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51.
We have obtained the first UV high resolution spectra of hot luminous stars in M31 with the FOS onHubble Space Telescope. The spectra, combined with optical spectroscopic and photometric observations, enable us to study their stellar winds and photospheric parameters. We derive mass-loss rates and velocity laws from the wind line profiles, with the SEI method, as well as information on abundances. The wind lines and photospheric spectra are compared with galactic stars of the same spectral type.The spectra analyzed so far indicate that the stars have mass-loss rates comparable or slightly lower than galactic stars of the same spectral type, but possibly different velocity laws in their winds. The spectra of two stars are discussed here. 相似文献
52.
Chung-Ming Ko Min-Hsu Chu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2115-2118
A two-fluid model is used to study the time evolution of stellar winds including the dynamical effect of cosmic rays. Neglecting the diffusion of cosmic rays, we seek self-similar solutions to spherically symmetric winds with a termination shock. The velocity upstream of the shock is taken to be zero. Physical solutions are those that can connect the shock to the star with the velocity approaching zero at the star. Two parameters govern the behaviour of the solutions, namely, the ratio of the upstream sound speed to the shock speed (in an inertial frame) and the gravitation potential of the central star. In some parameter regimes, no physical solution is possible. 相似文献
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54.
对纳米炭黑(UC)、特导纳米炭黑(L6)、碳纳米管(CNT)三种材料在8~18 GHz波段吸波涂层进行了优化设计及吸波性能分析.结果表明,三种材料的复介电常数随着纳米碳材料质量分数的增加,其实部和虚部均以不同的速度增大.利用理论计算的Cole-Cole图,结合实验测得的复介电常数,求解出这三种材料理想的介电常数,材料的质量分数和吸波涂层的匹配厚度.结果表明,CNT的吸波效果最好,当CNT质量分数为20%涂层、厚度为1.6mm时,反射衰减率在11.2~ 15 GHz均优于-10 dB吸收峰最大值,达到29.6 dB. 相似文献
55.
A. Galli P. Wurz S. Barabash A. Grigoriev H. Gunell R. Lundin M. Holmström A. Fedorov 《Space Science Reviews》2006,126(1-4):267-297
We present measurements of energetic hydrogen and oxygen atoms (ENAs) on the nightside of Mars detected by the neutral particle
detector (NPD) of ASPERA-3 on Mars Express. We focus on the observations for which the field-of-view of NPD was directed at
the nightside of Mars or at the region around the limb, thus monitoring the flow of ENAs towards the nightside of the planet.
We derive energy spectra and total fluxes, and have compiled maps of hydrogen ENA outflow. The hydrogen ENA intensities reach
105 cm−2 sr−1 s−1, but no oxygen ENA signals above the detection threshold of 104 cm−2 sr−1 s−1 are observed. These intensities are considerably lower than most theoretical predictions. We explain the discrepancy as due
to an overestimation of the charge-exchange processes in the models for which too high an exospheric density was assumed.
Recent UV limb emission measurements (Galli et al., this issue) point to a hydrogen exobase density of 1010 m−3 and a very hot hydrogen component, whereas the models were based on a hydrogen exobase density of 1012 m−3 and a temperature of 200 K predicted by Krasnopolsky and Gladstone (1996). Finally, we estimate the global atmospheric loss
rate of hydrogen and oxygen due to the production of ENAs. 相似文献
56.
在铁路无线列调通信中存在弱场区和盲区,通信质量难以控制。设计了完整的方案,提高了原无线列调中存在的弱场区的场强,并增大场强覆盖率,使通话距离得到扩展,改善了话音质量。 相似文献
57.
为了探究航空发动机的风扇噪声,通过试验研究了缩尺风扇前传噪声在不同转速工况下的频谱特性和周向模态特性,并对所设计的环形声衬降噪效果进行了验证。研究结果表明,基于试验测量数据分析得到的频谱特性和周向模态特性满足转静干涉噪声理论。随着转速的提高,风扇纯音噪声越显著,高转速工况下纯音噪声的能量约占风扇前传噪声的85%。在所研究的工况范围内,该声衬对目标频率及模态均有显著的降噪效果,且在85%转速工况时的纯音降噪效果最优,其主模态的传声损失约为59dB。该声衬对于设计频率附近的宽频噪声也有一定降噪效果,在85%转速时的宽频噪声平均传递损失约为3dB。 相似文献
58.
59.
Honglei Ma Feng Zhang Yu Zhu Yanhua Xiao Abrar Wazir 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The purpose of the present study was to analyze and predict the changes in acceleration tolerance of human vertebra as a result of bone loss caused by long-term space flight. A human L3–L4 vertebra FEM model was constructed, in which the cancellous bone was separated, and surrounding ligaments were also taken into account. The simulation results demonstrated that bone loss has more of an effect on the acceleration tolerance in x-direction. The results serve to aid in the creation of new acceleration tolerance standards, ensuring astronauts return home safely after long-term space flight. This study shows that more attention should be focused on the bone degradation of crew members and to create new protective designs for space capsules in the future. 相似文献
60.
航天员在长期失重环境影响下,会容易造成椎体失重性骨质疏松。为了探究骨质流失对腰椎承载能力的影响,设计了不同骨密度的腰椎力学仿真,通过图像处理建立了腰椎三维模型,利用有限元算法得到腰椎应力分布,对比了不同材料属性腰椎模型应力结果。结果表明:骨质疏松腰椎的应力值较正常腰椎变小,而形变量却明显增大。可以看出,骨质流失时,会导致腰椎骨骼材料性能发生变化,使腰椎形变量增大,并且使腰椎结构承载能力降低。 相似文献