舱内航天服散热途径分析

为分析常压下航天员穿着舱内航天服时的散热性能，６名健康男性青年按二次复合设计分组共进行２４人次试验，经分析计算了获得了服装各散热途径的散热率随通风气源参数及人体活动水平变化的数学模型。对影响服装散热性能的因素及服装散热特性进行了分析讨论。     

Space Weather applications with CDPP/AMDA

AMDA (Automated Multi-Dataset Analysis), a new data analysis service, recently opened at the French Plasma Physics Data Center (CDPP). AMDA is developed according to the Virtual Observatory paradigm: it is a web-based facility for on-line analyses of space physics. Data may come from its own local database as well as remote ones. This tool allows the user to perform classical manipulations such as data visualization, parameter computation and data extraction. AMDA also offers innovative functionalities such as event searches on the content of the data in either visual or automated ways, generation, use and management of time tables (event lists). The general functionalities of AMDA are presented in the context of Space Weather with example scientific use cases.     

The relationship between plasma effects and cosmic radiation studied with TriTel-LMP measurements during the ESEO mission

The main point of the paper is to use the simultaneous measurements of the energetic particle flux by TriTel and those of electron density by a Langmuir probe to study the question of to what extent solar electromagnetic and corpuscular radiation (galactic cosmic rays, particle precipitation from the radiation belts) are responsible for the ionization of the atmosphere. The electron density measured by the Langmuir probe is the sum of the ionization produced by the solar electromagnetic radiation and that due to the corpuscular radiation. The ionization produced by the solar electromagnetic radiation may be computed. The flux of energetic particles in an energy range may be determined by taking the difference between the threshold energy of the TriTel telescopes and the energy corresponding to the local cut-off rigidity. As the ESEO satellite will have a quasi-polar and circular orbit, the cut-off rigidity will change from low to high latitudes, thus enabling the assignment of different energy bands for the telescopes. Thus, it will be possible to determine which energy bands of particle produce ionization at different latitudes.     

Who’s supporting space activities? An ‘issue public’ for US space policy

Using data from the General Social Survey, this research identifies the issue public of US space policy. Highlighting the need to understand and identify the portion of the public that supports space activities, this study underscores the limited appeal of space for the public as a whole. We find that those who support space activities tend to be younger, male, Republican, and have a higher level of education and socioeconomic status. Because these characteristics make up a relatively small proportion of the American population, those supporting space activities must broaden the appeal of space, making it more accessible and understandable for those with whom the issue does not have much saliency.     

Spatial approaches to moons from resonance relative to invariant manifolds

In this study, the final approach to a moon or other body from resonance is explored and compared to the invariant manifolds of unstable periodic orbits. It is shown that the stable manifolds of planar Lyapunov orbits can act as a guide for the periods or resonances that are required for the final approach in both the planar and spatial problems. Previously developed techniques for the planar problem are expanded for use with resonances and used for comparison with trajectories approaching a moon from these resonances. A similar technique is then used for exploring the relationship of invariant manifolds to approach trajectories in the spatial problem. It is shown that the invariant manifolds of unstable periodic orbits provide insight into the trajectory design, and they can be used as a guide to the more direct approach trajectories.     

现代小卫星与大众化空间时代

通过论述现代小卫星技术30年的发展历程,总结其技术发展水平并举出现阶段的典型应用实例,讨论小卫星未来的发展方向,论述大众化空间与现代小卫星的关系,总结现代小卫星技术服务于大众化空间的各项特征。     

环境减灾-1A、1B卫星光学载荷在轨运行情况分析

环境减灾-1A、1B卫星于2008年9月6日发射升空,至2013年7月20日,2颗卫星的4台宽覆盖多光谱CCD相机、1台超光谱成像仪(HSI)和1台红外相机(IRS)已在轨稳定工作近5年,共获取超过61万景2级地面遥感图像数据。文章对在轨运行的光学载荷遥测参数进行了统计和分析,结果表明:DC/DC电压遥测变化量不超过5%,关键光机部位温度遥测变化量小于2.25℃,转动部件电压和电流遥测变化量小于1%,遥测参数均在设计范围内,显示光学载荷在轨稳定正常工作。最后,综合分析了光学载荷图像数据应用情况,分析表明:光学载荷图像数据具有较强的地物影像分类、提取和分辨能力,与国外同类卫星比较,水体识别符合度达到90%以上,旱情分级符合度大于66%,光谱分辨率达到5nm,积雪范围提取精度达到90%以上,在各类应用领域发挥了较大的效能。     

一种团块位置的提取方法

如何正确提取团块位置以实现自动跟踪对图像理解有重要意义。由于团块在图像中出现频繁且位置不确定，位置提取困难。针对一个二值图像识别系统提出了基于集合变换（即数学形态学和二值有序统计）的团块位置提取方法。即，首先对图像进行二值化，其次对二值化图像进行形态学变换，最后对变换的结果图像进行统计分析，由分析结果得出团块的位置信息。用本方法对地图中九种团块线型作了实验，表明该方法运算简单，并行性高。