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361.
N. Prantzos 《Space Science Reviews》2007,130(1-4):27-42
After a short historical (and highly subjective) introduction to the field, I discuss our current understanding of the origin
and evolution of the light nuclides D, 3He, 4He, 6Li, 7Li, 9Be, 10B and 11B. Despite considerable observational and theoretical progress, important uncertainties still persist for each and every one
of those nuclides. The present-day abundance of D in the local interstellar medium is currently uncertain, making it difficult
to infer the recent chemical evolution of the solar neighborhood. To account for the observed quasi-constancy of 3He abundance from the Big Bang to our days, the stellar production of that nuclide must be negligible; however, the scarce observations of its abundance in planetary nebulae seem to contradict this idea. The observed
Be and B evolution as primaries suggests that the source composition of cosmic rays has remained ∼constant since the early
days of the Galaxy, a suggestion with far reaching implications for the origin of cosmic rays; however, the main idea proposed
to account for that constancy, namely that superbubbles are at the source of cosmic rays, encounters some serious difficulties.
The best explanation for the mismatch between primordial Li and the observed “Spite-plateau” in halo stars appears to be depletion
of Li in stellar envelopes, by some yet poorly understood mechanism. But this explanation impacts on the level of the recently
discovered early “6Li plateau”, which (if confirmed), seriously challenges current ideas of cosmic ray nucleosynthesis. 相似文献
362.
以甲烷为前驱体,碳布缝合织物为预制体,采用等温化学气相渗透(ICVI)工艺,在1 368 K温度和1 s滞留时间下制备了C/C复合材料。采用压汞仪表征不同致密化时间下预制体的孔隙分布,采用偏光显微镜观察热解碳的结构。结果表明:预制体的孔隙分布呈现多峰分布,热解碳的沉积速率与[A/V]值成反比,热解碳的结构与预制体的比表面积相关,沉积初期比表面积较大时,得到的热解碳织构为各相同性和低织构热解碳,随着沉积的进行,比表面积逐渐减小,在纤维束的边沿等部位出现了高织构热解碳。 相似文献
363.
Basic performance of BeiDou-2 navigation satellite system used in LEO satellites precise orbit determination 总被引:1,自引:0,他引:1
The visibility for low earth orbit(LEO) satellites provided by the BeiDou-2 system is analyzed and compared with the global positioning system(GPS). In addition, the spaceborne receivers' observations are simulated by the BeiDou satellites broadcast ephemeris and LEO satellites orbits. The precise orbit determination(POD) results show that the along-track component accuracy is much better over the service area than the non-service area, while the accuracy of the other two directions keeps at the same level over different areas. However, the 3-dimensional(3D) accuracy over the two areas shows almost no difference. Only taking into consideration the observation noise and navigation satellite ephemeris errors, the 3D accuracy of the POD is about30 cm. As for the precise relative orbit determination(PROD), the 3D accuracy is much better over the eastern hemisphere than that of the western hemisphere. The baseline length accuracy is 3.4 mm over the service area, and it is still better than 1 cm over the non-service area. This paper demonstrates that the BeiDou regional constellation could provide global service to LEO satellites for the POD and the PROD. Finally, the benefit of geostationary earth orbit(GEO) satellites is illustrated for POD. 相似文献
364.
First results of PRECISE—Development of a MEMS-based monopropellant micro chemical propulsion system
PRECISE focuses on the research and development of a MEMS-based monopropellant micro chemical propulsion system for highly accurate attitude control of satellites. The availability of such propulsion systems forms the basis for defining new mission concepts such as formation flying and rendezvous manoeuvres. These concepts require propulsion systems for precise attitude and orbit control manoeuvrability. Application-oriented aspects are addressed by two end-users who are planning a formation flying mission for which the propulsion system is crucial. Basic research is conducted aiming at improving crucial MEMS technologies required for the propulsion system. Research and development also focuses on the efficiency and reliability of critical system components. System analysis tools are enhanced to complement the development stages. Finally, the propulsion system will be tested in a simulated space vacuum environment. These experiments will deliver data for the validation of the numerical models. 相似文献
365.
366.
T. Schildknecht R. MusciT. Flohrer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(7):1039-1045
In the framework of its space debris research activities ESA established an optical survey program to study the space debris environment at high altitudes, in particular in the geostationary ring and in the geostationary transfer orbit region. The Astronomical Institute of the University of Bern (AIUB) performs these surveys on behalf of ESA using ESA’s 1-m telescope in Tenerife. Regular observations were started in 1999 and are continued during about 120–140 nights per year. Results from these surveys revealed a substantial amount of space debris at high altitudes in the size range from 0.1 to 1 m. Several space debris populations with different dynamical properties were identified in the geostationary ring. During the searches for debris in the geostationary transfer orbit region a new population of objects in unexpected orbits, where no potential progenitors exist, was found. The orbital periods of these objects are clustered around one revolution per day; the eccentricities, however, are scattered between 0 and 0.6. By following-up some of these objects using the ESA telescope and AIUB’s 1-m telescope in Zimmerwald, Switzerland, it was possible to study the properties of this new population. One spectacular finding from monitoring the orbits over time spans of days to months is the fact that these objects must have extreme area-to-mass ratios, which are by several orders of magnitudes higher than for ‘normal-type’ debris. This in turn supports the hypothesis that the new population actually is debris generated in or near the geostationary ring and which is in orbits with periodically varying eccentricity and inclination due to perturbations by solar radiation pressure. In order to further study the nature of these debris, multi-color and temporal photometry (light curves) were acquired with the Zimmerwald telescope. The light curves show strong variations over short time intervals, including signals typical for specular reflections. Some objects exhibit distinct periodic variations with periods ranging from 10 to several 100 s. All this is indicative for objects with complicated shapes and some highly reflective surfaces. 相似文献
367.
提出了一种在自旋稳定卫星自旋轴与几何体轴重合或几乎重合时只利用太阳角计算自旋卫星姿态的方法。给出了方法的原理及适用范围。研究表明:定姿精度仅与太敏测量精度有关,减小了传统方法中太敏与地敏两项测量误差产生的误差,方法原理简单、精度高。由实际卫星数据的长期验证可知:方法能在卫星自旋轴与实际几何轴偏差较小时实现快速定姿,定姿结果满足要求。 相似文献
368.
利用本征值和本征矢量的分析方法,对钠层的光化学反应的寿命进行了研究,结果表明,利用该方法计算出的钠原子的化学寿命与传统理论有所不同.从而证明了在中层顶区,钠层的中上部的扰动主要受大气动力学过程的影响,钠层底部主要由光化学控制.这为利用钠层作为示踪剂研究中层顶大气动力学的理论提供了理论依据. 相似文献
369.
370.
采用仪器中子活化方法分析了宁强碳质球粒陨石基质及暗色边化学成份。结果表明,宁强陨石的基质比全岩富集轻稀土和亲硫元素,并大致具有与Allende陨石基质相似的稀土特征。暗色边与陨石基质的差别在于:前者富FeO而贫难熔元素。推测陨石基质与暗色边物质来源于太阳星云不同区域。与形成暗色边有关的突发性事件可能曾多次在太阳星云的不同区域中发生。 相似文献