The chromospherically active binary CF Tuc revisited     

D. Do&#;ru  A. Erdem  S. S. Do&#;ru  S. Zola 《Monthly notices of the Royal Astronomical Society》2009,397(3):1647-1660

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Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys     

L. P. L. Colombo  E. Pierpaoli  J. R. Pritchard † 《Monthly notices of the Royal Astronomical Society》2009,398(4):1621-1637

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New faint optical spectrophotometric standards: hot white dwarfs from the Sloan Digital Sky Survey     

Carlos Allende Prieto  Ivan Hubeny  J. Allyn Smith 《Monthly notices of the Royal Astronomical Society》2009,396(2):759-771

The spectral energy distributions for pure-hydrogen (DA) hot white dwarfs can be accurately predicted by model atmospheres. This makes it possible to define spectrophotometric calibrators by scaling the theoretical spectral shapes with broad-band photometric observations – a strategy successfully exploited for the spectrographs onboard the Hubble Space Telescope ( HST ) using three primary DA standards. Absolute fluxes for non-DA secondary standards, introduced to increase the density of calibrators in the sky, need to be referred to the primary standards, but a far better solution would be to employ a network of DA stars scattered throughout the sky. We search for blue objects in the sixth data release of the Sloan Digital Sky Survey (SDSS) and fit DA model fluxes to identify suitable candidates. Reddening needs to be considered in the analysis of many of these stars. We propose a list of nine pure-hydrogen white dwarfs with absolute fluxes with estimated uncertainties below 3 per cent, including four objects with estimated errors <2 per cent, as candidates for spectrophotometric standards in the range  14 < g < 18  , and provide model-based fluxes scaled to match the SDSS broad-band fluxes for each. We apply the same method to the three HST DA standards, linking the zero point of their absolute fluxes to ugr magnitudes transformed from photometry obtained with the US Naval Observatory 1-m telescope. For these stars, we estimate uncertainties of <1 per cent in the optical, finding good consistency with the fluxes adopted for HST calibration.  相似文献   

Simulation Study About the Influence of Atmospheric Stratification on Lightning Activities          下载免费PDF全文

ZHENG Dong  ZHANG Yijun  LU Weitao  MA Ming  MENG Qing 《Acta Meteorologica Sinica》2008,22(1):78-90

A 2D model about charging and discharging processes in thundercloud is used to simulate three differential atmospheric stratifications resulting in discrepant thunderstorm processes in Beijing region. The dynamic and microphysical processes in thunderstorm and their influence on lightning activities are also discussed.The results indicate that ascending velocity and water vapor axe the most important factors to influence lightning activities. At the same time, they affect each other and are together controlled by atmospheric stratification. The magnitude of the ascending velocity determines the intensity of storm and the time when the thunderstorm matured. The thunderstorm with strong updrafts can reach a large height in a short time. Strong persistent updrafts and sufficient water vapor which help to generate more ice phase hydrometeors that directly influence charging and discharging process will prolong the mature stage of the thunderstorm and thereby enhance lightning activities. Though the big density of ice phase hydrometeors can be formed, it is difficult to sustain a long time in the condition of strong updrafts and scant water vapor. Under the condition of weak updrafts and suffcient water vapor in the whole levels, it is easy to form warm cloud process in which the ice phase process and lightning activities are weak. The favorable stratification conditions for strong lightning activities are the sufficient vapor in the lower atmosphere,moderate humidity in the mid troposphere, big instability energy and some suitable convective inhibition.Through calculating some atmospheric instability parameters, it is indicated that convective instability index smaller than -10℃ (negative means instable), convective available potential energy larger than 1000 J kg-1,convective inhibition larger than 40 J kg-1, the 700-hPa potential equivalent temperature larger than 340 K and the 35%-85% humidity in the mid troposphere (700-400 hPa) are the advantageous conditions for strong lightning activities.  相似文献   

2006年5—9月雷暴天气及各种物理量指数的统计分析   总被引：2，自引：0，他引：2  

李勇  孔期 《气象》2009,35(2):64-70

对2006年5-9月全国雷暴天气时空特征进行了统计分析,结果表明:雷暴天气的发生具有明显的短时局地特征,大多数发生在17-20时,上午11时发生最少.全国范围发生过雷暴天气的站点不到总数的三分之一.从空间分布来看,广东、广西及云南三省(区)是雷暴发生最为频繁的省份,内蒙古中西部、新疆北部、青海北部等地则发生较少.此外,统计分析各物理量指数后发现,各种物理量指数对于雷暴等强对流天气发生呈现出不同的概率分布特征,其中最主要的特征是当雷暴等强对流性天气发生时,存在3个高概率区域,每个区域对应物理量指数值相对集中在一个特定范围内.  相似文献   

MODIS BRIGHTNESS TEMPERATURE DATA ASSIMILATION UNDER CLOUDY CONDITIONS: METHODS AND IDEAL TESTS   总被引：1，自引：1，他引：0  

丁伟钰  万齐林  张诚忠  陈子通  黄燕燕 《热带气象学报(英文版)》2010,16(4):313-324

Clouds have important effects on the infrared radiances transmission in that the inclusion of cloud effects in data assimilation can not only improve the quality of the assimilated atmospheric parameters greatly, but also minimize the initial error of cloud parameters by adjusting part of the infrared radiances data. On the basis of the Grapes-3D-var (Global and Regional Assimilation and Prediction Enhanced System), cloud liquid water, cloud ice water and cloud cover are added as the governing variables in the assimilation. Under the conditions of clear sky, partly cloudy cover and totally cloudy cover, the brightness temperature of 16 MODIS channels are assimilated respectively in ideal tests. Results show that when the simulated background brightness temperatures are lower than the observation, the analyzed field will increase the simulated brightness temperature by increasing its temperature and reducing its moisture, cloud liquid water, cloud ice water, and cloud cover. The simulated brightness temperature can be reduced if adjustment is made in the contrary direction. The adjustment of the temperature and specific humidity under the clear sky conditions conforms well to the design of MODIS channels, but it is weakened for levels under cloud layers. The ideal tests demonstrate that by simultaneously adding both cloud parameters and atmospheric parameters as governing variables during the assimilation of infrared radiances, both the cloud parameters and atmospheric parameters can be adjusted using the observed infrared radiances and conventional meteorological elements to make full use of the infrared observations.  相似文献   

矿床工业指标优化及其对矿山可持续发展的意义:以紫金山金矿为例     

万昌林 《地质与勘探》2010,46(2):285-290

矿床工业指标的优化应体现动态性和及时性的原则,建立起能反映各有关参数间动态联系的数学模型,在生产成本、产品价格、生产技术等有较大变化时及时进行优化,从而有效地保护和科学、合理地开发利用矿产资源,实现可持续发展。本文以福建紫金山金矿为例,论述了矿床工业指标优化的原则和可行性,阐述了矿床工业指标优化参数的选择和论证过程,以及增加矿产资源储量,提高资源利用率,延长矿山服务年限,实现矿山可持续发展的意义。  相似文献   

CSAMT视电阻率曲线对水平层状大地的识别与分辨   总被引：3，自引：0，他引：3  

汤井田 《地质与勘探》2010,46(6):1079-1086

在三层和五层介质模型上,通过改变各电性层层参数并进行相应的数值计算,比较并分析了可控源音频大地电磁法卡尼亚视电阻率曲线对各层信息的识别与分辨能力。上部覆盖层厚度的增大和电阻率的减小使视电阻率曲线对下部信息的分辨能力下降,而下部地层层参数变化的影响则相对较小;低阻薄夹层对曲线的影响主要由其纵向电导所决定,纵向电导越大异常值越明显;高阻夹层对曲线的影响则取决于其厚度埋深比,比值越大高阻层越易于分辨,而曲线对高阻层电阻率值变化反应不敏感;在10%的分辨标准下,当低阻夹层纵向电导大于覆盖层的0.2倍、高阻夹层电阻率大于围岩5倍以上并且厚度埋深比大于0.2时,各有可分辨异常。相邻高低阻层差异的增大将使曲线的震荡假异常更加明显,导致分辨能力下降。  相似文献   

储层宏观非均质性研究——以吉林油田大208区黑帝庙油田为例     

胡望水程超  王炜牛世忠  彭国红王东辉  张宇昆周萍 《地质科学》2010,45(2):466-475

储层非均质性是影响油气藏中油、气、水渗流及油气采收率的主要内因。进行储层非均质研究,对查明油藏剩余油分布、采取合理注采措施、提高采收率显得十分必要。以吉林油田大208区黑帝庙油层三角洲前缘亚相储层为例,采用隔夹层识别对比、沉积微相分析、地质统计学系数和劳伦兹系数方法分析了层间、层内和平面非均质性。研究表明：黑帝庙油层发育3套稳定隔层,据此可划分为3套开发层系; 夹层在各单砂体中比较发育,应将夹层分割的注采井归为不同注采井网; 非均质性受沉积微相影响明显,水下分流河道和河口坝微相的非均质性最强; 地质统计学参数和劳伦兹系数研究表明,黑帝庙油层10个单砂体均为极强的非均质性,统计学参数往往偏离强非均质标准甚远,而劳伦兹参数值分布于0～1间,更能直观定量的表现出储层宏观非均质性强弱。  相似文献   

SCS2D程序反演参数的应用效果分析     

李茂  张俊伟  伍显红  许弟桥 《铀矿地质》2010,26(6):369-375

SCS2D程序中反演参数应用不当将使反演的地电模型与实际的地电模型产生较大的差别。通过对该软件反演参数圆滑系数、模型顶层厚度、初始背景模型的应用效果分析,为正确选择应用各参数、提高资料的反演精度打下基础。  相似文献