AFS-2202E型原子荧光光度计故障诊断方法

比较全面地分析了AFS-2202E型原子荧光光度计的故障现象及产生原因。从仪器灵敏度下降、空白值升高等光路故障,通信失败及气路自检、空心阴极灯供电、负高压电路、光电倍增管及检测电路等方面故障检修,进样及原子化系统等故障检修方面,归纳出仪器故障的排除方法。     

高氯酸-盐酸体系-火焰原子吸收光谱法测定铅精粉中的银

采用X射线衍射技术(XRD)对水镁石原矿和不同工艺条件生产的出口镁砂产品进行了物相组成分析,水镁石原矿粉中主相Mg(OH)2含量达到85.9%,杂质主要是Mg3Si2(OH)4O5、CaCO3和CaMg(CO3)2;轻烧镁砂中的Mg(OH)2大部分已经分解为MgO,但还有12.3%的Mg(OH)2未分解,并在低温煅烧的情况下生成了微量的新相Mg2SiO4;重烧镁砂中的Mg(OH)2已经完全分解为MgO,杂质主要存在形式是Mg2SiO4和CaCO3,占总量的18.5%。实验结果将成为提高水镁石矿煅烧生产的镁砂品质而改进提纯工艺的参考依据。     

标准加入-原子吸收光谱法测定钢渣中的铁

样品经硝酸-氢氟酸混合酸溶解后,用标准加入-原子吸收光谱法测定钢渣中的铁.实验探讨了钢渣的均匀性等干扰因素对结果的影响,并提出基体高、浓度高的样品稀释倍数过高误差越大,建议采用如旋转燃烧头、选择次灵敏线等降低仪器灵敏度的方法或采用标准加入法.并将标准加入法与X射线荧光光谱、电感耦合等离子体发射光谱、原子吸收光谱直接测定法进行比较,铁的实验结果分别为51.6%、54.2%、46.2%、16.6%,相对标准偏差分别为2.8%、5.3%、2.0%、2.3%.标准加入-原子吸收光谱法用于测定基体高、浓度高的样品是准确可靠的.方法可用于环境类实验室用水剂标准溶液进行钢渣类样品中元素的分析.     

太阳射电尖峰爆与电子回旋共振吸收

本文采用等离子体动力学方法，研究了日冕条件下磁化非相对论热等离子体对太阳射电辐射产生的电子回旋共振吸收，并在辐射频率等于电子回旋谐波频率时求得ｎ≥２谐波吸收率的近似表示式，以及其对等离子体温度，出射角度和谐波数的变化规律，在应用部分，讨论了电子回旋共振吸收对于太阳射电尖峰爆发的影响，认为目前观测到的尖峰爆，大多数高能电子束来自日冕的内层。     

Radiation-induced amorphization of crystalline ice

We study radiation-induced amorphization of crystalline ice, analyzing the results of three decades of experiments with a variety of projectiles, irradiation energy, and ice temperature, finding a similar trend of increasing resistance of amorphization with temperature and inconsistencies in results from different laboratories. We discuss the temperature dependence of amorphization in terms of the ‘thermal spike’ model. We then discuss the common use of the 1.65 μm infrared absorption band of water as a measure of degree of crystallinity, an increasingly common procedure to analyze remote sensing data of astronomical icy bodies. The discussion is based on new, high quality near-infrared reflectance absorption spectra measured between 1.4 and 2.2 μm for amorphous and crystalline ices irradiated with 225 keV protons at 80 K. We found that, after irradiation with 10¹⁵ protons cm⁻², crystalline ice films thinner than the ion range become fully amorphous, and that the infrared absorption spectra show no significant changes upon further irradiation. The complete amorphization suggests that crystalline ice observed in the outer Solar System, including trans-neptunian objects, may results from heat from internal sources or from the impact of icy meteorites or comets.     

The ultraviolet reflectance of Enceladus: Implications for surface composition

The reflectance of Saturn’s moon Enceladus has been measured at far ultraviolet (FUV) wavelengths (115-190 nm) by Cassini’s Ultraviolet Imaging Spectrograph (UVIS). At visible and near infrared (VNIR) wavelengths Enceladus’ reflectance spectrum is very bright, consistent with a surface composed primarily of H₂O ice. At FUV wavelengths, however, Enceladus is surprisingly dark - darker than would be expected for pure water ice. Previous analyses have focused on the VNIR spectrum, comparing it to pure water ice (Cruikshank, D.P., Owen, T.C., Dalle Ore, C., Geballe, T.R., Roush, T.L., de Bergh, C., Sandford, S.A., Poulet, F., Benedix, G.K., Emery, J.P. [2005] Icarus, 175, 268-283) or pure water ice plus a small amount of NH₃ (Emery, J.P., Burr, D.M., Cruikshank, D.P., Brown, R.H., Dalton, J.B. [2005] Astron. Astrophys., 435, 353-362) or NH₃ hydrate (Verbiscer, A.J., Peterson, D.E., Skrutskie, M.F., Cushing, M., Helfenstein, P., Nelson, M.J., Smith, J.D., Wilson, J.C. [2006] Icarus, 182, 211-223). We compare Enceladus’ FUV spectrum to existing laboratory measurements of the reflectance spectra of candidate species, and to spectral models. We find that the low FUV reflectance of Enceladus can be explained by the presence of a small amount of NH₃ and a small amount of a tholin in addition to H₂O ice on the surface. The presence of these three species (H₂O, NH₃, and a tholin) appears to satisfy not only the low FUV reflectance and spectral shape, but also the middle-ultraviolet to visible wavelength brightness and spectral shape. We expect that ammonia in the Enceladus plume is transported across the surface to provide a global coating.     

Computable extensions of generalized fractional kinetic equations in astrophysics

Fractional calculus and special functions have contributed a lot to mathematical physics and its various branches.The great use of mathematical physics in distinguished astrophysical problems has attracted astronomers and physicists to pay more attention to available mathematical tools that can be widely used in solving several problems of astrophysics/physics.In view of the great importance and usefulness of kinetic equations in certain astrophysical problems,the authors derive a generalized fractional kin...     

三维极限平衡法通用形式的建立及应用

在满足边坡整体力平衡、力矩平衡以及边坡微条柱力平衡的条件下,提出了一个综合各种三维极限平衡法的通用形式,该通用形式包含3个表达式。通过这3个表达式利用已有方法的假定条件就可以得到原方法的表达形式,并将他们解析化,不仅大大降低了传统三维极限平衡法的计算工作量,还使得具体实现各种方法时,编程变得更方便,计算更简便,提高了计算效率。最后,通过经典算例,利用通用形式导出的各种方法的解析形式,分析了滑体宽度、滑面强度参数以及滑面剪切力方向对稳定系数的影响。结果表明,该通用形式是正确有效的。     

“金丝砗磲”研究初探

最近,在北京珠宝市场上出现了大量的＂金丝砗磲＂。通过常规宝石学检测和紫外-可见光吸收光谱测试,对其进行了初步研究。结果表明,此种＂金丝砗磲＂并不是砗磲,而是一种海洋腹足纲类海螺贝经染色而成的饰品。该海螺贝呈螺旋状层状构造,可以通过其表面颜色不均、黄色部分不透明、黄色部分无荧光加以鉴别,也可以采用紫外-可见光分光光度计测试加以鉴别。