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1.
This work aims to investigate far-UVC light at 222 nm as a new microbial reduction tool for planetary protection purposes which could potentially be integrated into the spacecraft assembly process. The major advantage of far-UVC (222 nm) compared to traditional germicidal UVC (254 nm) is the potential for application throughout the spacecraft assembly process in the presence of humans without adverse health effects due to the limited penetration of far-UVC light into biological materials. Testing the efficacy of 222-nm light at inactivating hardy bacterial cells and spores isolated from spacecraft and associated surfaces is a necessary step to evaluate this technology. We assessed survival of Bacillus pumilus SAFR-032 and Acinetobacter radioresistens 50v1 exposed to 222-nm light on proxy spacecraft surfaces simulated by drying the bacteria on aluminum coupons. The survival fraction of both bacteria followed a single stage decay function up to 60 mJ/cm2, revealing similar susceptibility of both species to 222-nm light, which was independent of the exposure rate. Irradiation with far-UVC light at 222 nm is an effective method to decontaminate the proxy spacecraft materials tested in this study.  相似文献   
2.
A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH+. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.  相似文献   
3.
Emergence of a Habitable Planet   总被引:2,自引:0,他引:2  
We address the first several hundred million years of Earth’s history. The Moon-forming impact left Earth enveloped in a hot silicate atmosphere that cooled and condensed over ∼1,000 yrs. As it cooled the Earth degassed its volatiles into the atmosphere. It took another ∼2 Myrs for the magma ocean to freeze at the surface. The cooling rate was determined by atmospheric thermal blanketing. Tidal heating by the new Moon was a major energy source to the magma ocean. After the mantle solidified geothermal heat became climatologically insignificant, which allowed the steam atmosphere to condense, and left behind a ∼100 bar, ∼500 K CO2 atmosphere. Thereafter cooling was governed by how quickly CO2 was removed from the atmosphere. If subduction were efficient this could have taken as little as 10 million years. In this case the faint young Sun suggests that a lifeless Earth should have been cold and its oceans white with ice. But if carbonate subduction were inefficient the CO2 would have mostly stayed in the atmosphere, which would have kept the surface near ∼500 K for many tens of millions of years. Hydrous minerals are harder to subduct than carbonates and there is a good chance that the Hadean mantle was dry. Hadean heat flow was locally high enough to ensure that any ice cover would have been thin (<5 m) in places. Moreover hundreds or thousands of asteroid impacts would have been big enough to melt the ice triggering brief impact summers. We suggest that plate tectonics as it works now was inadequate to handle typical Hadean heat flows of 0.2–0.5 W/m2. In its place we hypothesize a convecting mantle capped by a ∼100 km deep basaltic mush that was relatively permeable to heat flow. Recycling and distillation of hydrous basalts produced granitic rocks very early, which is consistent with preserved >4 Ga detrital zircons. If carbonates in oceanic crust subducted as quickly as they formed, Earth could have been habitable as early as 10–20 Myrs after the Moon-forming impact.  相似文献   
4.
本文综述了用4台发动机为动力的水上飞机自由飞模型起飞与降落性能的综合试验,这些性能包括稳定性、操纵性、飞溅、水阻力、着水撞击、起飞砰击、失速及耐波性等。模型与真实飞机保持几何、质量、运动状态、拉力、升降舵效率及其波浪谱的相似,故模型试验与真实飞机的试飞结果比较符合。同时着重介绍了模型试验的机载测试系统与地面测试系统。  相似文献   
5.
前轮非线性摆振稳定性分析   总被引:1,自引:0,他引:1  
飞机前起落架支柱上的几个非线性项,例如扭转间隙、库仑摩擦以及速度平方阻尼等,对前轮摆振稳定区域有着重要的影响.文中假设前起落架支柱上端固支,并且给出了用以描述五自由度的前轮摆振运动的非线性微分方程组,使用描述函数法研究了上述三个非线性项对前轮摆振稳定区域的影响,将准线性化的方程组代入状态空间内,利用优化特征值实部的方法确定摆振系统的极限环幅值、摆振频率以及临界参数曲线,这种方法可以免去以往摆振稳定性分析时冗长的代数推导.作为比较,文中还计算了前轮线性摆振系统的临界频率以及临界参数曲线,两种结果比较分析表明,支柱内的几个非线性项对前轮摆振稳定区域有着重要的影响,由于扭转间隙的存在,使得飞机临界滑跑速度大大降低.  相似文献   
6.
建立了升降平台跌落时起落架动力学模型,给出了描述缓冲支柱和轮胎力性能的数学公式,使之适用于起落架严重受载的情况;通过数值仿真研究了升降平台跌落时的直升机起落架过载。分析了升降平台跌落时起落架产生大过载的力学机理。升降平台从不同高度自由跌落时,机轮系留引起的起落架正过载相对增加量不超过10%,而系留情况下起落架回弹行程中的负过载比压缩行程中的正过载高得多。  相似文献   
7.
在未来月球探测中,需要对一些地形复杂的区域进行探测,而在这些区域软着陆,潜在的危险性增加,这就要求着陆时具有较高的定位精度并能够自动避险。当前,由于着陆时定点的误差较大,在小范围安全地域准确着陆很难。研究了一种精确定位、安全的软着陆方式,它在软着陆过程中增加了悬停阶段。在这一阶段中,通过着陆区危险地域的识别、着陆地点位置误差的计算,加上对着陆器横向漂移的控制技术,使着陆地点的精度以及着陆生存率大为提高,能够满足未来月球探测的软着陆要求。  相似文献   
8.
通过分析返回舱在着陆时所具有的水平速度也可能对着陆安全构成威胁的事实,论述了为返回舱增加横向缓冲装置的必要性,由此提出亟需解决的问题——在返回舱着陆下降过程中测量其水平运动速度。提出了全新概念的以视觉图像为唯一信息来源的返回舱水平速度测量方法,仅以双目摄像机系统作为传感器,避免了对返回舱原有传感器系统的改造。通过对着陆区域地面图像的采集和在线处理,利用双目交会测量原理得到返回舱当前的大地坐标和姿态。仿真实验证明,方法简单易行,测量结果可靠。  相似文献   
9.
文章描述了回收着陆半实物仿真系统的整个框架,针对整个半实物仿真系统的设计需要和回收程控装置的特点,设计了回收程控装置模拟程序。在程序中所选择的定时方法既满足实时仿真的需要,保证了定时的精度又提高了程序的效率。该程序和半实物仿真系统为回收程控装置设计人员提供了一个快捷的平台来修改程控装置的设计时序。  相似文献   
10.
基于自适应模拟退火遗传算法的月球软着陆轨道优化   总被引:13,自引:4,他引:13  
朱建丰  徐世杰 《航空学报》2007,28(4):806-812
 将自适应遗传算法与模拟退火算法相结合,形成一种自适应模拟退火遗传算法。该算法不但具备了自适应遗传算法的强大全局搜索能力,也拥有模拟退火算法的强大局部搜索能力。针对月球软着陆轨道优化的特点,利用一种新的参数化方法将轨道优化问题转换为非线性规划问题,并应用提出的自适应模拟退火遗传算法进行优化。数值结果表明:该算法的收敛速度快,优化精度高,且避免了初值敏感、病态梯度和局部收敛等问题,能够搜索到全局最优轨道。  相似文献   
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