地震前电磁辐射信息特征研究

反映电磁辐射信息的地震前异常变化很多,但都有一个震前平静－加强－平静然后发震的特征,为了更好地体现这种特征,根据十几年来河北廊坊电磁台网的观测资料,通过给不同强度段的各台日信息量赋予不同的权值,并把当日各台权值累加来反映当日内多台信息量集中的强弱,然后把上述权累加和用一种不连续积分的方法反映异常的持续时间,通过对监测范围内４次Ｍｓ≥５．０地震震例分析,发现该方法反映震前异常特征明显,短临效果很好,     

Five dimensional universe model with variable cosmological term Λ and a big bounce

We assume the four dimensional induced matter of the 5D Ricci flat bouncing cosmological solution contains a perfect fluid. The big bounce singularity of simple 5D cosmological model is studied with the cosmological term Λ=α ρ and Λ=β H ² where α and β are constants and ρ and H are respectively energy density and Hubble parameter. This big bounce singularity is found to be an event horizon at which the scale factor and mass density of the universe are finite, while the pressure is infinite.      

土壤铅含量高光谱遥感反演中波段选择方法研究

利用高光谱遥感数据进行了南京郊外土壤重金属元素铅的含量反演,由于高光谱数据波段众多,波段选择或变换至关重要。比较了基于次贪婪的前向选择模型的最小角度拟合和基于遗传算法进行波段选择的最小二乘和偏最小二乘拟合,结果发现基于遗传算法的偏最小二乘反演结果优于全波段的偏最小二乘,表明波段选择在高光谱反演重金属中是有益的。尽管采取了波段选择后的各方法在反演时均能达到70%以上的训练精度,但因遗传算法搜索的解空间范围更宽广,使得基于遗传算法的偏最小二乘优于前向选择模型的最小角度拟合。最后还比较了基于遗传算法的普通最小二乘和偏最小二乘拟合,结果表明偏最小二乘更优,因此在高光谱反演重金属含量当中,偏最小二乘精度较高,而在波段选择方法中,遗传算法更优。     

阿拉善地区土壤盐渍化的遥感反演及分布特征

土壤盐渍化是威胁干旱区土地的重要环境问题。利用遥感技术对土壤盐渍化进行动态监测,分析土壤盐度水平与空间分布,有利于掌握土壤盐渍化现状,为土地资源可持续利用提供理论依据。现有研究多在田间尺度,随着土壤环境问题涉及的范围越来越大,区域斑块信息的提取已无法满足宏观地模拟和展示整体土壤环境的空间分布。以阿拉善地区为例,结合遥感光谱指数与实测土壤盐分数据,运用偏最小二乘回归（PLSR）方法,构建区域尺度范围的土壤盐渍化反演模型,实现大面积地区土壤盐度的精准模拟和定量监测。结果表明,构建的模型验证精度达到0.8788,达到极显著水平,预测结果与实际情况相符,可以较准确地模拟研究区土壤盐渍化状况。受地形、气候、景观类型、农业活动以及土地管理等因素的综合影响,阿拉善地区约20%的区域土壤呈现出不同程度的盐渍化,其中黑河下游河岸带、雅布赖山西侧及贺兰山西侧冲积扇土壤盐渍化程度最为严重。本研究可为大面积区域土壤盐分状况的快速监测及遥感定量反演提供可行的方法,同时为该区域不同程度盐渍化土壤的治理和土地利用管理提供依据。     

Study of frequency domain full waveform inversion based on Huber norm and L-BFGS algorithm

Full waveform inversion( FWI)is a high resolution inversion method,which can reveal detailed in-formation of the structure and lithology under comPlex geological background. It is limited by many kinds...     

甘肃白银厂矿区及其外围铜矿床成矿特征与定量预测

北祁连地区是我国重要的海相火山成因铜多金属块状硫化物矿床成矿带,位于该区东段的白银矿田内产出有多个大型-特大型VMS矿床,具有较好的找矿前景.在该地区铜矿床成矿特征研究的基础上,利用GIS技术提取与成矿有关的地层、构造、岩浆岩、地球化学等多元找矿信息,构建了白银矿区及外围铜矿床的证据权重找矿模型,利用后验概率圈定出找矿远景区,按照各找矿远景区相对成矿可能性的大小和各找矿标志将远景区分为Ⅰ、Ⅱ、Ⅲ3级,各级找矿远景区各3个.     

Λ Varying Cosmological Models with Viscous Fluid

Evolution of a homogeneous, isotropic Universe with flat geometry filled with a viscous fluid is investigated in presence of a variable cosmological Λ. A non-singular solution leading to a variable deceleration parameter is obtained which reduces to the solution of Murphy in the ‘no Λ limit’ and to the recent solution of Vishwakarma in the context of ‘a Machian model of dark energy’ in the ‘no viscosity’ limit.     

UBV光电测光系统的转换方程和精度比较

根据对鬼星团中Ｊｏｈｎｓｏｎ测光标准星的观测，我们研究了北京天文台６０ｃｍ望远镜直流光电光度计ＵＢＶ测光系统的转换方程．应用该方程推算了对三颗变星观测得到的ＵＢＶ星等，讨论了所得光变曲线的精度，并与较差方法所得结果进行了比较     

Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni

In this study complete BV light curves of the W Ursae Majoris binary V1073 Cygni obtained in 2005 are presented. We have used the spectroscopic data of V1073 Cyg obtained by Ahn et al. (1992) for analysis. The analysis of radial velocity and light curves was made with Wilson} program (1998) and the geometric and physical elements} of the system were derived. By searching the simultaneous} solutions of the system, we have determined the masses and radii of the components: 1.64M_⊙, 2.275R_⊙ for the primary component and 0.55M_⊙, 1.397R_⊙ for the secondary component respectively. The effective temperature of 6494 ± 53 K for the secondary component was also estimated.     

A new class of bulk viscous universe with time dependent deceleration parameter and Λ-term

A new class of exact solutions of Einstein’s field equations with a bulk viscous fluid for an LRS Bianchi type-Ia obtained by using a time dependent deceleration parameter and cosmological term Λ. The coefficient of bulk viscosity is assumed to be a power function of mass density (ξ=ξ ₀ ρ ⁿ ). We have obtained a general solution of the field equations from which six models of the universe are derived: exponential, polynomial and sinusoidal form respectively. The behaviour of these models of the universe are also discussed in the frame of reference of recent supernovae Ia observations.