Magnetic field of a neutron star with a superconducting quark core in the CFL-phase

The Ginzburg-Landau equations are derived for the magnetic and gluomagnetic gauge fields in the color superconducting core of a neutron star containing a CFL-condensate of diquarks. The interaction of the diquark CFL-condensate with the magnetic and gluomagnetic gauge fields is taken into account. The behavior of the magnetic field in a neutron star is studied by solving the Ginzburg-Landau equations taking correct account of the boundary conditions, including the gluon confinement conditions. The magnetic field distribution in the quark and hadronic phases of a neutron star is found. It is shown that a magnetic field generated in the hadronic phase by the entrainment effect penetrates into the quark core in the form of quark vortex filaments because of the presence of screening Meissner currents. __________ Translated from Astrofizika, Vol. 50, No. 1, pp. 87–98 (February 2007).     

依巴谷星(104297)相对于伽里略卫星Callisto的CCD位置测量

１９９７年１１月１４日晚，在中国科学院云南天文台１米望远镜上用新安装的１０２４２ＣＣＤ观测到了木星的两颗伽里略卫星；Ｅｕｒｏｐａ和Ｃａｌｌｉｓｔｏ及一颗依巴谷星（星号为 １０４２９７）．当采用新的 ＪＰＬ ＤＥ４０５和 Ｓａｍｐｓｏｎ－Ｌｉｅｓｋｅ理论（Ｇ５）计算卫星的理论位置并相对于Ｃａｌｌｉｓｔｏ测量恒星位置时，视位置的观测值与计算值之差的平均值在赤经和赤纬方向分别为△α＝－０″０２９±０．″０１２，△δ＝０．″００５± ０．″０１１．这对应于平均观测历元（ＵＴ）：１９９７年１１月１４日１３时４３分５０秒．这一试验结果与 Ｃａｓａｓ等在同一时期内ＣＣＤ观测的结果有着很好的一致性 它反映了依巴谷星表体现的光学参考系与ＤＥ４０５体现的动力学参考系在观测历元具有较好的一致性．单次位置测定的标准误差在赤经赤纬方向分别为±０．″０５２和０．″０４７．这一精度明显优于 Ｃａｓａｓ等人发表的 Ｃａｌｌｉｓｔｏ的处理精度，并与目前国际上最好的伽里略卫星观测精度相当     

A numerical study of the r-mode instability of rapidly rotating nascent neutron stars

The first results of numerical analysis of classical r-modes of rapidly rotating compressible stellar models are reported. The full set of linear perturbation equations of rotating stars in Newtonian gravity is solved numerically without the slow rotation approximation. A critical curve of gravitational wave emission induced instability, which restricts the rotational frequencies of hot young neutron stars, is obtained. Taking the standard cooling mechanisms of neutron stars into account, we also show the 'evolutionary curves' along which neutron stars are supposed to evolve as cooling and spinning down proceed. Rotational frequencies of 1.4-M_⊙ stars suffering from this instability decrease to around 100 Hz when the standard cooling mechanism of neutron stars is employed. This result confirms the results of other authors, who adopted the slow rotation approximation.     

论地理知识图谱

网络文本蕴含大量隐式地理空间信息,为地理知识获取与知识服务提供了巨大潜能。地理知识图谱是将传统地理信息服务拓展到地理知识服务的关键,也是网络文本蕴含地理信息采集与处理的终极目标。本文系统评述了开放地理语义网、开放地理实体及关系抽取、地理语义网对齐、知识图谱存储方法等地理知识图谱相关主题的研究进展,从网络文本蕴含地理空间信息量与质量评价、地理信息语义理解、空间语义计算模型和异构地理语义网对齐等方面剖析了目前亟需解决的关键科学问题。     

地面加热对沙尘暴数值模拟结果的影响研究

利用沙尘数值预报模式并针对2002年3月18—20日典型沙尘暴过程,模拟研究了地面热通量对沙尘暴的影响及其机制。结果发现,沙尘天气数值预报模式较准确地模拟了本次沙尘暴过程。模式对白天地面加热强度和夜间地面冷却强度均有一定程度的高估。地面热通量能够使沙尘暴明显增强,同时也通过导致地面风速、层结稳定度、地面摩擦速度产生明显的日变化,进而导致沙尘暴强度的日变化。地面热通量影响地面风速的方式是导致混合层形成,从而有利于产生高空动量下传。另外,沙尘暴发生时地面热通量主要影响地面和行星边界层中的天气要素,随时间推移地面热通量能够持续影响上升运动强度,且这一影响从边界层逐渐向上扩展到自由大气,并达到500 hPa以上。     

亚热带4种行道树树干表面CO_2释放速率昼夜动态

采用LI-8100土壤碳通量自动测量系统,与自制的树干呼吸观测气室相连,原位观测亚热带春、秋2个季节4种行道树树干呼吸速率及相关环境因子的昼夜动态.结果表明:在秋季土壤水分较低水平下(VWC平均为11.6%),羊蹄甲、香樟树干呼吸速率昼夜动态呈单峰曲线,和温度变化呈极显著指数函数关系,峰值分别出现在17:00和13:00;芒果和高山榕树干呼吸速率昼夜动态单峰不明显,白天与树干温度变化呈极显著指数函数关系,但芒果白天与夜间的树干呼吸速率差异不显著,而高山榕树干呼吸速率夜间显著高于白天,二者出现"白昼抑制"现象.在春季土壤水分较高水平下(VWC平均为22.1%),羊蹄甲、芒果和高山榕树干呼吸速率昼夜动态呈单峰型曲线,峰值分别出现在11:00、15:00和14:00;而香樟树干呼吸速率单峰不明显,4种树种的树干呼吸速率昼夜动态均与温度变化呈极显著指数函数关系.2个季节中,树干温度与树干呼吸的指数函数关系最好,秋季羊蹄甲、芒果和香樟树干呼吸速率对树干昼夜温度变化的Q10值分别为2.04、2.37和2.18,春季羊蹄甲、芒果、香樟和高山榕树干呼吸速率对树干昼夜温度变化的Q10值分别为2.27、2.58、1.90和1.8...     

X-ray spectral evolution of low-mass X-ray binary GX 349+2

We present the results of a systematic investigation of spectral evolution in the Z source GX 349+2, using data obtained during 1998 with the Proportional Counter Array (PCA) on-board the RXTE satellite. The source traced a extended normal branch (NB) and flaring branch (FB) in the colour–colour diagram (CD) and the hardness-intensity diagram (HID) during these observations. The spectra at different positions of the Z-track were best fitted by a model consisting of a disc blackbody and a Comptonized spectrum. A broad (Gaussian) iron line at ∼6.7 keV is also required to improve the fit. The spectral parameters showed a systematic and significant variation with the position along the Z-track. The evolution in spectral parameters is discussed in view of the increasing mass accretion rate scenario, proposed to explain the motion of Z sources in the CD and the HID.     

THERMAL EFFECTS OF BUILDING′S EXTERNAL SURFACES IN CITY——Characteristics of Heat Flux into and out of External Wall Surfaces

1INTRODUCTIONWiththerecentmodernizationandurbanizationofChi-na,urbanareashavegreatlyincreased, andgiantbuild-ings,especiallythosetallerthan100m,havebeendomi-nantincities,whichhave resultedinthegreatincreaseintheproportionofbuilding'sexternalsurfacetototalurbanarea.Thedifferencesofthermalpropertiesmain-lyinducedbysolarradiationbetweenbuilding'sexter-nalsurfacesareobviousfordifferentexposures,whichcaninevitablyinfluencethedistributionsofairtempera-turenearby,eventheverticaldistributionsofurb…