Seasonally steady planetary disturbances in the troposphere and stratosphere as seen in 30 years of NCEP reanalysis data

Zonal velocity and temperature daily global reanalysis data of 30 years are used to search seasonally steady planetary disturbances in the middle troposphere (400 hPa) and middle stratosphere (10 hPa). Significant wavenumber 1, 2 and 3 modes are found. Constant phase lines of zonal velocity 1 modes exhibit significant inclination angles with respect to the meridians. The winter hemisphere generally shows a more significant presence of structures. The Northern Hemisphere (NH) exhibits all over the year a larger amount of structures and more intense amplitudes than the Southern Hemisphere (SH). Middle latitudes exhibit the most significant cases and low latitudes the least significant ones. Longitudinally oriented land–sea transitions at ±$\pm$65° and −35° latitudes appear to play a significant role for the presence of steady planetary modes. The stratosphere exhibits a much simpler picture than the troposphere. Large scale structures with respectively NE–SW (NH) and NW–SE (SH) tilts in the observed temperature and zonal velocity constant phase lines recall the quasi-stationary Rossby wave trains that favor the poleward transport of angular momentum.     

太阳紫外辐射对星上光学膜层的影响

光学遥感是当前卫星遥感的重要手段, 而卫星温控和能源系统也广泛采 用光学膜层, 它们在空间环境条件下的性能对卫星应用任务的完成, 乃至卫星寿命、安全将起着非常重要的作用. 本文给出了太阳紫外辐射对星上光学膜层影响的主要机制, 分析了这一影响的主要规律和原子氧剥蚀、高能粒子和静电场的作用, 综述了太阳紫外辐射对星上光学系统表面膜层影响的测量结果, 最后提出了星上光学膜层污染防护中应重点关注的几个方面.      

Mars Phobos and Deimos Survey (M-PADS) – A martian Moons orbiter and Phobos lander

We describe a Mars ‘Micro Mission’ for detailed study of the martian satellites Phobos and Deimos. The mission involves two ∼330 kg spacecraft equipped with solar electric propulsion to reach Mars orbit. The two spacecraft are stacked for launch: an orbiter for remote investigation of the moons and in situ studies of their environment in Mars orbit, and another carrying a lander for in situ measurements on the surface of Phobos (or alternatively Deimos). Phobos and Deimos remain only partially studied, and Deimos less well than Phobos. Mars has almost always been the primary mission objective, while the more dedicated Phobos project (1988–89) failed to realise its full potential. Many questions remain concerning the moons’ origins, evolution, physical nature and composition. Current missions, such as Mars Express, are extending our knowledge of Phobos in some areas but largely neglect Deimos. The objectives of M-PADS focus on: origins and evolution, interactions with Mars, volatiles and interiors, surface features, and differences. The consequent measurement requirements imply both landed and remote sensing payloads. M-PADS is expected to accommodate a 60 kg orbital payload and a 16 kg lander payload. M-PADS resulted from a BNSC-funded study carried out in 2003 to define candidate Mars Micro Mission concepts for ESA’s Aurora programme.     

Six sigma robust design optimization for thermal protection system of hypersonic vehicles based on successive response surface method

Lightweight design is important for the Thermal Protection System(TPS) of hypersonic vehicles in that it protects the inner structure from severe heating environment. However, due to the existence of uncertainties in material properties and geometry, it is imperative to incorporate uncertainty analysis into the design optimization to obtain reliable results. In this paper, a six sigma robust design optimization based on Successive Response Surface Method(SRSM) is established for the TPS to improve the reliability and robustness with considering the uncertainties. The uncertain parameters related to material properties and thicknesses of insulation layers are considered and characterized by random variables following normal distributions. By employing SRSM, the values of objective function and constraints are approximated by the response surfaces to reduce computational cost. The optimization is an iterative process with response surfaces updating to find the true optimal solution. The optimization of the nose cone of hypersonic vehicle cabin is provided as an example to illustrate the feasibility and effectiveness of the proposed method.     

热防护系统损伤容限分析

建立了含初始矩形损伤的热防护系统(Thermal protection system,TPS)气动热分析的CFD数值模型,分析结果表明损伤区域侧壁出现了很高的热流密度峰值,并且迎风面侧壁峰值高于背风面,而损伤区域底部热流密度却很低。利用分析获得的热流密度建立了含损伤和无损伤TPS的有限元传热分析模型。分析结果表明:损伤的存在导致防热瓦最高温度急剧上升,超过其材料能承受的极限温度(1 500℃),防热瓦首先失效,而损伤对机体最高温度影响较小。最后进行了TPS损伤容限分析,在防热瓦极限温度约束下,外部热流密度最大值从100kW/m2增加到140kW/m2,矩形损伤宽度最大容许值从22.7mm减小到12.6mm,而弧形损伤宽度最大容许值从34.6mm减小到25.1mm,即随着外部热流密度最大值增加,损伤宽度的最大容许值降低,并且相同外部热流密度水平下弧形损伤宽度的最大容许值大于矩形损伤。     

联邦学习安全与隐私保护综述

联邦学习是一种新型的分布式学习框架,它允许在多个参与者之间共享训练数据而不会泄露其数据隐私。但是这种新颖的学习机制仍然可能受到来自各种攻击者的前所未有的安全和隐私威胁。本文主要探讨联邦学习在安全和隐私方面面临的挑战。首先,本文介绍了联邦学习的基本概念和威胁模型,有助于理解其面临的攻击。其次,本文总结了由内部恶意实体发起的3种攻击类型,同时分析了联邦学习体系结构的安全漏洞和隐私漏洞。然后从差分隐私、同态密码系统和安全多方聚合等方面研究了目前最先进的防御方案。最后通过对这些解决方案的总结和比较,进一步讨论了该领域未来的发展方向。     

一种新型燃烧室供油系统热防护方案

随着航空发动机燃烧室进口空气温度的不断升高,燃油在供油管路内受热氧化结焦从而引发诸多隐患的情况日益突出。本文针对某型中心分级、多点喷射供油系统,开展了以空气隔热屏结合“油冷”的热防护方案设计研究,并通过数值 模拟分析了热防护效果。研究表明,在典型高温进气工况下,空气隔热屏结构可将燃油管路湿壁温度降低至燃油氧化结焦临界温度以下;在慢车主油路停止供油的情况下,单一的空气隔热措施难以满足热防护设计要求,结合“油冷”方案可达到设计要求。     

载人火星探测的行星保护

行星保护是影响载人火星探索任务的重要问题之一。载人探测的行星保护包括3个方面,即防止来源于地球的微生物污染目标星球的正向污染防护、防止外来生物对地球的潜在危害的逆向污染防护,以及确保航天员的健康和安全。国际宇航界已经开始针对载人火星探测的行星保护制定政策法规和开展技术研讨。本文介绍了行星保护的定义和法理依据,简要回顾了美国国家航空航天局在“阿波罗登月”中的行星保护措施,并对未来载人火星探测中的主要污染物、污染途径以及污染防护策略进行了初步探讨。     

电脉冲除冰系统参数的合理选择

目前,尽管可采用各种防(除)冰方法,但它们在需用能量及除冰性能上尚有不足之处。电脉冲除冰所需能量少、维护方便(无运动部件)、可靠性高、重量小及经济性好等方面大大优于现有的其他防(除)冰系统。本文介绍了电脉冲除冰系统的基本工作原理,分析了能量,电容和电压等电气参数、线圈的几何参数及蒙皮的材料等对除冰性能的影响。根据分析和实验室、冰风洞及飞行实验的资料,提出了有效除冰时各种參数的选择范围,以及提高性能的措施。     

发动机气瓶热防护产品绝热性能评定研究

通过批抽检热真空试验,能够评定发动机气瓶热防护产品的绝热性能,由于试验设备和试验工艺过程对产品温升会产生巨大影响,依据绝热材料导热系数测试方法,在试验方法不变的条件下,提出新的试验评定要求:稳态过程中产品温升速率。新的产品测试评定要求,能够客观准确的评定产品的隔热性能,排除设备和工艺过程对评定结果的影响。此评定方法也可用于形状不规则、厚度不一致的整件产品绝热性能评定。