Effects of solution mining on groundwater quality in the Kazan trona field,Ankara-Turkey: model predictions

Three aquifer systems as deep, middle, and shallow were identified in the Kazan trona ore deposit area. The flow conditions and the interaction between various layers were conceptualized into a site hydrogeological model. Each aquifer system was hydraulically and chemically characterized and represented in a numerical groundwater model. The resulting model has been calibrated under steady-state and transient conditions using available data. The flow model was used in conjunction with a three-dimensional solute transport model to assess the impacts of the pilot well solution mining of the trona deposit on groundwater resources during operation and post-operation periods. The results of operation period indicate that, even under the worse conditions (50 times increase in vertical hydraulic conductivity due to subsidence), ion contribution from the mine area with 118,000 mg/l maximum concentration would be about 58 mg/l into the deep aquifer system. This contribution is about 1.45% of the existing concentration (4,000 mg/l) in the deep aquifer. After 1,000 years of post-operation period, ion contribution from the mine area with maximum 119,000 mg/l concentration would be about 205 mg/l into the deep aquifer under extremely worse conditions. This contribution is about 5–20% of present concentrations in the deep aquifer. Retardation factors, which were not considered during model simulations would decrease the predicted concentrations. It is concluded that pilot well solution mining of the trona deposit would not have significant impact on the quality of groundwater resources in the overlying aquifers.     

碘氟法测铜改进

碘氟法测铜较其他碘量法快速、准确。提出以三价铁沉淀完全时,作为中和溶液调节所需PH值的指示,直观方便,容易掌握。     

质量吸收因子的经验公式

采用非线性最小二乘法拟合获得了生物学、地学和化学上重要的18种元素的质量吸收因子经验公式μ/ρ=cλ3-dλ4-aλ2+bλ+e,其R2比0.9999更精确。并给出了系数及其适用的波长或能量范围,简单讨论了各系数与原子序数Z和原子量之间的关系。     

The contribution of Very Long Baseline Interferometry to ITRF2005

The contribution of the International VLBI Service for Geodesy and Astrometry (IVS) to the ITRF2005 (International Terrestrial Reference Frame 2005) has been computed by the IVS Analysis Coordinator’s office at the Geodetic Institute of the University of Bonn, Germany. For this purpose the IVS Analysis Centres (ACs) provided datum-free normal equation matrices in Solution INdependent EXchange (SINEX) format for each 24 h observing session to be combined on a session-by-session basis by a stacking procedure. In this process, common sets of parameters, transformed to identical reference epochs and a prioris, and especially representative relative weights have been taken into account for each session. In order to assess the quality of the combined IVS files, Earth orientation parameters (EOPs) and scaling factors have been derived from the combined normal equation matrices. The agreement of the EOPs of the combined normal equation matrices with those of the individual ACs in terms of weighted root mean square (WRMS) is in the range of 50–60 μas for the two polar motion components and about 3 μs for UT1−UTC. External comparisons with International GNSS Serive (IGS) polar motion components is at the level of 130–170 μas and 21 μs/day for length of day (LOD). The scale of the terrestrial reference frame realized through the IVS SINEX files agrees with ITRF2000 at the level of 0.2 ppb.     

利用余震震源分布确定主震断层面的方法研究

利用余震震源位置的空间分布,采用Newton-Raphson算法和遗传算法确定主震断层面参数的方法,对仿真数据求出了地震主断层面走向角和倾角,验证了方法的有效性。该方法可以与其他数据结合共同约束主震断层面的参数。     

影响惯性重力波活动规律的动力学因子研究

通过探测发现大气重力波有明显的活动规律:重力波强度在冬、春季强于夏、秋季,在5月和10月发生急剧减弱和加强的转变,无天气过程时晚上比白天强,尤其短周期的重力波,周期为40~80min的重力波平均强度最强,其他较弱。在斜压大气和考虑积云对流加热条件下,运用积云对流参数化、Taylor公式展开等方法,推导出惯性重力波的非线性KdV方程,求出其孤立波解,以此解释以上得出的大气重力波的活动规律:惯性重力波强度随风速垂直切变增大而增大,急流是最重要的惯性重力波波源,是重力波强度在冬、春季强于夏、秋季的主要原因,亚洲急流在5月和10月的北跃和南落,是重力波强度发生急剧变化的原因,急流下方是激发惯性重力波最强的地方。一般情况下,惯性重力波强度随着大气背景流场绝对涡度增大而增大,正涡度对惯性重力波起激发和增强的作用。当惯性重力波向下传播时,波的强度随层结稳定度(N2)增大而增大,由于太阳辐射的作用白天大气层结稳定度比晚上小,这解释了在无天气过程时晚上重力波强度强于白天的原因。惯性重力波强度和波的频率成正比,这解释了周期为40~80 min比周期为140~160 min的重力波强的原因。重力波强度还与非线性积云对流参数常数b及科氏力参数f成正比。     

Inversion and III-Posed Problem Solutions in Atmospheric Remote Sensing

With the swift advances in earth observation,satellite remote sensing and application of atmospheric radiation theory have been developed in the past decades,atmospheric sensing inversion with its algorithms is getting more and more importance.It is known that since a remote sensing equation falls into an integral equation of the first kind,thus leading to the fact that it is ill-posed and particularly the solution is unsteady,tremendous difficulties arise from the retrieval.This paper will present a simple review on the inversion techniques with some necessary remarks,before introducing the successful efforts with respect to such equations and the encouraging solutions achieved in recent decades by researchers of the world.     

Inversion and III-Posed Problem Solutions in Atmospheric Remote Sensing

With the swift advances in earth observation, satellite remote sensing and application of atmospheric radiation theory have been developed in the past decades, atmospheric sensing inversion with its algorithms is getting more and more importance. It is known that since a remote sensing equation falls into an integral equation of the first kind, thus leading to the fact that it is ill-posed and particularly the solution is unsteady, tremendous difficulties arise from the retrieval. This paper will present a simple review on the inversion techniques with some necessary remarks, before in-troducing the successful efforts with respect to such equations and the encouraging solutions achieved in recent dec-ades by researchers of the world.