Synthesis and Characterization of an Extractant [Bmim]PF_6 for Lithium Ion

正With the rapid increasing demand of metal lithium and its compounds in science and technology,studies on lithium recovery though lithium ion extraction from salt lake brines are blooming bacause more than 60 percent of     

对流层折射对超视距雷达信号定位的影响

超视距雷达信号的精确定位对于提高超视距探测能力有十分重要的意义。但由于对流层中的折射效应，定位系统所测目标的仰角、距离等参量均存在一定的折射误差。主要分析对流层的折射效应对超视距雷达信号定位的影响，并且给出相应的折射误差图（仰角误差和距离误差）；此外，还针对3种不同的大气折射指数模型进行比较，得出折射误差对比图。     

Pulsar investigation using interstellar scintillation

We discuss the resolution of pulsar magnetospheres using interstellar scintillation. The two-dimensional spatial structure of pulsar emission zones can be obtained from analysis of diffractive scintillations at low frequencies. Based on refractive and diffractive scintillation of pulsars we can also reconstruct the distribution of turbulent plasma along the line of sight, and using this analysis a new approach to pulsar distance estimation can be made. This revised version was published online in July 2006 with corrections to the Cover Date.     

双成分星际介质的折射闪烁

本文用比较严格的理论讨论了由连续介质和散射薄屏组成的星际介质对河外射电源的折射闪烁．对折射闪烁引起的流量变化的结构函数Ｄ（τ）（τ为迟后时间）的计算表明，结构函数的幂律部份的指数Ｐ（Ｄ（τ）（∝τＰ）依赖于上述两个成份的相对散射强度，即在连续介质散射为主的情况下；而在薄屏散射为主的情况下；若两个成份的散射可相比较时，１＜Ｐ＜２．因此本模型可以用于解释在河外射电源和脉冲星中观测到的折射闪烁的结构函数具有不同幂指数的情形，特别是Ｐ～１．５的情形．     

Propagation of Extremely Low Frequency Waves Through the Ionosphere

The propagation features of extremely low frequency electromagnetic waves through the multicomponent ionospheric plasma are studied. It is shown that at relatively lower frequencies refractive index for right hand mode is higher than the left-hand mode, which is reversed at higher frequencies. The thermal temperature of plasma particle causes decrease in phase and group velocities of both right and left-hand modes. The crossover frequencies for different plasma models are computed and variation with ion concentration and thermal velocity is studied. Explicit expression for group velocity and travel time has been derived and studied numerically. Finally, we have presented simulation of the ion whistler spectrograms for Hydrogen, Helium and Oxygen ions present in the ionospheric plasma. The results are compared with the experimentally detected hydrogen and helium ion whistlers. The importance of the present study in the exploration of ionospheric plasma is illustrated.     

Measuring the sizes of stars

The Chatterton Astronomy Department aims to apply interferometers with very high resolving power to optical astronomy. The programme of the stellar intensity interferometer at Narrabri Observatory was completed in 1972 and since then the work has been directed towards building a more sensitive instrument with higher resolving power. As a first step a much larger intensity interferometer was designed but was not built because it was large, expensive and not as sensitive as desired. Efforts are now being made to design a more sensitive and cheaper instrument. A version of Michelson’s stellar interferometer is being built using modern techniques. It is hoped that it will reach stars of magnitude +8 and will work reliably in the presence of atmospheric scintillation. It is expected to cost considerably less than an intensity interferometer of comparable performance. The pilot model of this new instrument is almost complete and should be ready for test in 1984. Text of an Academy Lecture delivered at the Raman Research Institute, Bangalore on January 27, 1984.     

Nouvelles données sur le téphra de Sarliève et le téphra CF7, marqueurs chrono-stratigraphiques de Grande Limagne (Massif central,France)

A trachytic tephra, discovered in the ancient lake of Sarliève, ‘Grande Limagne’, has been dated using the thermoluminescence technique. The obtained age, 16±4 ka ($\text{2}\text{σ}$), is older than that of the trachytic volcanoes of the Cha??ne des Puys, the ashes of which have already been locally recognised in the region. Its analysis confirms its originality. In the course of the comparisons made to search for its spring, it appears that the wide-dispersion tephra CF7, beforehand correlated by hypothesis to the Puy de Clierzou, probably originates from the Kilian crater or the Puy de Vasset. To cite this article: D. Miallier et al., C. R. Geoscience 336 (2004).     

风廓线雷达在一次短时暴雨过程中的应用

利用2014年8月24日天津地区一次短时暴雨天气的3部风廓线雷达资料和降水实况资料,对比分析降水发生、维持和消亡期间风廓线雷达资料的变化特征,以探讨风廓线雷达对降水天气的监测能力。结果表明:1)风廓线雷达不仅能够反映大气层结上冷下暖的结构,并且能够探测到切变线的存在,对风的垂直结构有较强的探测能力。2)当降水出现时,垂直速度和大气折射率结构常数明显增大。4 m·s~(-1)的垂直速度出现和消失时刻,对应降水的开始和结束时刻;降水期间,4000 m高度以下的垂直速度越大降水越强。西青、静海站的折射率结构常数与降水强度之间有很好的对应关系,但不同地区的大气折射率结构常数值对降水强度的指示标准并不一致。3)在降水最强阶段,风廓线雷达数据获取率明显下降,因此低的数据获取率对强降水有一定的指示意义。     

测氡仪标准仪器校准法的可行性研究

针对目前台站测氡仪校准困难的问题,提出标准仪器校准法,并将其与RN-FD循环式氡气固体源进行对比,同时利用台站应用最为广泛的RN-150小型氡气固体源验证该方法的可行性。结果表明,利用RN-150小型氡气固体源及AlphaGUARD P2000F标准仪器分别对FD-125测氡仪3个闪烁室进行校准后得到的校准系数相对误差分别为0.2%、3.4%、2.8%,均达到目前地震监测中氡观测的技术要求,进一步验证了测氡仪标准仪器校准法的可行性。     

利用GPS三频数据计算电离层垂直总电子含量变化率

研究了通过采样间隔为1 s的GPS三频载波相位观测数据计算1 Hz电离层垂直总电子含量变化率（RVTEC）的方法,推导了直接采用双频载波相位观测量计算RVTEC的公式,对一般空间环境与电离层活动剧烈两种条件下L1L2、L1L5、L2L5三种载波相位组合计算的RVTEC进行了一致性分析,给出了通过三频载波相位观测数据计算电离层RVTEC的修正方法,比较了X射线太阳耀斑期间RVTEC与由传统方法计算的总电子含量变化率（ROT）响应,在双星串飞编队测高模式下对计算方法进行了应用.结果表明,L1L2、L1L5两种组合之间的一致性较好,由L1L2、L1L5组合计算的RVTEC的中误差约为0.004 TECu/s,RVTEC较ROT更能体现TEC变化的细节,在双星串飞编队测高模式下海面高梯度的计算中,电离层延迟之差可以忽略.