垂直气柱中大气微量成分总含量的反演

提出了一种利用地面中等光谱分辨率的太阳红外光谱反演整层大气中某几种微量成分总含量的方法,用逐线积分（ Ｌ Ｂ Ｌ） 法计算整层大气分子吸收,采用差分吸收法测量太阳红外光谱得到实际大气中微量成分的吸收,用最大似然法反演出微量成分的总量。详细分析了这种方法的可行性和反演精度,数值模拟分析和实际测量表明该方法有较高的精度,已把该方法用于监测实际大气中甲烷和水汽总含量的变化。     

中尺度大气波动的波谱和谱函数——数学模型和计算方法

作者得到了准二维Boussinesq方程组，并用其研究了中尺度大气波动的波谱和谱函数。在一定条件下对该方程组线性化并取标准模后，可将其初边值问题转化为矩阵的广义特征值问题来进行数值求解，这样就可知原问题波谱和谱函数的性质。当无基本流且取地转参数、层结参数为常数时，可求得其波谱和谱函数的解析解。此时该模式中仅包含有一对重力惯性内波模态，且各模态均是简谐波；模态越高，垂直波数越大则波动传播得越慢，所有的模态均为离散谱，并存在聚点。对此作者用数值解作了验算，结果表明，该数值求解方案合理可行，对不太高的模态其精度也令人满意。在无基本流然而考虑层结的垂直变化后，则一般无法求取解析解，为此进行了数值求解。这时该模式仍仅包含有一对重力惯性内波的离散谱模态，不过由于层结参数的变化，各模态结构与简谐波出现了偏差。     

基于Clementine热红外数据的Apollo17登月点区域氧化钙含量反演

为了研究利用Clementine热红外数据反演月球表面岩石的氧化钙(Ca O)含量,论文选取了两景覆盖Apollo17登月点的Clementine热红外影像,将其覆盖的区域选为研究区。利用月球表面温度物理模型模拟月表温度,结合普朗克函数,完成发射率反演。在此基础上,对LPI中35个除Apollo17登月计划外所采集的样品Ca O含量与其热红外发射率特征做回归统计分析,发现存在很好的线性关系(R2=0.661)。由此,基于Clementine热红外发射率实现了研究区Ca O含量反演。通过利用LPI Apollo17月岩(壤)样品实际Ca O含量分析数据对反演结果进行精度评价,发现8组反演值与实际值的相对误差最小为1.77%,最大为9.29%,均方根误差为0.767。研究结果表明,使用发射率进行Ca O含量反演方法可行,为利用Clementine热红外数据对月表矿物成分含量定量反演提供一种新的思路。     

张北-尚义地震震前阶段中小地震速度谱周期特征的研究

从 Duda 和 Nortmann 提出的谱震级定义出发,利用北京台网中小地震速度数字化记录资料,采用14组0.5倍频程滤波器组,其中心周期为:0.04s、0.06s、0.08s、0.12s、0.18s、0.28 s、0.40s、0.60s、0.96s、1.28s、2.40s、3.80s、6.20s、10.00s,分别计算了各中小地震的速度 谱综合因子f值,结果显示张北-尚义地震震前阶段中小地震的三分向速度谱卓越频率向高频 方向偏离,综合因子 f 值逐渐增加,且蓝地震的发生有向主震震中靠拢的趋势。同时,研究认为 综合因子 f 值可以量化蓝地震的定义。     

Thickness estimates of the upper-mantle transition zone from bootstrapped velocity spectrum stacks of receiver functions

We modify the receiver-functions stacking technique known as velocity spectrum stacking (VSS) so as to estimate combinations of velocity model ( V_P and V_S ) and depth that stack the Ps conversion from upper-mantle discontinuities most coherently. We find that by estimating the differences in the depths to the 660 and 410 km discontinuities using velocities that maximize the stacked amplitudes of P410s and P660s phases we can estimate the thickness of the transition zone more accurately than the depths to either of these discontinuities. We present two examples indicating that the transition zone beneath Obninsk, Russia, is 252±6 km thick and that beneath Pasadena, California, is only 220±6 km thick.     

AR模型谱在超导重力数据信号检测中的分析研究

在介绍AR(auto-regression)模型谱分析原理的基础上,分别采用AR模型谱和周期图法对法国Strasbourg、澳大利亚Mt Stromlo和日本Matsushiro三个站的超导重力数据进行信号检测,以半日波的理论值[1]为依据,运用两种方法进行半日波信号检测、分析与比较。结果表明,在超导重力数据信号检测分析中,AR模型谱比周期图法更准确、稳定,且受数据量的影响较小。     

缅甸 Mong Hsu 红宝石的颜色成因

摘 要 Mong Hsu 红宝石原石具有独特的暗蓝至紫色的核心色带‚即黑心。这种黑心可以借 助热处理法加以去除‚从而改善其颜色。通过对 Mong Hsu 红宝石化学成分及可见光谱的研 究‚阐明了其颜色成因与化学成分的关系‚分析了蓝紫色调的形成机理‚这些均为红宝石的 热处理提供了理论依据。     

Evaluation of ASCE 7 equations for designing acceleration‐sensitive nonstructural components using data from instrumented buildings

This study uses instrumented buildings and models of code‐based designed buildings to validate the results of previous studies that highlighted the need to revise the ASCE 7 F_p equation for designing nonstructural components (NSCs) through utilizing oversimplified linear and nonlinear models. The evaluation of floor response spectra of a large number of instrumented buildings illustrates that, unlike the ASCE 7 approach, the in‐structure and the component amplification factors are a function of the ratio of NSC period to the supporting building modal periods, the ground motion intensity, and the NSC location. It is also shown that the recorded ground motions at the base of instrumented buildings in most cases are significantly lower than design earthquake (DE) ground motions. Because ASCE 7 is meant to provide demands at a DE level, for a more reliable evaluation of the F_p equation, 2 representative archetype buildings are designed based on the ASCE 7‐16 seismic provisions and exposed to various ground motion intensity levels (including those consistent with the ones experienced by instrumented buildings and the DE). Simulation results of the archetype buildings, consistent with previous numerical studies, illustrate the tendency of the ASCE 7 in‐structure amplification factor, [1 + 2(z/h)] , to significantly overestimate demands at all floor levels and the ASCE 7 limit of to in many cases underestimate the calculated NSC amplification factors. Furthermore, the product of these 2 amplification factors (that represents the normalized peak NSC acceleration) in some cases exceeds the ASCE 7 equation by a factor up to 1.50.     

A laboratory study of directional spectra with maximum likelihood method-Ⅰ Developing wind wave

measurements by a circular array consisting of 18 wave gauges in a large wave tank, directional spectra of wind-generated waves in deep water are systematically determined by using maximum likelihood method The investigations reveal that the angular spreading of the wave energy is consistent with cos^2s(θ/2) proposed by Longuet-Higgins et al.(1963, Ocean Wave Spectra, 111-136), if the bimodal distributions of wave energy are not taken into account. Bimodality occurring on higher frequency than peak frequency is too rare to affect our whole resalts. Surprisingly, a much broader directional spreading than that of the field, which is interpreted by the strongly nonlinear energy transfer because of the very young waves in laboratory, is found. The parameter s depends on frequency in the same way as observed by Mitsuyasu et al.(1975, Journal of Physical Oceanography, 5, 750-760) and Hasselmann et al.(1980, Journal of Physical Oceanography, 10, 1264-1280) in the field, and the relationship between the four nondimensional parameters s_m, f_o, b₁ and b₂, determining the directional width, and ū₁₀ (corresponding to the inverse of wave age) are given respectively. The observed distributions are found to agree well with the suggestion of Donelan et al.(1985, Philosophical Transaction of Royal Society of London, A315, 509-562) when applied to field waves.     

应用~(40)Ar/~(39)Ar定年技术研究清原花岗岩-绿岩地体的形成时代

辽宁清原绿岩地层自下而上分为榆树底组、红透山组和南天门组。小莱河铁矿区榆树底组斜长角闪岩岩石化学性质和稀土元素分布曲线表明,该岩石的原岩属太古代亏损型(DAT)拉斑玄武岩。此斜长角闪岩中的角闪石的两个~(40)Ar/~(39)Ar年龄谱给出该岩石的变质作用发生在29.9亿年。清原绿岩地层形成时代可能在30亿年或稍早一些。全球范围绿岩地层的年龄是35—19亿年,峰值是27亿年.清原绿岩地层的早期形成年龄则大于全球绿岩的峰值年龄。