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71.
72.
李东阳 《华北航天工业学院学报》2014,(1):10-11,15
分析螺纹塑件的结构特点、工艺要求,介绍了基于拼合结构模外卸除螺纹型环的注射模结构以及工作过程,并且对ABS的注射成型工艺进行了分析。 相似文献
73.
月尘累积对太阳电池阵电帘除尘效率影响的实验研究 总被引:4,自引:0,他引:4
月尘在月球探测器太阳电池阵表面的累积将会导致其输出功率下降甚至功能失效。近年来,电帘除尘方法被认为是月尘清除防护的有效手段。文章实验研究了月尘累积对三结砷化镓太阳电池性能影响,拟合得到了月尘累积质量与太阳电池相对输出功率的数学模型;利用电帘除尘装置,研究了不同月尘累积质量下电帘的除尘效率。研究结果表明,6 mg/cm2月尘累积质量是太阳电池阵电帘除尘装置启动的最佳工作条件。该研究成果可为开发具有自适应除尘能力的太阳电池阵提供技术支持。 相似文献
74.
75.
本文介绍了直升机发动机进气防砂装置核心元件-涡旋管的砂尘分离效率计算方法.在柱坐标系中推导出了砂尘在涡旋管中运动的三维动力学方程,并通过数值计算方法,成功地解决了砂尘在涡旋管中运动轨迹的求解问题,得出了涡旋管砂尘分离效率计算方法和计算结果,试验数据表明,该计算方法是可行的. 相似文献
76.
Michael R. Collier William M. Farrell Timothy J. Stubbs 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
An analytic model for the motion of a positively charged lunar dust grain in the presence of a shadowed crater at a negative potential in vacuum is presented. It is shown that the dust grain executes oscillatory trajectories, and an expression is derived for the period of oscillation. Simulations used to verify the analytic expression also show that because the trajectories are unstable, dust grains are either ejected from the crater’s vicinity or deposited into the crater forming “dust ponds.” The model also applies to other airless bodies in the solar system, such as asteroids, and predicts that under certain conditions, particularly near lunar sunset, oscillating dust “canopies” or “swarms” will form over negatively charged craters. 相似文献
77.
S. Takechi T. Onishi S. Minami T. Miyachi M. Fujii N. Hasebe K. Mori K. Nogami H. Ohashi S. Sasaki H. Shibata T. Iwai E. Grün R. Srama N. Okada 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A cosmic dust detector is currently being developed using a piezoelectric lead zirconate titanate (PZT) element. The characteristics of the multilayered detector (MD), which was composed of one hundred PZT disks, were investigated by bombarding it with hypervelocity iron particles supplied by a Van de Graaff accelerator. It was confirmed that there was a linear relationship between the signal amplitude observed from MD and the momentum of the particles. As compared with the single-layered detector (SD) that was composed of one PZT disk, it was found that the sensitivity of MD was ∼3 times higher than that of SD within the limits of the experimental conditions. 相似文献
78.
P. Muralikrishna V.H. Kulkarni 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Dust particles of meteoric origin in the lower E-region can affect the conductivity parameters by varying the effective collision frequency and by causing electron bite outs through the capture of ambient electrons. In magnetized plasma, neutral dust particles can alter the effective collision frequency parameters and thus affect the Pedersen and Hall conductivities in the electrojet region. The Cowling conductivity profile is determined by the height profiles of the Hall and Pedersen conductivities. The collision parameters altered by the neutral dust particles can be considerably different from those estimated from atmospheric models, in the lower E-region heights where dust particles of meteoric origin are known to exist in large numbers. A significant fraction of these dust particles may capture free electrons from the ambient medium and get charged negatively. This can result in reduction in the number density of free electrons especially below the electrojet peak where the dust particles can be present in large numbers, at least on days of large meteor showers. This, in turn, can once again alter the vertical profile of the east–west Hall current driven by the vertical Hall polarization field and under favorable conditions, can even account for the reversal of the electrojet currents below the current peak. Assuming a realistic model for the distribution of neutral dust particles, the conductivity parameters are estimated here. Conditions under which the dust particles can cause partial reversals in the electrojet currents are critically examined here. 相似文献
79.
Johannes Mathies Steffen Mauceri Lukas Pfeiffer Marco Vietze Hans-Peter Roeser Felix BoehringerMichael Lengowski 《Acta Astronautica》2014
SSETO is the result of a phase-A study in context of the small satellite program of the University of Stuttgart that demonstrates the capability of a university institute to build a small satellite with a budget of 5 million Euro. The satellite will be capable of observing exoplanets in a Neptune–Earth scale and obtaining data of interstellar dust. Due to a system failure of NASA?s Kepler mission, there is currently (October 2013) a lack of satellites searching for exoplanets. This paper details the design of subsystems and payload, as well as the required test tasks in accordance with the mission profile at a conceptional level. The costs for standard spacecraft testing and integration tasks are included, but not those of launch, ground support, operations and engineer working hours. 相似文献
80.
Harald Krüger Markus Landgraf Nicolas Altobelli Eberhard Grün 《Space Science Reviews》2007,130(1-4):401-408
The Ulysses spacecraft has been orbiting the Sun on a highly inclined ellipse almost perpendicular to the ecliptic plane (inclination
79°, perihelion distance 1.3 AU, aphelion distance 5.4 AU) since it encountered Jupiter in 1992. The in situ dust detector
on board continuously measured interstellar dust grains with masses up to 10−13 kg, penetrating deep into the solar system. The flow direction is close to the mean apex of the Sun’s motion through the
solar system and the grains act as tracers of the physical conditions in the local interstellar cloud (LIC). While Ulysses
monitored the interstellar dust stream at high ecliptic latitudes between 3 and 5 AU, interstellar impactors were also measured
with the in situ dust detectors on board Cassini, Galileo and Helios, covering a heliocentric distance range between 0.3 and
3 AU in the ecliptic plane. The interstellar dust stream in the inner solar system is altered by the solar radiation pressure
force, gravitational focussing and interaction of charged grains with the time varying interplanetary magnetic field. We review
the results from in situ interstellar dust measurements in the solar system and present Ulysses’ latest interstellar dust
data. These data indicate a 30° shift in the impact direction of interstellar grains w.r.t. the interstellar helium flow direction,
the reason of which is presently unknown. 相似文献