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排序方式: 共有647条查询结果,搜索用时 468 毫秒
51.
A.R. Engel K. Beurle A. Bewick P.K.S. Harper J.J. Quenby N.J.C. Spooner A.G. Fenton K.B. Fenton A.B. Giles J.G. Greenhill D.M. Warren I.M. Martin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
Hard X-ray balloon altitude measurements with a 1600 cm2 phoswich array are described. Data from observations on Sco X-1, GX1+4, GX5−1, Nova Oph. 1977, SMC X-1, SS433, IC 4329A and MR 2251-178 are presented. The role of Comptonisation in X-ray production for Sco X-1 and GX1+4 is discussed. 相似文献
52.
Sachindra Naik U. Mukherjee B. Paul C.S. Choi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2. 相似文献
53.
Wing-Huen Ip 《空间科学学报》2011,31(2):150-153
The magnetic field disturbances detected by the Phobos-2 spacecraft in 1989 have been suggested to be caused by a ring of dust and/or gas emitted from the Martian moon, Phobos. The physical nature of these ``Phobos events' is examined using results from related investigations over the last twenty years. It is concluded that there is no clear evidence at present to support the association of magnetic field disturbances in the solar wind with Phobos. The situation will be further clarified taking advantage of the multi-spacecraft observations of the Yinghuo-1(YH-1), Mars Express and MAVEN missions beginning in 2012. It is expected that many novel features of solar wind interaction with Phobos (and possibly also Deimos) itself will also be revealed. 相似文献
54.
Shuanggen Jin Sundaram Arivazhagan Hiroshi Araki 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The moon has longstanding questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure and possible life. The recent lunar missions, e.g., SELenological and ENgineering Explorer “KAGUYA” (SELENE), Chang’E-1, Chandrayaan-1, and Lunar Reconnaissance Orbiter/Lunar CRater Observation and Sensing Satellite (LRO/LCROSS), have provided new opportunities to explore and understand these issues. In this paper, we reviewed and presented the results and findings in the fields of lunar gravity, magnetic field, atmosphere, surface geomorphology and compositional variations, volcano, craters, internal structure, water and life science from new lunar exploration missions. In addition, the new objectives and scientific questions on lunar explorations in near future are presented and discussed. 相似文献
55.
中俄联合火星电离层星-星掩星探测 总被引:1,自引:0,他引:1
孙越强 杜起飞 朱光武 吴季 陶鹏 白伟华 赵华 胡雄 吴小成 郑建华 A S Kosov T K Breus V M Gotlib A M Krymskii A V Zakharov 《空间科学学报》2009,(5)
中俄联合火星星-星掩星探测是人类首次在火星空间环境进行此类的联合试验。用于探测火星电离层的星-星掩星技术较以前星地间的探测技术相比,有可接收高信噪比信号,反演精度高,可探测火星上太阳天顶角大于43°,或者小于138°的区域电离层等优点。本文介绍了中俄联合火星星-星掩星探测方案、基本原理,给出了主要技术指标、地面模拟测试结果。 相似文献
56.
根据LR(0)自动机的构造理论及Deremer和Pennello的LALR(1)向前看符号集计算公式,提出求解公式中的lookback关系和includes关系的高效算法. 研究过程表明,LR(0)项目集闭包计算和项目集的查找是LR(0)分析器构造过程中的主要性能瓶颈.对这两个计算过程给出了高效的数据结构和算法设计,实现了LALR(1)分析器的快速生成.系统实现及实验数据表明,LALR(1)分析器的生成速度超过了自由软件基金会的LALR(1)分析器生成器Bison. 相似文献
57.
N2O单组元微推力器性能分析及试验 总被引:4,自引:0,他引:4
N2O单组元微推进是当前微推进领域的一个热点问题.在N2O催化分解热力计算的基础上开展了对N2O单组元微推力器比冲性能影响因素的分析,分析结果表明微推力器比冲与N2O分解效率及喷管扩张比有密切关系.所开展的亚牛级N2O单元微推力器催化分解试验结果表明所设计N2O单元推力器能在250℃初温条件下启动,初步验证了N2O单元微推力器的可行性;也揭示了推力室结构及床载大小对亚牛级N2O单元微推力器性能的影响,为进一步的结构及试验设计提供了参考. 相似文献
58.
SUN Huixian WU Ji DAI Shuwu ZHAO Baochang SHU Rong CHANG Jin WANG Huanyu ZHANG Xiaohui REN Qiongying CHEN Xiaomin OUYANG Ziyuan ZOU Yongliao 《空间科学学报》2008,28(5)
Chang'E-1,the orbiter circling the moon 200km above the moon surface,is the first Chinese Lunar exploration satellite.The satellite was successfully launched on 24th October 2007.There are 8 kinds of scientific payloads onboard,including the stereo camera,the laser altimeter,the Sagnac-based interferometer image spectrometer,the Gamma ray spectrometer,the X-ray spectrom-eter,the microwave radiometer,the high energy particle detector,the solar wind plasma detector and a supporting payload data management system.Chang'E-1 opened her eyes to look at the moon and took the first batch of lunar pictures after her stereo camera was switched on in 20th November 2007.Henceforth all the instruments are successfully switched on one by one.After a period of parameter adjustment and initial check out,all scientific instruments are now in their normal operating phase.In this paper,the payloads and the initial observation results are introduced. 相似文献
59.
基于L2范数度量的k平面聚类(k-Plane Clustering,k PC)设计思想,本文提出了一种采用L1范数度量的聚类算法。由于在平面更新步骤中,所导出的优化问题是非凸的,文中给出了一种求解方法,即将非凸问题转化为有限个子集上的凸问题,为避免求解多个优化问题导致训练时间过长问题,本文还设计了一种新的优选策略,有限个子集的搜索任务可在线性时间内完成。本文所提出的方法只需要求解k个线性规划,而不再是k PC的求解特征值问题。在人工和UCI数据集上的实验结果表明:基于L1范数平面聚类算法的训练和测试时间更短,且在大多数数据集上均表现出了更好的聚类性能。 相似文献
60.
针对卫星导航所需的高精度地球定向参数(EOP)中的UT1-UTC预报问题,提出了基于双差分LS+AR的UT1-UTC参数预报方法。对UT1-UTC观测数据进行跳秒检测、固体地球带谐潮汐项改正,然后对改正后的UT1-UTC数据进行双差分处理,增强数据平稳性;采用最小二乘拟合(LS)与自回归(AR)分析方法对差分处理后的数据进行分析与预报;对预报结果进行逆差分处理与潮汐项改正外推、跳秒恢复,获取高精度的UT1-UTC预报值。通过与国际EOP_PCC预报结果对比表明,UT1-UTC短期预报精度与EOP_PCC较优的预报精度相当,其中1天UT1-UTC预报精度优于0.03ms,优于EOP_PCC预报结果。介绍了北京航天飞行控制中心的UT1-UTC每日例行预报情况。 相似文献