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The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest
dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006.
We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe)
and others of which there are always many, like meteors and molecules, black holes and binaries. 相似文献
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A.G. Lyne 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2716-2720
A recent multibeam pulsar survey of the outer Galactic plane at Parkes has discovered the first-known double-pulsar binary, a very compact double neutron star system in which both stars are observable as radio pulsars. In this review, we briefly describe the discovery and the studies which have been enabled by the unique properties of the system. These range from the most precise confirmation yet of the theory of general relativity, with the possibility of even more new tests and the measurement of second-order post-Newtonian effects, to studies of the magnetospheres and emission properties of the two pulsars. The discovery also results in a significant increase in the expected rate of occurrence of the mergers of double neutron star systems, and hence the rate of detection of such events by the new ground-based gravitational wave detectors. 相似文献
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根据小样本和小失效数系统的特点,以及可靠性分布函数和参数估计的不确定性和模糊性,提出了一种可靠性分析方法。采用指数分布族,通过分析最少和最大失效数两种最极端状态,确定中间状态的备选点,运用最小平方差原理进行逐个筛选,并给出了算法流程。分析结果表明,计算值与实际观测值较为吻合。该方法可使系统可靠性的估计精度有较大提高。 相似文献
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本文在最少量测条件下采用视线角速度q趋于零的指标函数和低阶等效辨识模型与快速自适应控制方法实现了战术导弹的平行接近制导律。这种最优制导律可以实现直接命中目标本体,实现一弹多用,可以用于反导弹的控制。能使制导装置简化并使其尺寸和重量减小,算法简单易于工程使用。经过大量数学和半实物仿真试验表明,上述成果可应用于实际工程当中。 相似文献
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P. C. Frisch 《Space Science Reviews》2007,130(1-4):355-365
The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter
distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae
that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun
appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff,
has a bulk velocity of ∼19 km s−1 in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova
remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped
over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal
pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet
flow direction is included. 相似文献
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灰色系统理论中非等时序序列或含有空穴的序列,通常可以用均值生成方法来填补,生成等时序序列。本文研究发现,用非紧邻均值生成方法生成的内点与实际存在有明显的误差,为此讨论了均值生成和有偏生成算法。利用数据序列点的局部凹凸特性来表示数据序列点的特征,提出了采用数据序列点连线的状态选取生成系数的方法。通过对一维数据序列传统均值生成方法的比较,给出了二维数据序列的定义,讨论了在二维数据序列下的均值生成方法,提出了有偏生成算法中生成系数分解的选取方法。 相似文献
10.
Mikhail Sachkov Boris Shustov Ana Ines Gómez de Castro 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
During last three decades, astronomers have enjoyed continuous access to the 100–300 nm ultraviolet (UV) spectral range where the resonance transitions of the most abundant atoms and ions (at temperatures between 3000 and 300 000 K) reside. This UV range is not accessible from ground-based facilities. The successful International Ultraviolet Explorer (IUE) observatory, the Russian ASTRON mission and successor instruments such as the Galaxy Evolution Explorer (GALEX) mission or the COS and STIS spectrographs on-board the Hubble Space Telescope (HST) prove the major impact of observations in the UV wavelength range in modern astronomy. Future access to space-based observatories is expected to be very limited. For the next decade, the post-HST era, the World Space Observatory – Ultraviolet (WSO–UV) will be the only 2-m class UV telescope with capabilities similar to the HST. WSO–UV will be equipped with instruments for imaging and spectroscopy and it will be a facility dedicated, full-time, to UV astronomy. In this article, we briefly outline the current status of the WSO–UV mission and the science management plan. 相似文献