锆石红外光谱在地质研究中的应用     

闫秋实  尹观 《物探与化探》2004,28(2):142-146

以甘肃白银厂地区的7件锆石同位素年龄样品为例,根据其红外光谱中615cm-1吸收峰的高和半高宽度的比值,将锆石样品的变生程度量化,并将其分为晶质锆石、半变生锆石和变生锆石3类。参考相关资料,利用7件锆石样品的红外光谱特征对其铀钍含量和"红外年龄"做了估测,并将估测年龄与其U Th年龄和全岩Rb Sr年龄进行了比较和分析。  相似文献   

原子吸收分光光度法快速测定铬铁矿中钙、镁、锰   总被引：2，自引：0，他引：2  

熊艳 《安徽地质》2006,16(4):270-272

通过在标液中加入相应的Sr来消除离子干扰,采用原子吸收分光光度法快速测定CaO、MgO、MnO的含量,方法经国家标准物质验证,其RSD<2%(n=6)。其结果与标准值相符。方法达到了准确、简便、快速、实用性强。  相似文献   

近红外波段(900—2500 nm)水吸收系数测量   总被引：1，自引：0，他引：1  

邓孺孺  何颖清  秦雁  陈启东  陈蕾 《遥感学报》2012,16(1):192-206

根据水在红外波段强吸收且吸收能力变化大的特点,在所提出可见光波段水吸收系数测量系统基础上增设了薄层水测量装置,使得测量水层厚度可在0.04—350 mm之间变化。在此基础上对厚度为0.04—150 mm的多个厚度水层进行了吸收系数测量,并对消除杂质影响后的测量数据进行了有效整合,得到900—2500 nm波段纯水吸收系数。由于确保了各波段数据均在仪器最佳探测区间取得,所得结果精度较高,且与被普遍接受的前期研究结果相一致,可作为相关定量遥感的基础数据。  相似文献   

近红外大气吸收波段太阳辐射计定标     

伽丽丽  戴聪明  徐青山  魏合理 《遥感学报》2012,16(5):928-938

用通用大气辐射传输软件CART模拟了POM02太阳辐射计的1020nm、1627nm和2200nm等3个近红外通道的大气透过率特性。结果表明,前两通道处于大气非吸收波段,其透过率很好的遵从Beer-Lambert定律,而2200nm通道则有较强的吸收,吸收光学厚度随大气质量的变化服从指数分布,与Beer-Lambert定律有一定的偏差,其定标需采用改进的Langley法。通过选取好天的5个定标实例证明,采用改进的Langley法定标2200nm通道,可提高其透过率测量精度约3.8%。  相似文献   

The Effects of Line-Wing Cutoff in LBL Integration on Radiation Calculations          下载免费PDF全文

ZHANG Hu  SHI Guangyu  LIU Yi 《Acta Meteorologica Sinica》2008,22(2):248-255

There are three basic methods in radiative transfer calculations, i.e., line-by-line (LBL) integration, correlated k-distribution method, and band model. The LBL integration is the most accurate of all, in which, there are two quadrature algorithms named in this paper as integration by lines and by sampling "points when calculating atmospheric transmittance in the considered wavenumber region. Because the LBL integration is the most expensive of all, it is necessary and important to save calculation time but increase calculation speed when it is put into use in the daily operation in atmospheric remote sensing and atmospheric sounding. A simplified LBL method is given in this paper on the basis of integration by lines, which increases computational speed greatly with keeping the same accuracy. Then, we discuss the effects of different cutoff schemes on atmospheric absorption coefficient, transmittance, and cooling rate under both of accurate and simplified LBL methods in detail. There are four cutoff schemes described in this paper, i.e., CUTOFFs 1, 2, 3, and 4. It is shown by this numerical study that the way to cut off spectral line-wing has a great effect on the accuracy and speed of radiative calculations. The relative errors of the calculated absorption coefficients for CUTOFF 2 are the largest under different pressures, while for CUTOFF 1, they are less than 2% at most of sampling points and for CUTOFFs 3 or 4, they are ahnost less than 5% in the calculated spectral region, however, the calculation time is reduced greatly. We find in this study that the transmittance in the lower atmosphere is not sensitive to different LBL methods and different cutoff schemes. Whereas for the higher atmosphere, the differences of transmittance results between CUTOFF 2 and each of other three cutoff schemes are the biggest of all no matter for the accurate LBL or for the simplified LBL integrations. By comparison, the best and optimized cutoff scheme is given in this paper finally.  相似文献   

Metal absorption systems in spectra of pairs of QSOs: how absorbers cluster around QSOs and other absorbers     

David Tytler  Mark Gleed  Carl Melis  Angela Chapman  David Kirkman  Dan Lubin  Pascal Paschos  Tridivesh Jena  Arlin P. S. Crotts 《Monthly notices of the Royal Astronomical Society》2009,392(4):1539-1572

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Gravitational lensing of anisotropic sources     

Rosalba Perna  Charles R. Keeton 《Monthly notices of the Royal Astronomical Society》2009,397(2):1084-1092

In strong gravitational lensing, the multiple images we see correspond to light rays that leave the source in slightly different directions. If the source emission is anisotropic, the images may differ from conventional lensing predictions (which assume isotropy). To identify scales on which source anisotropy may be important, we study the angle δ between the light rays emerging from the source, for different lensing configurations. If the lens has a power-law profile   M ∝ R ^γ  , the angle δ initially increases with lens redshift and then either diverges (for a steep profile  γ < 1  ), remains constant (for an isothermal profile  γ= 1  ), or vanishes (for a shallow profile  γ > 1  ) as   z _l→ z _s  . The scaling with lens mass is roughly  δ∝ M ^1/(2−γ)  . The results for an Navarro–Frenk–White (NFW) profile are qualitatively similar to those for a shallow power law, with δ peaking at about half the redshift of the source (not half the distance). In practice, beaming could modify the statistics of beamed sources lensed by massive clusters: for an opening angle  θ_jet  , there is a probability as high as   P ∼ 0.02–0.07(θ_jet/0.5°)⁻¹  that one of the lensed images may be missed (for  2 ≲ z _s≲ 6  ). Differential absorption within active galactic nuclei (AGNs) could modify the flux ratios of AGNs lensed by clusters; a sample of AGNs lensed by clusters could provide further constraints on the sizes of absorbing regions. Source anisotropy is not likely to be a significant effect in galaxy-scale strong lensing.  相似文献   

A joint model for the emission and absorption properties of damped Lyα absorption systems     

Luke A. Barnes  Martin G. Haehnelt 《Monthly notices of the Royal Astronomical Society》2009,397(1):511-519

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Influence of the water layer upon the depth of ground radar investigations in freshwater reservoirs     

M. L. Vladov  A. M. Pyatilova 《Moscow University Geology Bulletin》2009,64(1):59-62

A number of problems associated with detailed investigation of subsurface geological structure below the bottoms of freshwater reservoirs (rivers, ponds, and lakes) arise during the study of the upper portions of geological sections. The present study is aimed at marginal estimation of the penetrating depth of ground radar investigations in freshwater reservoirs (based on bottom reflections), taking into account the complex nature of conductivity and its dependence upon the frequency under ideal conditions with no noise. The same method can be applied for estimating any given dynamic recording range.  相似文献   

微波消解等离子体发射光谱和石墨炉原子吸收光谱法联合测定土壤中多元素   总被引：6，自引：2，他引：4  

陈江  姚玉鑫  费勇  姚建民  吴杰 《岩矿测试》2009,28(1):25-28

采用密闭式微波消解系统处理土壤样品,电感耦合等离子体发射光谱法或石墨炉原子吸收光谱法测定土壤样品中铜、砷、铅、锌、钴、铬、锰、镍、钒9个元素。分别从消解液的选择、用酸量及样品消解量等方面进行消解条件的优化,确定了一个最适合土壤消解的前处理体系。各元素的检出限为0.16～2.52μg/g,回收率为95.2%～106.6%,精密度为2.03%～9.79%(n=7)。方法简单快速,效率高,劳动强度低,是进行土壤中多元素测定的高效方法。  相似文献