Photolytic behaviour of methane at Lyman-α and 248 nm: Studies in the frame of a simulation program of Titan’s atmosphere (S.E.T.U.P.)

This paper first describes briefly some of the forefront global simulations of Titan’s atmosphere that have been carried out up to now. In these experiments, an initial gaseous mixture of N₂/CH₄ is submitted to a single energy source and the retrieved gas and/or solid phase(s) is/are analyzed by different techniques.     

Propagation and interaction of interplanetary transient disturbances. Numerical simulations

We study the heliocentric evolution of ICME-like disturbances and their associated transient forward shocks (TFSs) propagating in the interplanetary (IP) medium comparing the solutions of a hydrodynamic (HD) and magnetohydrodynamic (MHD) models using the ZEUS-3D code [Stone, J.M., Norman, M.L., 1992. Zeus-2d: a radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. i – the hydrodynamic algorithms and tests. Astrophysical Journal Supplement Series 80, 753–790]. The simulations show that when a fast ICME and its associated IP shock propagate in the inner heliosphere they have an initial phase of about quasi-constant propagation speed (small deceleration) followed, after a critical distance (deflection point), by an exponential deceleration. By combining white light coronograph and interplanetary scintillation (IPS) measurements of ICMEs propagating within 1 AU [Manoharan, P.K., 2005. Evolution of coronal mass ejections in the inner heliosphere: a study using white-light and scintillation images. Solar Physics 235 (1–2), 345–368], such a critical distance and deceleration has already been inferred observationally. In addition, we also address the interaction between two ICME-like disturbances: a fast ICME 2 overtaking a previously launched slower ICME 1. After interaction, the leading ICME 1 accelerates and the tracking ICME 2 decelerates and both ICMEs tend to arrive at 1 AU having similar speeds. The 2-D HD and MHD models show similar qualitative results for the evolution and interaction of these disturbances in the IP medium.     

捷联惯导方位大失准角对准研究

在游动方位角坐标系下建立了方位大失准角条件下的SINS初始对准误差模型.在静基座下验证了该误差模型在方位大失准角情况下的滤波效果,比较分析了不同方位失准角的滤波收敛情况,并与线性模型进行滤波比较.最后,将该模型用于动基座的初始对准.静基座和动基座下的初始对准结果表明所提出的SINS误差模型是正确有效的.     

抑涡孔气膜冷却的大涡模拟

采用大涡模拟研究抑涡孔气膜冷却的流动和换热机理.通过与相同工况下圆孔气膜冷却流场的湍流结构进行比较分析,得出辅孔射流与主孔射流之间的干涉作用,并探索大尺度湍流结构影响气膜冷却效率的物理机制.结果表明:①辅孔射流抑制主孔射流形成的反转涡对的尺寸和强度,并为主孔射流的卷吸提供冷气补充;②由于上游辅孔出流冷气的保护作用以及对主孔出口尾缘低压区的冷气补充作用,主孔射流在气膜孔出口处温度没有急剧升高;③由于辅孔射流的干涉作用,主孔射流并未形成完整的发卡涡结构,而是无规律的近壁条带结构,减少了冷气和主流的掺混,并使冷气更好覆盖和冷却壁面.      

波音737—200／300／500飞机尾部结构疲劳裂纹的探伤检查

波音系列飞机一定时间后,飞机尾部结构出现疲劳裂纹,需用涡轮检测法进行损伤检查。     

亚格子模型对泵喷推进器宽带非定常力预测的影响研究

为了研究亚格子模型对泵喷推进器非定常流动与宽带非定常力预报结果的影响,采用分块结构化网格建立了模型尺度下艇后泵喷推进器的计算模型,并进行了大涡模拟数值计算。从艇尾非定常流场特征量和推进器转子脉动载荷两个方面对比了三种不同亚格子模型计算结果的差异,并分析了泵喷内部流动与转子非定常力间的内在联系。研究结果表明：三种亚格子模型均能得到含有叶频宽带峰的轴向推力谱,且整体趋势相近。泵喷转子上游的湍流强度和尺度的分布对亚格子模型较敏感,其中Smargrinsky-Lilly模型得到的湍流强度较强,尺度较大,该模型下的湍流谱在非平衡区量级较大,但由低频向高频的衰减较快,并且预测到的分离区范围大,导叶尾缘脱落涡分散,导致转子上游来流空间分布不均程度较强。对于转子叶片上的载荷脉动,Smargrinsky-Lilly模型预测的推力谱中线谱成分明显,并且叶频处宽带谱峰“陡峭”,而WALE模型和KET模型的结果宽带特性较强,对比非定常推力测试结果可知,WALE模型和KET模型更适于该问题宽带非定常力预测。     

轮控小卫星姿态大角度机动递阶饱和控制器设计

针对采用反作用飞轮的小卫星姿态大角度机动控制，在反作用轮输出力矩受限、速率饱和的约束条件下，采用递阶饱和方法，即限制卫星每次姿态机动的最大偏差，对姿态偏差进行逐次消除。在毋需获知最优机动轨迹规划的情况下，可用于卫星任意时刻的姿态捕获和机动控制。数学仿真结果表明，本文设计的控制算．去能够实现快速姿态机动任务，具有良好的鲁棒性。     

一种剪切修正的涡黏性亚格子模型及其在槽道湍流中的应用

提出了一种利用壁面附近强剪切对涡黏系数进行修正的亚格子模型,称为剪切修正的涡黏模型.该模型能使涡黏系数在壁面附近自动满足壁面修正,在脉动为零的地方,涡黏系数自动为零,保证了壁面附近涡黏系数趋于零的特性.用该模型对槽道湍流壁面无吹吸、有吹吸,较低和较高雷诺数的情况进行了数值模拟,与直接数值模拟的结果进行了对比,结果吻合较好.      

室火轰燃的大涡模拟

采用一套修正的适用于低马赫数浮力流的N-S方程组来描述火灾场,运用Smagorinsky亚格子模型的大涡模拟方法对室内池火的轰燃发展过程进行了数值模拟,把模拟与实验结果进行了对比和分析。结果表明,该方法能较好地预测轰燃。同时模拟结果显示火焰区向房间后部偏转稍大,近壁处温度预测的误差大一些,随着亚格子模型的不断完善和计算能力的提高,用该技术来预测轰燃现象会更加准确。     

The BOSS and BIOMEX space experiments on the EXPOSE-R2 mission: Endurance of the desert cyanobacterium Chroococcidiopsis under simulated space vacuum,Martian atmosphere,UVC radiation and temperature extremes.

The proposed space experiments BOSS (Biofilm Organisms Surfing Space) and BIOMEX (BIOlogy and Mars experiment) will take place on the space exposure facility EXPOSE-R2 on the International Space Station (ISS), which is set to be launched in 2014. In BOSS the hypothesis to be tested is that microorganisms grown as biofilms, hence embedded in self-produced extracellular polymeric substances, are more tolerant to space and Martian conditions compared to their planktonic counterparts. Various microbial biofilms have been developed including those obtained from the cyanobacterium Chroococcidiopsis isolated from hot and cold deserts. The prime objective of BIOMEX is to evaluate to what extent biomolecules are resistant to, and can maintain their stability under, space and Mars-like conditions; therefore a variety of pigments and cell components are under investigation to establish a biosignature data base; e.g. a Raman spectral library to be used for extraterrestrial life biosignatures. The secondary objective of BIOMEX is to investigate the endurance of extremophiles, focusing on their interactions with Lunar and Martian mineral analogues. Ground-based studies are currently being carried out in the framework of EVTs (Experiment Verification Tests) by exposing selected organisms to space and Martian simulations. Results on a desert strain of Chroococcidiopsis obtained from the first set of EVT, e.g. space vacuum, Mars atmosphere, UVC radiation, temperature cycles and extremes, suggested that dried biofilms exhibited an enhanced survival compared to planktonic lifestyle. Moreover the protection provided by a Martian mineral analogue (S-MRS) to the sub-cellular integrities of Chroococcidiopsis against UVC radiation supports the endurance of this cyanobacterium under extraterrestrial conditions and its relevance in the development of life detection strategies.