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排序方式: 共有729条查询结果,搜索用时 468 毫秒
1.
Arman Seuylemezian Manuela Buonanno Lisa Guan David J. Brenner David Welch 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):496-503
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.
本文建立了包括非线性环节在内的横航向驾驶员—操纵系统—飞机本体组合系统的数学模型,采用闭环控制原理,对JJ-7飞机横航向驾驶员诱发振荡PIO问题进行了研究,并详细地讨论了驾驶员参数及其各种操纵动作、操纵系统和飞机本体气动参数对横航向PIO的影响,探讨了横航向PIO产生的机理。文中以JJ-7飞机为例,采用时域法在整个飞行包线各点进行了检查,并用固基飞行模拟器进行模拟验证。其结果与理论计算结果相一致。 相似文献
3.
Joris A. D. L. Blommaert Jan Cami Ryszard Szczerba Michael J. Barlow 《Space Science Reviews》2005,119(1-4):215-243
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
4.
Emergence of a Habitable Planet 总被引:2,自引:0,他引:2
Kevin Zahnle Nick Arndt Charles Cockell Alex Halliday Euan Nisbet Franck Selsis Norman H. Sleep 《Space Science Reviews》2007,129(1-3):35-78
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
5.
研究了面向星敏感器的星模式识别算法。首先扼要介绍了到目前为止出现的所有面向星敏感器的星模式识别算法和星图预处理,然后详细论述了本文提出的基于旋转和比例不变点特征松弛匹配算法的一种新的面向星敏感器的星模式识别算法。在第三部分通过仿真试验检验了新算法的性能。初步的仿真试验结果表明该星模式识别算法性能优良,具有实用价值。最后讨论了待深入研究的问题。 相似文献
6.
二维有限元多尺度小波 总被引:1,自引:0,他引:1
本文利用有限元插值和多尺度分析理论构造出了二维有限元尺度函数及相应的有限元多尺度小波。构造出的尺度函数及小波函数具有许多良好的性质,如短支集、高阶消失矩、半正交性、正则性和对称性等。 相似文献
7.
硝化剂五氧化二氮的合成与放大 总被引:3,自引:0,他引:3
对五氧化二氮(N2O5)的特性、合成及放大方法进行了概括和分析。同时,结合我国硝化工业的现状,介绍了较为可行的工业化合成路线,以及国外的一些N205生产动态和装置。 相似文献
8.
许多严重的飞行事故都与由速率限制引起的Ⅱ型PIO有关。针对如何预防PIO,首先介绍了自适应杆增益和软件限制环节的设计原理。然后以某带速率限制的电传飞机为例,运用同一理论,分析采用自适应杆增益和软件限制环节来改善速率限制的不利影响。仿真结果表明,自适应杆增益环节和软件限制环节都能抑制住PIO的发生,但两者组合加入抑制效果更好,飞行品质也能达到满意的程度。 相似文献
9.
10.
移相全桥变换器是中大功率直流/直流变换场合的一种理想拓扑,但在其输出整流桥上会产生寄生振荡,二极管上存在很高的尖峰电压。这将带来电路损耗并影响整流桥的使用寿命,因此应该想办法抑制。文中分析了寄生振荡产生的原因,介绍了几种可行的抑制方法,并进行了比较研究和实验验证。 相似文献