利用激发极化驰豫时间谱确定渗透率的实验研究   总被引：1，自引：1，他引：0  

童茂松  王伟男  范清华  姜亦忠  王荣  杜国同 《吉林大学学报(地球科学版)》2004,34(4):625-629

激发极化驰豫时间是孔隙大小的函数,采用奇异值分解方法对激发极化衰减曲线进行多指数反演,得到光滑的驰豫时间谱,该谱呈现多峰特性.实验结果表明,溶质对该谱的影响主要是由于溶质离子的扩散系数不同所致.对于同一块岩心,衰减谱随扩散系数的增大而向小驰豫时间方向移动.结合岩心地层因素F,研究了激发极化驰豫时间几何平均值Tg与岩石的渗透率K的关系,结果表明,logK和log(T1/2g/F)、log(Tg/F)呈现良好的线性关系.  相似文献   

Presence of LaO, ScO and VO Molecular Lines in Sunspot Umbral Spectra     

P. Sriramachandran  S. P. Bagare  N. Rajamanickam  K. Balachandrakumar 《Solar physics》2008,252(2):267-281

High-resolution Fourier Transform Spectrometer sunspot umbral spectra of the National Solar Observatory/National Optical Astronomy Observatory at Kitt Peak were used to detect rotational lines from 19 electronic transition bands of the molecules LaO, ScO and VO, in the wavenumber range of 11 775 to 20 600 cm⁻¹. The presence of lines from the following transitions is confirmed: A ² Π _r1/2 – X ² Σ ⁺(0, 0; 0, 1), A ² Π _r3/2 – X ² Σ ⁺(1, 0), B ² Σ ⁺ – X ² Σ ⁺(0, 0; 0, 1; 1, 0) and C ² Π _r1/2 – A′²Δ _r3/2(0, 0; 1, 1) of LaO; A ² Π _r3/2 – X ² Σ ⁺(0, 0), A ² Π _r1/2 – X ² Σ ⁺(0, 0) and B ² Σ ⁺ – X ² Σ ⁺(0, 0) of ScO; and C ⁴ Σ ⁻ – X ⁴ Σ ⁻(0, 1; 1, 0; 0, 2) and (2, 0) of VO. However, the presence of A ² Π _r3/2 – X ² Σ ⁺(0, 0) and C ² Π _r3/2 – A′²Δ _r5/2(0, 0; 1, 1) of LaO and C ⁴ Σ ⁻ – X ⁴ Σ ⁻(0, 0) of VO are found to be doubtful because the lines are very weak, and detections are difficult owing to heavy blending by strong rotational lines of other molecules. Equivalent widths are measured for well-resolved lines and, thereby, the effective rotational temperatures are estimated for the systems for which the presence is confirmed.  相似文献   

Lithium abundance in sunspots     

E. A. Baranovsky  V. P. Tarashchuk 《Bulletin of the Crimean Astrophysical Observatory》2008,104(1):19-25

The observations of lithium were carried out with the TST-2 telescope at CrAO on August 15–20, 2006. A sunspot model was calculated for the dates of observations. The lithium abundance in a sunspot and in the undisturbed photosphere was determined. It is log(N _Li) = 1.35 for the sunspot and log (N _Li) = 1.05 for the undisturbed photosphere.  相似文献   

张家口地震台和兴隆地震台地脉动信号初步分析   总被引：1，自引：0，他引：1  

张从珍  高景春  刁桂苓  赵英萍  宋梦真 《华北地震科学》2004,22(3):56-60

选取河北省张家口和兴隆2个台站的数字化地震仪连续1年,每日02～03时的地脉动记录,计算功率谱和自相关函数。结果发现兴隆台脉动谱中有4个比较突出的峰值,分别为0．3Hz、3Hz、8Hz、15Hz,张家口台只有3个峰值0．3Hz、3Hz、15Hz。兴隆台UD向的自相关函数呈现出一种比较典型的“红噪声”形态,EW向则呈现出负相关特征,认为可能是只作用于水平向的倾斜脉动的影响。小幅度的仪器干扰信号无论从脉冲标定还是地震波形中都很难发现的,而对脉动进行谱分析则很容易分辨。兴隆台和张家口台地脉动卓越周期时间曲线,基本集中在0．3秒,比较稳定。  相似文献   

ATMOSPHERIC TURBULENCE STRUCTURE AND SPECTRAL CHARACTERISTICS AT NEAR SURFACE LAYER ON TROPICAL COASTS     

邓雪娇  吴兑 《热带气象学报(英文版)》1997,3(1):27-34

By use of an observational experiment at the village of Tianwei, Haikou, Hainan province in 1990,characteristic turbulence values such as velocity component spectra and turbulence intensity are studied.The data were mostly obtained in cloudy condition, so that the stability parameter (L) and thermal flux (wt) did not vary diurnally while the turbulent energy and mean-temperature did. The basic characteristics of turbulence spectra are similar to those with fine weather, hems close to local isotropy in the inertial subrange. The velocity spectra agree with the law of "-2/3 th power"in Kolmogrov's similarity theory. The relationship between turbulent intensity of components δ_i/U (i=u,v,w) and stability Z/L is studied follow ins the Monim-Obukhov(M-O) similarity theory. It is shown that the two observe the law of "1/3 th power", though the turbulent intensity and energy are generally larger than those on the flat underlying topography.  相似文献   

极光粒子沉降研究:谱形式及其在极区大气中的传输   总被引：1，自引：0，他引：1       下载免费PDF全文

宗秋刚  付绥燕  濮祖荫  叶宗海  余彬 《极地研究》1999,11(3):203-220

分析了近年来南极地区极光沉降粒子的卫星、火箭、地面观测和研究结果,分别给出了极光椭圆区、极盖区、南大西洋异常区和极尖／极隙区粒子沉降的形式来源和特点。并根据磁尾研究的新进展,提出极光粒子沉降谱存在另外两种形式谱：（１）κ分布谱;（２）κ分布加上一个或多个脉冲谱,这两种谱来源于磁尾中性片区（绝热区非绝热区）。南极不同的区域,极光粒子有不同的沉降特点。这些沉降对极区电离层产生极大的影响。根据带电粒子在磁化大气中运动的Ｆｏｋｋｅｒ Ｐｌａｎｋ 方程,利用带电粒子在大气中传输的电离理论,导出极光粒子谱在极区大气中传播的解析表达式,对各种极光粒子谱在极区中的演化规律加以分析,并以此来解释在南极地区探测到的不同高度的极光电子谱的演化  相似文献   

A record of changing redox conditions in the northern Peru Basin during the Late Quaternary deduced from Mn/Fe and growth rate variations in two diagenetic manganese nodules     

A. Bollhfer  N. Frank  S. Rohloff  A. Mangini  J.C. Scholten 《Earth and Planetary Science Letters》1999,170(4):91-415

Two diagenetic manganese nodules from the Peru Basin were investigated by thermal ionization mass spectrometry and high resolution alpha spectrometry for uranium and thorium. The TIMS concentrations for nodule 62KD (63KG) vary as follows: 0.12–1.01 ppb (0.06–0.59) ²³⁰Th, 0.51–1.98 ppm (0.43–1.40) ²³²Th, 0.13–0.80 ppb (0.09–0.49) ²³⁴U, and 1.95–13.47 ppm (1.66–8.24) ²³⁸U. Both nodules have average growth rates of 110 mm per million years. However, from the variations of excess ²³⁰Th with depth we estimate partial accumulation rates which range from 50 to 400 mm per million years. The δ²³⁴U dating method cannot be applied due to remobilization of U from the sediment and subsequent incorporation into the nodules' crystal lattice, reflected by decay corrected δ²³⁴U values far above the ocean water value. Sections of fast nodule growth are related to those layers having high Mn/Fe ratios (up to 200) and higher densities. As a possible explanation we develop a scenario that describes similar glacial/interglacial trends in both nodules as a record of regional changes of sediment and/or deep water chemistry.  相似文献   

星叶石族矿物红外光谱研究   总被引：4，自引：0，他引：4  

李国武  马喆生  施倪承  N.A.Yamnova 《矿物学报》1999,19(1):9-14

在新测定的星叶石晶体结构资料的基础上,对星叶石矿物进行了详细和红外光谱研究,对比了单斜及三斜星叶石的红光谱特征,并对星叶石中工外吸收振动的归属问题进行了讨论。  相似文献   

A Possible Mechanism of Ocean Finestructure Part Ⅰ: Energy and Coherence     

范植松  方欣华 《中国海洋大学学报(自然科学版)》1999,(2)

依据在作者的前文（１９９８）中对于考虑旋转向量水平分量（ｆ～）的大洋内波方程求出的渐近解,文中对Ｓ场（考虑ｆ～条件下的总的内波场）,ＳＩ场（不计ｆ～影响的内波场）和ＳＦ场（Ｓ场中与ｆ～相关联的部分）导出了能量谱和相干谱。此理论谱与Ｍｕｌｅｒ等（１９７８）的ＩＷＥＸ实验的观测结果相比较表明,ＳＦ场的水平动能谱和铅直位移谱基本上与水平流细结构和铅直位移细结构的观测谱一致。作者推测ＳＦ场对应于中纬度大洋可逆细结构。但是对于相干谱的观测结果,在不考虑内波非线性相互作用和破碎过程的条件下,仅考虑ＳＦ场的影响还不能给予满意的解释。  相似文献   

近断层竖向地震动P-Δ效应研究   总被引：1，自引：1，他引：0  

范优铭  夏群 《震灾防御技术》2017,12(1):177-184

竖向效应是近断层地震动的主要特点,竖向地震动对工程结构形成的P-Δ效应是造成结构破坏的主要原因。本文以单自由度体系为研究对象,选取汶川地震的近断层强震数据进行研究,分析竖向地震动所产生P-Δ效应的放大作用特征。分析结果表明汶川地震中,相比于中远场区域,近断层区域内竖向地震动作用所产生的P-Δ效应具有明显的放大作用,且近断层内这种放大作用具有普遍性;当自振周期一定时,不同台站获得地震动的放大系数离散性较小,主要分布于均值附近;其分析结果符合地震动的一般规律,分析结果合理。在此基础上建立了以均值为代表值的放大系数谱,可以与抗震设计反应谱结合使用,从而为活断层附近区域内的结构抗震设计问题提供定量化参考依据。  相似文献