类星体吸收线

类星体光谱中有大量的吸收线 ,它们或者产生于与类星体本身有联系的气体云 ,或者产生于类星体和观测者之间的吸收系统。因此 ,类星体吸收线是强有力的宇宙探针。对类星体吸收线的研究将有助于我们了解星系的形成和演化。本文介绍了类星体吸收线的性质并评述了近年来类星体吸收研究的最新进展。     

The amplitude of mass density fluctuations at z 3.25 from the Ly forest of Q1422+231

The real-space optical-depth distribution along the line of sight to the QSO Q1422+231 is recovered from two HIRES spectra using a modified version of the inversion method proposed by Nusser & Haehnelt. The first two moments of the truncated optical-depth distribution are used to constrain the density-fluctuation amplitude of the intergalactic medium (IGM) assuming that the IGM is photoionized by a metagalactic UV background and obeys a temperaturedensity relation. The fluctuation amplitude and the power-law index of the relation between gas and neutral hydrogen (H  i ) density are degenerate. The rms of the IGM density at z 3.25 estimated from the first spectrum is with 1.56< <2 for plausible reionization histories. This corresponds to 0.9 2.1 with ( =1.7)=1.44±0.3. The values obtained from the second spectrum are higher by 20 per cent. If the IGM density traces the dark matter (DM) as suggested by numerical simulations we have measured the fluctuation amplitude of the DM density at an effective Jeans scale of a few 100 kpc. For cold dark matter (CDM)-like power spectra the amplitude of dark matter fluctuations on these small scales depends on the cosmological density parameter . For power spectra normalized to reproduce the space density of present-day clusters and with a slope parameter of =0.21 consistent with the observed galaxy power spectrum, the inferred can be expressed as: =0.61( /1.7)^1.3( x _J/0.62)^0.6 for a flat universe, and =0.91( /1.7)^1.3( x _J/0.62)^0.7 for a =0 universe. x _J is the effective Jeans scale in (comoving) h ¹ Mpc. Based on a suite of detailed mock spectra the 1 error is 25 per cent. The estimates increase with increasing . For the second spectrum we obtain 15 per cent lower values.     

膨胀土阳离子交换量的测定

应用对膨胀土勘测样的蒙脱石含量和阳离子交换量测定数据 ,按行业标准对膨胀土进行了评判和分级。两种方法的判别和分级结果基本相符 ,能满足工程地质膨胀土的测试要求     

合兴场地震资料吸收油气预测研究

在地震勘探中快速有效地进行油气预测的方法研究已成为我们目前十分重要的研究课题。我们研究了对地震资料利用吸收衰减理论对油气进行预测的油气预测实用技术。     

人体泌尿系统结石及人发成分分析的意义

利用红外光谱分析法对尿路结石进行了物相分析,并用原子吸收分光光度法测定了结石和发样的微量元素,根据结石的物相特征、微量元素含量以及与人体发样微量元素含量进行对比分析,探讨了尿路结石的成因、影响因素及预防措施。     

纳米碳纤维红外消光数值计算

为探讨纳米碳纤维作为烟幕粒子的红外消光特性,基于电磁场理论建立了细直的纳米碳纤维感应电流积分方程,并利用矩量法进行了求解,导出了纳米碳纤维散射场及吸收、散射和消光截面的计算式.通过与变分法的计算结果相比较,表明了该方法的有效性.利用该方法数值分析了纳米碳纤维红外消光截面与入射场波长、入射角、纤维长度和半径的关系,计算结果为纳米碳纤维用于红外烟幕干扰提供了理论依据.     

NaAlH4 表面Ti催化空间构型和X射线吸收光谱:Car-Parrinello分子动力学和密度泛函理论研究

通过采用Car-Parrinello分子动力学方法对掺杂Ti前后的NaAlH₄(001)2×2×1超晶胞表面晶体在333 K(60 ℃)温度条件催化脱氢的空间构型做了理论研究,发现掺杂Ti的合金中AlH₄团的其中两个Al—H键长分别从约1.64 (1 =0.1 nm)增大至1.74和1.93 ,而未掺杂合金表面中AlH₄团的4个Al—H键长基本不变,这意味着掺杂Ti相对未掺杂的合金更易于放氢.但在模拟温度条件下并未发现Ti-Al成键趋     

Tunable surface-plasmon-resonance wavelength of silver island films

This paper experimentally and theoretically investigates the effect of the underlayer medium on tuning of the surface plasmon resonance (SPR) wavelength of silver island films, and the effect of substrate temperature on the morphologies and optical properties of the films. From the absorption spectra of single Ag with various thickness and overcoated (Ag/TiO₂) films deposited on glass substrates at various substrate temperatures by RF magnetron sputtering, we demonstrate that the surface plasmon resonance wavelength can be made tunable by changing the underlayer medium, the thickness of metal layer and the substrate temperature. By varying substrate temperatures, the interparticle coupling effects on plasmon resonances of nanosilver particles enhance as the spacing between the particles reduces. When the substrate temperature is up to 500 ℃, the absorption peak decreases sharply and shifts to shorter wavelength side due to the severe coalescence between silver islands in the film.     

基于两种半分析算法的水体吸收系数反演

本文基于42组不同年份不同季节获得的遥感反射率、水体各组分吸收系数的实测数据,对QAA（Quasi-Analytical Algorithm）和GSM（Garver-Siegel-Maritorena）算法在寡营养的南海和富营养的福建沿岸两种不同类型水体的吸收系数反演进行了检验。以水样测量值为参考,两种算法在本研究水体中的反演成效与他人在其它水域的研究结果相当。QAA算法在南海的反演成效高于福建沿岸水体。对于443 nm的总吸收系数（a443 ）,南海的对数均方根误差（RMSE ）为0.046,平均相对误差为7.9%,对数平均偏差为0;福建沿岸水体的对数均方根误差（RMSE ）为0.194,平均相对误差为30.6%,对数平均偏差为-0.167 。GSM算法在两类水体的反演成效类似,A443 之RMSE和平均相对误差,南海分别为0.161和27.7%,福建沿岸分别为0.149和32.1%,但从A443的对数平均偏差值看,其在南海反演值低于实测值（对数平均偏差为-0.142 ）,在福建沿岸则略呈高于实测值（对数平均偏差为0.016）。两种算法中的部分经验参数与实测值之间的差异是产生反演误差的主要原因,为了提高反演精度,对算法中经验参数的更进一步区域化调整可能是必要的。