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421.
422.
星用材料出气加速规律扩散模型 总被引:1,自引:0,他引:1
基于扩散理论分析获得了星用材料在一定温度范围内出气加速过程遵循的规律,给出了加速系数与扩散系数,加速系数与出气过程等当时间及与温度之间的函数关系,并经实验测试证明,理论分析结果克能良好反映材料出气加速过程所遵循的规律。 相似文献
423.
424.
M. Kawaji R.Q. Liang M. Nasr-Esfahany S. Simic-Stefani S. Yoda 《Acta Astronautica》2006,58(12):622-632
The effects of small vibrations on Marangoni convection were investigated experimentally using a liquid bridge of 5 cSt silicone oil with a disk diameter of 7.0 mm, and an aspect ratio close to 0.5. Experiments were performed to determine the critical temperature difference data for no vibration case and with small vibrations applied. The experimental results have shown that the effect of small vibrations on the onset of oscillatory flow is small since the critical temperature difference data for different aspect ratios were not affected by the vibrations. To clarify the surface oscillation phenomena induced by external vibrations, a 3-D numerical simulation model was also developed using a level set algorithm to predict the surface oscillations of isothermal silicone oil bridges. By subjecting the liquid bridge to small vibrations, the surface oscillation characteristics were predicted numerically, and the numerical results compared well with the predictions of an analytical model proposed previously. Furthermore, the effect of small vibrations on the surface vibration amplitude of the liquid bridge is also discussed. 相似文献
425.
空间环境因素引发的星载软件瞬态的控制流错误可能对系统执行效能造成严重影响,为避免容错算法存储开销和执行开销给系统带入过多的计算压力,提出在容错算法开销和所取得的系统的可靠性提升上取得一定折衷,这是星载软件可靠性设计的合理方向。设计了一种适合于弹性添加容错代码的容错方法:扩展块数字签名的控制流检测方法ESCFC(Extend block Signatures for Control Flow Checking)。由空间高能粒子的实验结果和在轨实测结果为系统可靠度建模,提出了算法开销和可靠性效能提升的平衡关系的工程参考和理论依据。定性分析和模拟,充分说明了将该方法运用于航天工程的可行性。 相似文献
426.
The low gravity of a small asteroid would present a challenge for an astronaut attempting to work on its surface. Extravehicular activities (EVAs) of the sophistication of the Apollo Moon missions are not likely to be possible if astronauts attempt to walk freely on the asteroid, hover above its surface, or anchor locally into the regolith. Manipulating large rocks, drilling, and excavating at multiple locations is a high priority science objective, but would be difficult without a hold-down mechanism. If the asteroid has even a small rotation rate, maneuvering precisely over its surface could be cumbersome. A plausible means of conducting complex EVAs is to tie ropes entirely around the asteroid, under which the astronaut is pushed downward onto the asteroid surface by the tension in the rope. The downward force provides an artificial gravity that permits the astronaut to drill, excavate, hammer, and carefully document materials on the surface without the worry of being thrown from the asteroid. An astronaut could also use the ropes as handholds or guides to maneuver freely over the surface. 相似文献
427.
Dirk H.R. Spennemann 《Space Policy》2004,20(4):9-290
The Moon landings of the Apollo programme irrevocably changed the way we see ourselves. Most significantly, this was the first time that humans had set foot on a celestial body other than Earth. The program has left a number of sites on the Moon as well as on Earth. While the management of the sites and artefacts on Earth is fairly straightforward as they are subject to national heritage legislation, it is not so simple with the sites and artefacts on the lunar surface. Moreover, the sites on the Moon differ in one unique aspect from all other heritage sites on Earth: the absence of a lunar atmosphere of any note means that all foot- and track prints of the astronauts are preserved providing a total record of the pioneering phases of human exploration of the Moon. The nascent developments of space tourism, including proposals for lunar heritage tourism, however, threaten the preservation of these traces on the Moon. This paper discusses the terrestrial and in particular the extraterrestrial heritage of the Apollo programme. Set out are the management ethics that need to apply on the lunar surface if this unique heritage is to have a future. 相似文献
428.
Smirnova N. V. Lyakhov A. N. Setzer Yu. I. Osepian A. P. Meng C.-I. Smith R. Stenbaek-Nielsen H. C. 《Cosmic Research》2004,42(3):210-218
Spatial distributions of the electron density in the latitude range 60°–90° N were calculated on the basis of a physical model of the E and lower Fregions of the high-latitude ionosphere using statistical models of auroral proton and electron precipitation. It is shown that precipitating protons can play the key role in the ionization of the Eregion in the dusk and midnight sectors of the auroral oval. However, quantitative estimates of the contribution of protons to the ionization depend on the used statistical models of electron precipitation. Comparison of the electron density profiles calculated for two incoherent scatter radars, EISCAT (Tromsö) and ESR (Svalbard), for simultaneous precipitation of electrons and protons and for electron precipitation only show that the influence of protons is the most significant in the dusk sector over the EISCAT radar and in the midnight sector over the ESR radar. The results presented indicate the need to take protons into account when radar data are used to derive precipitating electron spectra. 相似文献
429.
针对固体火箭发动机药柱存在裂纹的情况,对运动激波在狭缝中绕射传播的非定常流场进行了计算,得到了清晰的流场变化图谱,从流场图中可分辨出激波在狭缝中的传播过程。对不同深宽比的狭缝进行研究,发现流场结构存在明显差别,在深宽比较小时狭缝内压力波振荡较小,当深宽比超过一定值时狭缝内的压力波产生剧烈振荡。研究结果表明,该方法可很好地描述激波在狭缝中的传播过程。 相似文献
430.