基于微波链路的路径雨强反演方法及实验研究

从大气气体吸收衰减模型出发, 基于微波雨衰特性和雨滴谱统计资料建立了微波链路降雨有效衰减的修正模型和视距微波链路的降雨反演模型. 设计并搭建一条视距微波链路测雨实验系统, 利用降雨反演模型反演了路径平均降雨强度, 并与雨滴谱仪进行了同步对比. 观测结果表明, 视距微波链路降雨反演模型的反演雨强与雨滴谱仪测量结果的相关系数大多高于0.6, 最高可达0.9647; 累积降雨量的绝对误差大多在0.5 mm以内, 最小偏差仅有0.0827 mm; 相对偏差大部分在15%以内, 最小相对误差为3.3415%. 实验结果验证了微波链路反演降雨的有效性和准确性.     

基于非球形雨衰模型的微波链路雨强反演方法

以T矩阵理论、Gamma谱分布为理论基础,基于Pruppacher-Beard降雨粒子模型,对OTT雨滴谱仪的Gamma谱参数历史资料与降雨强度值进行非线性拟合得到具有实地谱分布的幂律系数,建立适合于本地区的雨衰模型,提出了基于非球形雨衰模型的微波链路雨强反演方法,分析了温度对模型幂律系数的影响,并开展了15—20 GHz频段的视距微波链路与地面雨滴谱仪的同步观测降雨实验.实验结果表明:反演雨强的相关系数全部高于0.6,最高达到了0.96,RMSE最小值为0.79,累积降雨量的绝对偏差在2.47 mm以内,最小偏差仅为0.28 mm,相对误差低于1.84%.实验结果验证了基于非球形雨衰模型的微波链路雨强反演方法的有效性、准确性和适用性,对于进一步提高微波链路反演降雨精度、改善降水监测效果具有重要意义.     

基于支持向量机的微波链路雨强反演方法

为提高微波链路雨致衰减反演雨强精度, 在Mie散射理论、气体吸收衰减模型以及Gamma雨滴谱分布的基础上, 将支持向量机引入到微波链路测量降水中, 提出了基于支持向量机的微波链路雨强反演方法, 并开展了15–20 GHz频段的视距微波链路与地面雨滴谱仪的同步观测降雨实验. 实验结果表明, 基于支持向量机的微波链路雨强反演模型的反演雨强与实测雨强的相关系数全部高于0.6, 最高达到0.9674; 雨强的均方根误差最小值为0.5780 mm/h, 累积降雨量的绝对最小误差仅为0.0080 mm; 相对偏差大部分在10%以内, 最小偏差为0.7425%. 实验结果验证了基于支持向量机的微波链路雨强反演方法的有效性、准确性和适用性, 对于进一步提高微波链路反演降雨精度、改善降水监测效果具有重要意义.     

用原子轨道强耦合方法研究H(1s)+H(1s)碰撞的反应截面

采用单电子的双中心原子轨道强耦合方法,研究了1-100 ke VH(1s)+H(1s)碰撞体系的激发、俘获和失去电子总截面,并分别与前人的理论结果和实验结果进行了比较.研究表明,采用双中心原子轨道强耦合方法得到的H(1s)+H(1s)体系激发到H(2s)过程和失去电子过程的截面与实验符合很好.     

用原子轨道强耦合方法研究H(1s)+H(2s)碰撞的反应截面

采用单电子的双中心原子轨道强耦合方法,计算了H(1s)+H(2s)碰撞体系H(2s)失去电子过程的总截面,并与前人的实验结果进行了比较.研究表明,采用双中心原子轨道强耦合方法得到的H(1s)+H(2s)体系H(2s)失去电子过程的截面与实验比较符合.同时,还给出了H(1s)+H(2s)碰撞体系H(2s)电离过程、H(1s)俘获电子过程和H(2s)退激发到H(1s)过程的理论截面.     

用原子轨道强耦合方法研究H(1s) + H(2s)碰撞的反应截面

采用单电子的双中心原子轨道强耦合方法,研究了1-100 碰撞体系的激发、俘获和失去电子总截面,并分别与前人的理论结果和实验结果进行了比较。研究表明,采用双中心原子轨道强耦合方法得到的 体系激发到 过程和失去电子过程的截面与实验符合很好。     

B$lt;sub$gt;$lt;i$gt;n$lt;/i$gt;$lt;/sub$gt;Y($lt;i$gt;n$lt;/i$gt;=1–11)团簇的结构和电子性质

利用密度泛函理论TPSSh方法对B采用6-311+G(d), 对Y采用Lanl2dz相对论有效势基组, 研究了B_nY (n=1–11)团簇的平均结合能、二阶能量差分、最高分子占据轨道和最低空轨道之间的能级间隙、极化率和第一静态超极化率等物理化学性质. 结果表明, 随着尺寸的增大, B_nY (n=1–11)团簇的最低能量结构从平面逐步演变为立体结构. 随硼原子数n的增加, 团簇的平均结合能表明了较好的热力学稳定性, 有利于Y掺杂B团簇形成较大的块体材料.二阶能量差分表明基态B₃Y, B₅Y和B₇Y团簇较相邻团簇稳定. 能隙表明了基态B₃Y, B₅Y, B₇Y和B₉Y的化学稳定性较高. 综合说明B_nY (n=1–11)硼团簇中, 基态B₃Y, B₅Y和B₇Y具有较好的稳定性. 极化率表明基态B_nY团簇的电子结构随B原子的增加趋于紧凑, 第一静态超极化率表明基态B₅Y, B₄Y, B₃Y和B₆Y平面结构的团簇具有明显的非线性光学性质, 为寻找性能优异的非线性光学材料提供了一定的参考. 关键词： 密度泛函TPSSh方法 nY (n=1–')" href="#">B_nY (n=1– 11)团簇 几何结构 电子性质     

Ti$lt;sub$gt;2$lt;/sub$gt;B$lt;sub$gt;$lt;i$gt;n$lt;/i$gt;$lt;/sub$gt;($lt;i$gt;n$lt;/i$gt;=1–10)团簇的结构与稳定性:基于从头算的研究

采用密度泛函理论中的B3LYP方法, 结合从头算的CCSD(T)方法对Ti₂B_n(n=1–10)团簇的稳定性和电子性质进行了研究. 发现两个Ti原子的掺杂导致B_n团簇结构发生了根本性变化. 随着n的增大, Ti₂B_n团簇结构生长非常规律. 所有的最稳定结构都可看成双锥结构, 并且两个Ti原子处在双锥结构的锥顶. 根据二阶差分能量分析, 得出Ti₂B_n(n=1–10)团簇的幻数是6, 7和8. 进一步分析了团簇的Ti原子解离能、B原子解离能以及团簇的电子亲和势和电离势. 这些能量分析表明Ti₂B₆团簇既有良好的热力学稳定性, 又有良好的动力学稳定性. 应用前线轨道理论, 对Ti原子与B₆之间的成键进行了分析, 了解其稳定性的根源. 关键词： 2B_n团簇')" href="#">Ti₂B_n团簇 稳定性 从头计算 电子结构     

Real-time frequency transfer system over ground-to-satellite link based on carrier-phase compensation at 10-16 level

We demonstrate a novel and stable frequency transfer scheme over ground-to-satellite link based on real-time carrier-phase detection and compensation. We performed a zero-baseline measurement with the designed system, an uninterrupted frequency standard signal is recovered in the reception station without additional post-correction of delay error caused in the route, which is because the phase error of the entire route is tracked and compensated continuously in real-time. To achieve this goal, we employed two carriers in the system and the differential signal is transferred in order to eliminate the instability results from the local oscillator at the satellite transponder as well as the common-mode noise induced in the transfer route and microwave components. The stability of 3×10^-16 with an integration time of 1 day was achieved and the time fluctuation during one day was measured to be about ±20 ps. Error sources and possible solutions are discussed. Our zero-baseline method shows a promising result for real-time satellite-based time and frequency transfer and deserves further research to find whether it works between long-baseline stations.     

Experimental determination and comparison of rain attenuation in free space optic link operating at 532 nm and 655 nm wavelength

The demand for high data rate, security and reliable communication is driving the development of free space optic communication (FSO) technology. The atmospheric effects such as scintillation, absorption and scattering severely affect the availability and range of the FSO system. The atmospheric rain absorbs and scatters the laser beam energy resulting in attenuation of the propagating signal. Initial development of FSO technology primarily used wavelength from infrared spectrum. In the recent years, the interest in visible light carrier for FSO applications is consistently increasing. In this paper, the effect of rain over two optical wavelengths from the visible spectrum i.e. 532 nm and 655 nm has been experimentally evaluated and results for the specific rain attenuation at 532 nm and 655 nm wavelengths have been compared.     

基于临界慢化现象的气候突变前兆信号的初步研究

近年来,临界慢化现象在揭示复杂动力系统是否趋于临界性灾变方面展示了重要潜力.基于临界慢化的理念,研究了气候突变的早期预警信号.针对20世纪70年代末80年代初的气候突变,对全国月平均温度资料和太平洋年代际振荡(PDO)指数进行分析,分别计算了表征临界慢化现象的方差和自相关系数.结果表明,气候发生突变前,全国月平均温度和PDO指数都存在明显的临界慢化现象,这表明临界慢化现象可能是气候突变发生前的一个早期信号.将临界慢化理论用于气候突变前兆信号的研究,对深入认识气候突变和捕捉气候突变前兆信号都具有重要的现实意义和科学价值.     

Understanding hydrogen plasma processes based on the diagnostic results of 2.45 GHz ECRIS at Peking University

Optical emission spectroscopy(OES), as a simple in situ method without disturbing the plasma, has been performed for the plasma diagnosis of a 2.45 GHz permanent magnet electron cyclotron resonance(PMECR) ion source at Peking University(PKU). A spectrum measurement platform has been set up with the quartz-chamber electron cyclotron resonance(ECR) ion source [Patent Number: ZL 201110026605.4] and experiments were carried out recently. The electron temperature and electron density inside the ECR plasma chamber have been measured with the method of line intensity ratio of noble gas. Hydrogen plasma processes inside the discharge chamber are discussed based on the diagnostic results. What is more, the superiority of the method of line intensity ratio of noble gas is indicated with a comparison to line intensity ratio of hydrogen. Details will be presented in this paper.     

新显色试剂1-(4-磺基苯)-3-(2-吡啶)-三氮烯的合成及其与镉(Ⅱ)的显色反应

合成了一种新三氮烯类显色剂1-(4-磺基苯)-3-(2-吡啶)-三氮烯(简称SPPT),并研究了在Triton X-100存在下,于pH为9.18的Na2B4O7-NaOH缓冲溶液中与镉的显色反应.结果表明,试剂与镉生成橙红色配合物.方法用于废水中微量镉的测定,结果令人满意.     

The effect of preparation time and aeration rate on the properties of bulk micro-nanobubble water using hydrodynamic cavitation

Fundamental research on bulk micro-nanobubbles (BMNBs) has grown rapidly due to the demand for their industrial applications and potential role in interfacial sciences. This work focuses on examining properties of such bubbles, including the number, concentration, zeta potential, and surface tension in water. For this purpose, BMNBs were generated by the hydrodynamic cavitation (HC) mechanism. Distilled water and air in the experiments were the liquid and gas phases, respectively. The characterization of bulk microbubbles (BMBs) and bulk nanobubbles (BNBs) were performed through focused beam reflectance measurement (FBRM) and nanoparticle tracking analysis (NTA) techniques, respectively. Zeta potential and surface tension of aqueous solutions were measured at different time and aeration rates. The results showed that aeration rate and preparation time had an important role in the properties of BNBs (concentration, bubble size, and surface charge) and BMBs (number, and bubble size). The instability of BMBs led to the rapid changes in the dissolved oxygen (DO) content in the water. The number of BMBs decreased when preparation time and aeration rate increased, but their size remained constant. By enhancing the preparation time and aeration rate, the concentration of BNBs improved first and then reduced. Additionally, the surface tension of an aqueous solution containing BNBs was significantly lower than that of pure water.     

The adsorption geometry of the (2 × 1)-2O oxygen phase formed on the Co(10 0) surface

The bond geometry of the (2 × 1)-2O-p2mg overlayer on Co(10 0) was determined by analyzing low-energy electron diffraction (LEED) intensity data. Oxygen occupies the three-fold coordinated hcp site along the densely packed rows on the unreconstructed surface. The O atoms are attached to two atoms in the first Co layer and to one Co atom in the second layer. The strong interaction between O and Co is indicated by the bond lengths of 1.83 ± 0.10 Å and 1.99 ± 0.10 Å to the top-layer Co and the Co atoms in the second layer, respectively. The most striking result of our work is that oxygen adsorption causes a marked expansion (by 25%) of the first Co layer spacing (0.90 Å) with respect to the bulk value of 0.72 Å. This strong expansion might offer diffusion channels for O atoms to penetrate further into the subsurface region.