一种改进的网络突发话题检测算法

引进文本相关度这一影响因子,提出了一种基于蚁群聚类算法的突发话题检测算法,该算法结合蚁群聚类算法的优势,综合考虑文本聚类和文本相关度的影响,得到对网络突发话题检测的最优聚类效果,并对近年来网络突发话题进行实验,达到了很好的聚类速度和聚类效果,验证了算法对突发话题检测的准确性和即时性.     

郭守敬的《授时历》和朝鲜的《七政算内篇》

《授时历》被评价为中国历史上最优秀的历法,并且成为明朝《大统历》和朝鲜《七政算内篇》成书的基础。《七政算内篇》是朝鲜世宗时代(1418—1450年)取得的重要天文业绩之一,以《回回历》为基础,与《七政算外篇》一同于1444年编纂成书。《七政算内篇》的历元、天文常数和计算法等基本体系参照《授时历》,应数值则参照了《大统历》的辛巳应数。且把四余添加在推步的项目中,在计算日月食时使用的常数值则参考了元统1384年编纂的《大统历法通轨》,《七政算内篇》汲取了《授时历》和《大统历》的优点。     

Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre

The cores of most galaxies are thought to harbour supermassive black holes, which power galactic nuclei by converting the gravitational energy of accreting matter into radiation. Sagittarius A* (Sgr A*), the compact source of radio, infrared and X-ray emission at the centre of the Milky Way, is the closest example of this phenomenon, with an estimated black hole mass that is 4,000,000 times that of the Sun. A long-standing astronomical goal is to resolve structures in the innermost accretion flow surrounding Sgr A*, where strong gravitational fields will distort the appearance of radiation emitted near the black hole. Radio observations at wavelengths of 3.5 mm and 7 mm have detected intrinsic structure in Sgr A*, but the spatial resolution of observations at these wavelengths is limited by interstellar scattering. Here we report observations at a wavelength of 1.3 mm that set a size of 37(+16)(-10) microarcseconds on the intrinsic diameter of Sgr A*. This is less than the expected apparent size of the event horizon of the presumed black hole, suggesting that the bulk of Sgr A* emission may not be centred on the black hole, but arises in the surrounding accretion flow.     

Macrophage migration inhibitory factor stimulates AMP-activated protein kinase in the ischaemic heart

Understanding cellular response to environmental stress has broad implications for human disease. AMP-activated protein kinase (AMPK) orchestrates the regulation of energy-generating and -consuming pathways, and protects the heart against ischaemic injury and apoptosis. A role for circulating hormones such as adiponectin and leptin in the activation of AMPK has received recent attention. Whether local autocrine and paracrine factors within target organs such as the heart modulate AMPK is unknown. Here we show that macrophage migration inhibitory factor (MIF), an upstream regulator of inflammation, is released in the ischaemic heart, where it stimulates AMPK activation through CD74, promotes glucose uptake and protects the heart during ischaemia-reperfusion injury. Germline deletion of the Mif gene impairs ischaemic AMPK signalling in the mouse heart. Human fibroblasts with a low-activity MIF promoter polymorphism have diminished MIF release and AMPK activation during hypoxia. Thus, MIF modulates the activation of the cardioprotective AMPK pathway during ischaemia, functionally linking inflammation and metabolism in the heart. We anticipate that genetic variation in MIF expression may impact on the response of the human heart to ischaemia by the AMPK pathway, and that diagnostic MIF genotyping might predict risk in patients with coronary artery disease.     

城市污水深度处理技术方案比选

简要介绍了城市污水的性质,对城市污水处理厂处理后的污水再次深度处理达到国家《景观娱乐用水水质标准》（GB12941—91）中规定的水体达标排放指标提出两种工艺技术方案,并对两种方案在系统组成、出水水质稳定性、运行费用3个方面进行了比选。     

头孢唑林钠中杂质噻二唑的分离与分析

采用化学法分离得到头孢唑林钠中的杂质噻二唑,用薄层色谱(TLC)和高效液相色谱(HPLC)对分离得到的噻二唑样品初步定性,用红外吸收光谱(IR)对分离得到的噻二唑样品进行结构确认;根据相对保留时间确定其在头孢唑林钠中的残留;依据欧洲药典的方法,用质量分数为1.0 %的头孢唑林钠溶液做对照,以头孢唑林钠供试品溶液中噻二唑的峰面积与质量分数为1.0 %的对照溶液中头孢唑林钠的峰面积比计算噻二唑的含量.结果表明,分离得到的噻二唑是生产工艺过程的残留,所建立的方法适合头孢唑林钠中残留的噻二唑的定性定量分析.进行实际样品分析,其含量在安全限度范围内(质量分数不超过1.0 %),患者可以放心使用.     

小鼠的生殖特性及阴栓

耳科、妇科、产科、计划生育、生殖医学中心及胚胎干细胞等医学科学研究中,常需要准确确定小鼠妊娠天数或获取适龄胎鼠,故选择适龄雌雄小鼠,鉴定动情期,恰当比例适时合笼,是确保小鼠受孕的关键;而识别阴栓是重中之重,这将直接影响实验进程和实验结果的精确度和可靠性。现就小鼠的生殖特性及阴栓作一简介,供广大科研人员参考。     

动物实验管理流程的建立及效果分析

探讨动物实验中心管理的难点,建立适合动物实验的管理流程,并对其效果进行评价和分析。     

一种流媒体代理缓存系统的研究与实现

在参考已有的流媒体代理缓存理论基础上,采用前缀缓存+补丁算法的缓存管理策略,参照流媒体服务器的工作原理,采用RTSP协议作为流传输协议,设计并实现了一种流媒体代理缓存系统.经实验测试该系统提高了系统的字节命中率,进一步减少对网络带宽资源的需求.     

Isotopic homogeneity of iron in the early solar nebula.

The chemical and isotopic homogeneity of the early solar nebula, and the processes producing fractionation during its evolution, are central issues of cosmochemistry. Studies of the relative abundance variations of three or more isotopes of an element can in principle determine if the initial reservoir of material was a homogeneous mixture or if it contained several distinct sources of precursor material. For example, widespread anomalies observed in the oxygen isotopes of meteorites have been interpreted as resulting from the mixing of a solid phase that was enriched in 16O with a gas phase in which 16O was depleted, or as an isotopic 'memory' of Galactic evolution. In either case, these anomalies are regarded as strong evidence that the early solar nebula was not initially homogeneous. Here we present measurements of the relative abundances of three iron isotopes in meteoritic and terrestrial samples. We show that significant variations of iron isotopes exist in both terrestrial and extraterrestrial materials. But when plotted in a three-isotope diagram, all of the data for these Solar System materials fall on a single mass-fractionation line, showing that homogenization of iron isotopes occurred in the solar nebula before both planetesimal accretion and chondrule formation.