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排序方式: 共有463条查询结果,搜索用时 15 毫秒
1.
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
2.
月食过程月表太阳辐照和温度变化模拟 总被引:1,自引:2,他引:1
月食对月球轨道探测器的温度有重要的影响,分析月食时月表的太阳辐照和温度,具有重要意义。文章给出了通用的月表温度模型和月食时月表太阳辐照模型,根据某次月食的天文参数,用太阳辐照模型可求出月表任一点在月食时的太阳直接辐照变化过程,代入温度模型可求出任一点的温度变化过程。此模型和方法可用于对任何一次月食的分析,并以2007年8月28日的月食为例,模拟了该次月食的表面太阳直接辐照和温度的变化过程。 相似文献
3.
本文叙述了高空科学气球上一种自行研制的宇宙尘收集器以及气球吊篮系统。利用该系统进行了五次高空字宙尘粒的收集飞行,简述了对所收集的尘粒进行系统研究的结果。 相似文献
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Necmi Cihan Orger Kazuhiro Toyoda Hirokazu Masui Mengu Cho 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(10):3270-3288
The charged dust particles can be mobilized electrostatically by the repulsion between the adjacent grains and the surface electric field due to the incoming electron current and the charge accumulation within the micro-cavities. In this study, the experimental results of the initial vertical launching velocities and the maximum dust heights are compared with the estimated values for the lofted spherical dust grains by the patch surface charging equations. Silica particles with the sizes between <6 and 45?µm in radius are loaded on a graphite plate, and they are exposed to the electron beam with 450?eV energy under 4?×?10?3?Pa vacuum chamber pressure. During the first set of the experiments, the dust samples are tested without an initial compression process and an additional horizontal electric field. Second, the dust samples are compressed by two different weights in order to increase the packing density under approximately 780.7?Pa and 3780?Pa. Finally, the dust grains are placed between the two parallel aluminum plates to apply approximately 2000?V/m and 4800?V/m horizontal electric field. A high-speed camera is used to record the transportation of the dust grains together with a microscopic telescope, and the results point out that the patch surface dust-charging model estimations are in agreement with the first experiments. On the other hand, the dust particles from the compressed samples are lofted with higher velocities than the estimations, and the number of the dust lofting observations decreases significantly, which demonstrates the importance of the micro-cavities and the increased charging requirement to overcome the contact forces. When the horizontal electric field is present, the initial vertical launching velocities are measured to be lower than the other experiments, which can be attributed to the decreased charging requirement for the dust lofting as a result of inter-particle collisions and rolling motion. According to the experimental results, the electrostatic dust transportation can be controlled not only by the ambient plasma and the solar irradiation on the airless planetary bodies, but also by the surface properties such as the contact surfaces between the dust grains, the number of the micro-cavities related to the packing density, and the presence of the horizontal electric field contributing to the external forces by other particle motions. 相似文献
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月球背面的探测器必须依靠地月中继卫星进行数据传输与通信。地月中继任务包括实时性任务和延迟容忍类任务,如数传任务。当探测器等待传输的数据量超出用户存储容量时,延迟容忍类任务会由于探测器本地存储资源不足和地月中继卫星天线资源受限而无法完成,导致任务数据丢失,所以需要设计一种合理的地月中继任务调度策略,提高地月中继卫星的资源利用率,减少数据的丢失。对地月中继卫星任务调度进行了研究,在分析地月中继卫星数传任务的特点及用户的存储限制的基础上,以最小化数据丢失量为优化目标,建立了地月中继卫星任务调度模型,并设计了一种基于离散烟花算法(DFWA)的地月中继卫星任务调度算法。仿真数据分析表明,基于离散烟花算法的地月中继卫星任务调度算法在求解结果上优于遗传算法,是一种合理、有效的调度方法。 相似文献
9.
崎岖地形中关节式月球车姿态估计数值求解方法 总被引:1,自引:1,他引:1
以被动关节式地形自适应月球车为研究对象,融合关节机器人D-H坐标建模方法构建了月球车悬架运动学模型和以侧倾、俯仰和偏转角表示姿态的欧拉角方式建立了车轮到世界坐标系的悬架完整表达模型。利用悬架完整表达模型,用带有迭代因子的连续迭代和离散迭代数值求解方法,建立了光滑和离散崎岖地形姿态估计算法。最后以8轮扭杆双摇杆摇臂月球车原理样机为例来验证此模型求解方法。仿真结果验证了所建立的基于数值方法的崎岖地形被动关节式月球车姿态估计模型的正确性,其求解模型精度能够满足仿真要求。 相似文献
10.
王海燕%张敏%王海峰%张永生%彭桂荣 《宇航材料工艺》2008,38(5)
进行了改性羰基铁粉-氯磺化聚乙烯(CSM)吸波涂层的臭氧环境暴露试验,并利用SEM、XRD、IR、DSC和TG等方法研究了臭氧对其表面结构和性能的影响。结果表明,臭氧造成CSM表层分解,部分羰基铁粉脱落,但未影响改性羰基铁粉的相组成,对涂层吸波性能的影响不显著。 相似文献