parameters (φPo, φEo, ψO, RC/ABS, RC/CS, PI_ABS, and PI_CS) were decreased under salt stress, while dVo/dto(Mo), Vj and φDo were increased. The decrease of ETRmax and Yield and the change of chlorophyll a fluorescence transients showed that salt stress had an important influence on photosynthesis. These results indicated that the effects of salinity stress on photosynthesis in S. javanicum may depend on the inhibition of electron transport and the inactivation of the reaction centers, but this inhibition may occur in the electron transport pathway at the PSII donor and acceptor sites.     

火箭深弹水下减阻技术研究

基于Fluent软件,对火箭深弹的水下减阻技术进行了研究。提出了火箭深弹中部补气的减阻方式。通过对下潜速度和通气量2个影响因素的分析,得到了火箭深弹在8～100 m/s速度范围的流场计算结果。计算结果表明,中部补气能有效地减小阻力,最大减阻效率达到25%;火箭深弹在水中所受阻力随通气量的增大而减小,在通气量相同的条件下,减阻效率随下潜速度的减小而增大。计算结果与实验结果基本一致。     

尾缘锯齿修形对波瓣强迫混合排气系统性能影响

针对某涡扇发动机波瓣强迫混合排气系统建立了尾缘锯齿修形流场数值计算模型,通过三维数值模拟研究,得到了不同尾缘锯齿修形波瓣强迫混合排气系统流场的演变规律和热混合效率、总压恢复系数的变化规律.结果表明:在强迫混合排气系统出口截面处,热混合效率随修形量的增加而增大,总压恢复系数随修形量的增加而减少.1个三角形(1-SJ)锯齿修形模型的热混合效率最大,达到79.73%;2个梯形修形(2-TX)的综合效果最优,其热混合效率达到77.50%,总压恢复系数比1-SJ高出0.5%.      

电热破膜激波管及其PLIF测量系统的研制

探讨了用Nd：YAG脉冲激光器作为泵浦光源对激波管内瞬态非定常流场进行平面激光诱导荧光（Planar laser induced fluorescence,PLIF）测量的时序同步问题。由于该激光器需要预热以获得稳定的倍频输出,作者研制了低压大电流的电热破膜装置,实现对激波产生时机的控制。在大尺寸矩形截面的激波管上搭建了PLIF测量平台,并在此平台上进行了丙酮示踪流场显示和氢氧基分布测量。     

A synchrotron-based facility for the in-situ location,chemical and mineralogical characterization of ∼10 μm particles captured in aerogel

NASA’s Stardust mission collected dust from the coma of Comet Wild-2 on January 2nd, 2004, by direct capture into aerogel cells that flew through the dust coma at ∼6 km/s. Stardust collected several hundred comet particles >10 μm in size. These comet samples were delivered to Earth on January 15th, 2006. We developed a facility at the National Synchrotron Light Source at Brookhaven National Laboratory (Upton, NY, USA) for the in-situ characterization of ∼10 μm particles collected in aerogel. These analytical instruments allow us to perform extensive chemical, mineralogical, and size-frequency characterization of particles captured in aerogel. These analyses are conducted without any invasive extraction, minimizing the possibility of contamination or particle loss during preparation. This facility was used to determine the chemical composition, the oxidation state, the mineralogy and to provide an indication of the grain size of the Wild-2 particles before they were removed from the aerogel. This information provides a catalog of particle types, allowing a more reasoned allocation of the particles to subsequent investigators based on a relatively detailed knowledge of the chemical composition and mineralogy of each particle. These measurements allowed a comparison of the chemical and mineralogical properties of the Wild-2 particles with other types of extraterrestrial materials, including interplanetary dust particles and meteorites. The success of in-situ analysis for Wild 2 particles demonstrates that synchrotron-based facilities will be important for the analysis of particles collected in aerogel on future earth-orbiting satellites and spacecraft.     

Theoretical modelling of X-ray fluorescence signals for different lunar compositions and dependence on solar activity

We present a forward modelling technique for calculating the surface X-ray spectra for a variety of lunar terrains. Our calculations considered variations in solar fluxes from solar quiescent condition to large flare activity (M1 flare), and expected elemental concentrations in the target, as well as yield, instrumental, and viewing geometry parameters for X-ray induced fluorescence from the lunar surface. Additionally, we present estimates of anticipated XRF signals from prominent K_α lines observable by a collimated 14 cm² X-ray detector from a 100 km lunar orbit with ∼20 km spatial resolution. Our results show that Mg, Al and Si characteristic K_α lines can be observed for all solar conditions. The Ca K_α lines line can be differentiated from a fixed background during more energetic solar conditions such as C1 and M1 flares, whereas Ti and Fe lines are identifiable only during C1 and M1 solar flare conditions for Apollo 12 site composition. Both the K_α X-ray intensity ratios of Mg/Si and Al/Si correlate well with concentration ratios of Mg/Si and Al/Si, respectively, for B1 and M1 solar conditions. The K_α X-ray intensity ratios of Fe/Si and Ca/Si correlates with concentration ratios of Fe/Si and Ca/Si, respectively, for M1 solar condition. In principle, the modelling technique outlined here can be used to determine absolute elemental abundances (Mg, Al, Si, Ca, Ti and Fe) from X-ray spectra measured during recent and future lunar missions.     

焊接构件低温疲劳P-S-N曲线的研究

焊接构件的低温 P-S-N曲线是冬季构件抗疲劳设计的基础.在PLG-300 kN高频疲劳试验机上,测定了在-25℃环境下4种应力水平对应的焊接构件的疲劳寿命,并得出了其中值S-N曲线.采用小样本实验的单侧容限分析方法,利用对数疲劳寿命变异系数的经验取值,得出了焊接构件的低温P-S-N曲线.这种方法既简便又经济,但需要由进一步的实验来完善.     

面向太空环境应用的抗辐照有源光纤特性研究

针对太空恶劣辐射环境会造成光器件的光学性能下降或失效的问题,利用改良化学气相沉积法(MCVD)结合原子层沉积(ALD)掺杂技术制备铋铒共掺光纤(BEDF)和掺铒光纤(EDF),经不同辐照剂量的伽马射线处理后,对它们的光谱特性进行对比研究。光纤样品分别经0.3kGy、0.5kGy、0.8kGy和1.5kGy辐照处理,对比光谱发现BEDF的辐照诱导损耗(RIA)的增幅明显低于EDF,特别是经1.5kGy的辐照处理后,EDF的RIA比BEDF高1.93dB/m。EDF的荧光强度随辐照剂量的增加而降低,且低于未辐照前的荧光强度;而对于BEDF而言,其荧光强度随辐照剂量的增加先增加后减弱,且均高于未辐照的荧光强度。实验结果表明,BEDF具有一定抗辐照特性,对应用于太空环境具有重要研究意义。     

导弹海上补给指挥关系优化分析

针对导弹海上补给指挥关系的优化问题,首先提出了整合导弹海上补给指挥机构从而优化指挥关系的设想,继而分别建立了导弹海上补给指挥关系相应拓扑结构的时效熵和质量熵模型,并通过计算分析对比优化前后指挥关系的优劣,得出了与设想一致的结论。