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111.
1.构造及其原始数据 滑轨舱门收放机构由中、侧滑轨、三角支架、外伸臂、链条条、链轮、液压马达及减速装置等组成(图1)。一根中滑轨布置在43框前飞机对称平面内与飞机外形的下零纵线相贴合,两根侧滑轨分别布置在43框后机身的两侧,舱门的前端由一个接头铰支在三角支架上,三角支架的前支点与链条相连,舱门的后部和两个外伸臂固接, 相似文献
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通过对7A04-T6包铝合金及去包铝合金与三种橡胶抗老化涂层材料在高温、高湿环境中的接触腐蚀产物SEM形貌分析及EDS成分分析,表明铝合金与橡胶抗老化涂层接触腐蚀形貌特征为点蚀,腐蚀严重时试样表面局部或全部被大量腐蚀产物所覆盖,腐蚀产物的主要元素为Al,C,O,Mg,Zn,Cl,Si,S.提出了铝合金与橡胶抗老化涂层"接触-扩散-吸附/沉积物层与电解质薄液膜层形成/腐蚀闭塞区形成/阴离子加速自催化腐蚀/点蚀-晶间腐蚀-剥落腐蚀"的接触腐蚀过程及机理. 相似文献
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Yuri N. Kulikov Helmut Lammer Herbert I. M. Lichtenegger Thomas Penz Doris Breuer Tilman Spohn Rickard Lundin Helfried K. Biernat 《Space Science Reviews》2007,129(1-3):207-243
Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation,
heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary
atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect
of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun
arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal
balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic
chemical reactions and cooling by IR-radiating molecules like CO2, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures
obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen
and high Jeans’ escape rates for heavier species like H2, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO2, N2 and H2O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various
non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian
magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease
the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost
its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the
young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations
for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount
of ∼250 bar of O+ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial
ocean (TO (1 TO ∼1.39×1024 g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and
compare our findings with the results of preceding studies. 相似文献
118.
H. J. Völk 《Space Science Reviews》2007,130(1-4):431-438
The dynamical and chemical effects of the Galactic Wind are discussed. This wind is primarily driven by the pressure gradient
of the Cosmic Rays. Assuming the latter to be accelerated in the Supernova Remnants of the disk which at the same time produce
the Hot Interstellar Medium, it is argued that the gas removed by the wind is enriched in the nucleosynthesis products of
Supernova explosions. Therefore the moderate mass loss through this wind should still be able to remove a substantial amount
of metals, opening the way for stars to produce more metals than observed in the disk, by e.g. assuming a Salpeter-type stellar
initial mass function beyond a few Solar masses. The wind also allows a global, physically appealing interpretation of Cosmic
Ray propagation and escape from the Galaxy. In addition the spiral structure of the disk induces periodic pressure waves in
the expanding wind that become a sawtooth shock wave train at large distances which can re-accelerate “knee” particles coming
from the disk sources. This new Galactic Cosmic Ray component can reach energies of a few×1018 eV and may contribute to the juncture between the particles of Galactic and extragalactic origin in the observed overall
Cosmic Ray spectrum. 相似文献
119.
针对微小精密机电系统中装配连接性能不一致、可靠性差等问题,以某微型挠性摆式加速度计的恒力锁紧机构为例,从装配结构优化、装配工艺精细化设计、装配连接可靠性等3个方面回顾了国内外研究现状,并论述了从这3个方面入手解决恒力锁紧机构载荷精准形成与保持的可行性。结合锁紧机构中被连接组件具有不同材料属性的“三明治”式结构,以及该机构具有多材料、异型异构、跨尺度变形的复杂几何与装配特性,提出了“由内向外”锁紧载荷设计和“由外向内”锁紧载荷保障的解决思路,旨在实现某微型挠性摆式加速度计装配连接性能的高可靠性与高保持性,并以此提升该型加速度计的零偏稳定性。 相似文献
120.
钛合金和铝合金均具有质轻、比强度高和抗腐蚀性能好等优点,已广泛应用于航空航天、军事工业和公共交通等领域,钛/铝异种金属复合结构的连接逐渐成为研究热点。然而,由于物理和化学性能差异明显,钛/铝焊接难度大,存在成形困难、接头性能较差等问题。搅拌摩擦焊作为一种固相焊接方法,对克服异种材料性能差异带来的焊接困难具有极大的优势。本文综述了钛/铝异质金属搅拌摩擦焊的研究现状,主要涉及焊缝成形、焊接参数、力学特征、冶金结合和连接机制等,以及衍生的搅拌摩擦焊新技术,为钛/铝异质金属结构的轻量化设计提供新思路,并对其未来发展进行了展望。 相似文献