Nitrogen isotopic geochemical characteristics of crude oils in several basins of China

Nitrogen occupies a high content in crust and in atmospheric circle. It is one of the main elements in organism and an important element in sedimentary circle. Although nitrogen is little in crude oil, to a cer-tain degree, it influences the physical and chemical properties of oil, such as viscosity and density[1]. In reservoir the nitrogen-bearing compounds can form ion bonds or hydrogen bonds with substances on rock and form van der Vaals’ force among moleculae so they affect and alter the …     

Impacts of land-use and climate changes on ecosystem productivity and carbon cycle in the cropping-grazing transitional zone in China

Terrestrial ecosystems are both a carbon source and sink, therefore play an important role in the global carbon cycle that act as a link of interactions between human activities and climate changes[1,2]. Climate change impacts ecosystem carbon cycle through af- fecting biological processes, e.g. plant photosynthesis, respiration, and soil carbon decomposition. Land-use change directly modifies the distribution and structure of terrestrial ecosystems and hence the carbon storage and fluxes. Usi…     

Photometric studies of three Be stars

From 1978 December to 1979 May, we made spectrographic observations of φPer, ζTau and κDra using our Schmidt cassegrain grating spectrograph. Values of electron density, rotational speed and variation have been obtained and a comparison between ζTau and the supergiant βOri carried out. We found that, over our observed period, θPer showed clear shell activities, ζTau was in a relatively calm phase, its shell slowly expanding, while κDra had all the signs of a “classical” Be star.     

Cross-correlation between WMAP and 2MASS: non-Gaussianity induced by the SZ effect

We study the non-Gaussianity induced by the Sunyaev–Zel'dovich (SZ) effect in cosmic microwave background (CMB) fluctuation maps. If a CMB map is contaminated by the SZ effect of galaxies or galaxy clusters, the CMB maps should have similar non-Gaussian features to the galaxy and cluster fields. Using the WMAP data and 2MASS galaxy catalogue, we show that the non-Gaussianity of the 2MASS galaxies is imprinted on WMAP maps. The signature of non-Gaussianity can be seen with the fourth-order cross-correlation between the wavelet variables of the WMAP maps and 2MASS clusters. The intensity of the fourth-order non-Gaussian features is found to be consistent with the contamination of the SZ effect of 2MASS galaxies. We also show that this non-Gaussianity can not be seen by the high-order autocorrelation of the WMAP . This is because the SZ signals in the autocorrelations of the WMAP data generally are weaker than the WMAP –2MASS cross-correlations by a factor f ², which is the ratio between the powers of the SZ-effect map and the CMB fluctuations on the scale considered. Therefore, the ratio of high-order autocorrelations of CMB maps to cross-correlations of the CMB maps and galaxy field would be effective to constrain the powers of the SZ effect on various scales.     

High-Spatial-Resolution Imaging Combining High-Order Adaptive Optics,Frame Selection,and Speckle Masking Reconstruction

We present, for the first time, high-spatial-resolution observations combining high-order adaptive optics (AO), frame selection, and post-facto image correction via speckle masking. The data analysis is based on observations of solar active region NOAA 10486 taken with the Dunn Solar Telescope (DST) at the Sacramento Peak Observatory (SPO) of the National Solar Observatory (NSO) on 29 October 2003. The high Strehl ratio encountered in AO corrected short-exposure images provides highly improved signal-to-noise ratios leading to a superior recovery of the object’s Fourier phases. This allows reliable detection of small-scale solar features near the diffraction limit of the telescope. Speckle masking imaging provides access to high-order wavefront aberrations, which predominantly originate at high atmospheric layers and are only partially corrected by the AO system. In addition, the observations provided qualitative measures of the image correction away from the lock point of the AO system. We further present a brief inspection of the underlying imaging theory discussing the limitations and prospects of this multi-faceted image reconstruction approach in terms of the recovery of spatial information, photometric accuracy, and spectroscopic applications.The editors apologize to the authors: due to a misunderstanding during the editorial process, the publication of this paper has been delayed.     

板状绿柱石晶体的结构测定

自然界中绿柱石晶体多为柱状,具板状晶形的绿柱石非常少见。本文对产于四川雪宝顶云英岩晶洞中的无色透明板状绿柱石进行了精确的结构分析,并与产于阿尔泰山号伟晶岩脉中的柱状绿柱石进行了比较。与阿尔泰柱状绿柱石相比,雪面板状绿石富Ｌi、Ｎａ,ｃ／ａ值较高,为１．００１,属钠－锂绿柱石或“四面体”绿柱石。本文还对这种特殊形貌柱石的形成机制进行了初步讨论,成矿流体中Ｌi的浓度以及Ｓi的化学形态可能是影响柱石忻驳闹     

资料插值的进展

对气候学中资料插值、数值天气预报中的客观分析和气候模拟中的降尺度技术作了统一论述，重点是气候资料插值的原理和进展。由于应用领域不同，这些技术也是很不相同的，但它们的动力学和统计学原理是相近或一致的。近十年来三种插值技术，尤其在建立计算机自动化插值系统方面，都取得了长足进展。     

北半球春季大气臭氧变化特征及其对大气温度和环流场的影响

该文利用美国1978～1993年TOMS臭氧资料以及NCEP提供的全球再分析资料,研究北半球大气臭氧变化特征及其对大气温度和环流的影响.研究表明1987年前后北半球40°N以北的中高纬地区春季大气臭氧柱总量的趋势变化存在明显的突变,大部分地区突然减少,与其相对应的对流层(平流层)平均温度突然升高(降低),300 hPa(30 hPa)层位势高度也突然增高(下降).但是在北大西洋北部和哈德逊湾地区大气臭氧柱总量却突然增加,与其相对应的对流层(平流层)平均温度突然降低(升高),300 hPa(30 hPa)位势高度突然下降(增高),平均温度突然升高(降低 )1～2°C.研究还表明,大气温度和环流的趋势变化主要是由于大气臭氧的趋势变化所引起.另一方面,在同一地区1979～1992年春季大气臭氧柱总量强弱异常年的大气温度场和环流场的差异也存在相同的分布特征,这一事实进一步说明大气臭氧柱总量的多少是决定大气温度场和环流场差异的重要原因.     

柴达木盆地新生代构造样式的演化特点

本文将柴达木盆地新生代构造样式的演化归纳为６种序列和两个主要阶段,即冲断构造→生背斜→反冲断层→断层背斜序列、生长背斜→反冲断层＋断层疹斜序列、生长背斜→纵弯背斜序列、生长断层→滑脱褶皱序列、水平岩层→纵弯背斜序列。构造样式的演化具有明显的地区性特点,盆地南北两侧具似性,而盆地中央呈东西差异。两个阶段是喜马拉雅早中期的压缩构造样式发育阶段和晚期的强烈压缩构造样式发育阶段。控制柴达木盆地构造样式规律     

基于信号重构的地震道插值

在简要回顾几种插值方法的基础上 ,提出了基于信号重构的地震道插值方法。这种方法无需任何地质和地球物理假设 ,主要用于恢复缺失的地震道。本方法的基础是傅立叶变换理论和最小平方反演技术。文中给出了原理、算法、实现步骤及简要的流程框图。如果对变换域的参数进行规则采样 ,则该方法可以用高效、快速的算法来实现。本插值方法适用于规则和非规则采样的数据。文中给出了理论合成数据和实际数据的试验结果 ,并对结果进行了讨论。同时 ,本方法对于 AVO分析、DMO处理、三维叠前偏移成像等研究也将是有益的