中国东部夏季降水与同期东亚副热带急流年代际异常的关系

利用中国738个台站的降水观测资料和NCEP/NCAR再分析资料, 分析了我国降水和200 hPa东亚副热带西风急流轴的年代际变化特征, 揭示了东亚副热带西风急流位置的南北移动与我国长江流域和华北降水异常之间的联系。结果表明, 我国东部地区夏季（7、 8月）降水异常主要表现为长江中下游地区多（少）雨, 华北及华南地区少（多）雨, 20世纪70年代末80年代初是这种异常分布型发生转折的时间。与此同时, 东亚高空副热带急流轴位置从70年代末开始逐渐偏南, 急流轴位置的变动将引起对流层低层水汽辐合区和高层散度分布以及垂直环流相应的变化, 进而引起降水区域的变化。相关分析发现, 当急流位置偏南时, 25°~35°N西风增强, 42°~50°N西风减弱, 华北夏季降水减少, 长江中下游地区夏季降水增多; 反之, 当急流位置偏北时, 华北夏季降水增多, 长江中下游地区夏季降水减少。与70年代末开始的我国东部地区急流轴位置逐渐南移相对应, 华北地区夏季降水呈现逐渐减少、 长江中下游地区夏季降水呈现逐渐增多的变化趋势。分析低层水汽通量和高层的散度分布以及垂直环流的差异发现, 1980年以来华北地区对流层中低层水汽通量辐合减弱, 水汽供应减少, 垂直上升运动减弱, 造成了华北夏季降水减少, 而长江中下游地区水汽通量辐合增加, 水汽供应增多, 垂直上升运动增强, 导致该地区降水增加。     

西太平洋副热带高压对华北地区降水蒸发差的影响

采用小波相关和交叉小波变换等方法, 分析了西太平洋副热带高压脊线和北界位置变化对华北地区降水蒸发差的影响。结果表明, 2000年以来华北区南部的水资源短缺问题有所缓解, 但以北京为中心的华北区东北部仍处于持续缺水期; 华北地区降水蒸发差与副热带高压脊线及北界位置变化相关密切, 存在年际和年代际尺度的显著相关振荡, 与副热带高压脊线的年代际尺度相关凝聚性最强; 时域中年际尺度相关存在局部化特征, 年代际尺度相关具有阶段性。分析认为, 2000年以来副热带高压脊线和北界位置偏北并维持反气旋型环流, 有利于水汽向华北输送, 使得华北降水增多, 是近年来华北中南部降水蒸发差增大的主要原因; 而东亚季风减弱不利于西南气流的水汽输送, 以及蒙古高原显著增暖导致蒸发增大等因素, 使得华北东北部仍处于持续缺水期。     

暗物质粒子探测器触发逻辑测试系统的设计和实现?

作为暗物质粒子探测器(DAMPE, Dark Matter Particle Explorer)的一部分,触发系统主要用于判选所需探测的目标粒子(高能电子和伽玛射线)事例,剔除非目标粒子事例。触发系统由触发探测器和触发判选逻辑电路组成。介绍了触发地检测试系统和宇宙线触发系统的设计和功能实现。触发地检系统实现了对触发判选逻辑电路的电子学验证;另外,配合宇宙线触发系统对部分触发逻辑和触发效率进行了测试。主要介绍了触发系统的测试方法和一些初步测试结果。     

Double-detonation model of type Ia supernovae with a variable helium layer ignition mass

Although Type Ia supernovae(SNe Ia) play an important role in the study of cosmology, their progenitors are still poorly understood. Thermonuclear explosions from the helium double-detonation sub-Chandrasekhar mass model have been considered as an alternative method for producing SNe Ia. By adopting the assumption that a double detonation occurs when a He layer with a critical ignition mass accumulates on the surface of a carbon–oxygen white dwarf(CO WD), we perform detailed binary evolution calculations for the He double-detonation model, in which a He layer from a He star accumulates on a CO WD. According to these calculations, we obtain the initial parameter spaces for SNe Ia in the orbital period and secondary mass plane for various initial WD masses. We implement these results into a detailed binary population synthesis approach to calculate SN Ia birthrates and delay times. From this model,the SN Ia birthrate in our Galaxy is ～0.4- 1.6 × 10-3yr-1. This indicates that the double-detonation model only produces part of the SNe Ia. The delay times from this model are ～ 70- 710 Myr, which contribute to the young population of SNe Ia in the observations. We found that the CO WD + sdB star system CD-30 11223 could produce an SN Ia via the double-detonation model in its future evolution.     

近30年我国高空风速变化趋势分析

1980-2006年间采用全国119个探空站14个等压面的月平均风速资料,分析了我国高空对流层和平流层下层风速变化的时间和空间特征,并和同期地面风速变化进行了对比.结果表明,我国近27年对流层中下层和对流层上层风速呈下降趋势,年平均风速线性变化速率分别为-0.10 m·s-1·(10a)-1和-0.17 m·s-1·(10a)-1,均未通过0.05显著性水平检验;平流层下层全国年平均风速呈上升趋势,上升速率为0.24 m·s-1·(10a)-1,亦未通过O.05显著性水平检验.同期全国地面风速则呈现更显著的降低趋势,年平均风速线性变化速率为-0.16 m·s-1·(10a)-1,通过了0.05显著性水平检验.我国地面气象站记录的平均风速减弱可能受到大尺度大气环流变化的影响,更可能与台站附近观测环境变化和城市化等人为因素影响有密切关系.     

Solving the G-dwarf problem with a three-component model of the chemical evolution of the Galaxy

A three-component chemical evolution model of the Galaxy is presented, which we believe will cast a new light on the G-dwarf problem. The model is based on a scenario of the Galaxy consisting of three major evolutionary phases: halo, thick disk and thin disk, separated by two short interludes of rapid collapse. The evolution of different stellar populations are treated separately, the combination of which yields an overall metallicity distribution function for the solar neighbourhood. We tested three different models using the same set of basic equations: the “prompt initial enrichment” (PIE) model, the “proportional yield” (PPY) model and the “collapse” (CLP) model. Best-fit parameters are derived. The results show that the different populations have remarkably different IMFs, while mass exchange has only minimally affected the chemical evolution in the solar vicinity, so that the solar vicinity can be regarded as a closed system, at least in the late stage of the Galactic evolution.     

晚型星HR5553,εEri和70 Oph的活动性,金属丰度和磁场的测定

对１９９５年１１月和１９９６年３、４月间观测获得的ＨＲ５５５３、７０Ｏｐｈ和εＥｒｉ给出了高分辨率,高信噪比的阶梯光栅光谱资料。确定了这３颗晚型活动星的大气参数,采用谱线细致分析方法求出了铁、锂、钙、钪、钛、钒、铬、锰、钴、镍、钇、锆和钡１３种金属元素的丰度。采用多重线统计方法测定了这３颗晚型活动星的磁场和磁场覆盖因子。     

激光参量对CPT铷原子钟稳定度影响的数值分析

为具体分析激光参量对相干布居囚禁(CPT)原子钟的稳定度性能的影响,在(-型三能级原子系统模型的基础上,采用半经典密度矩阵方法,数值模拟计算了不同激光参量对CPT铷原子钟共振谱线信号的影响,并给出了比较分析.结果显示:两束激光强度的不对称对CPT钟信号强度的影响很大,而激光频率失谐对CPT钟信号影响较小;此外,当激光强度不对称与频率失谐同时存在时,荧光信号谱出现不对称,微波辐射信号发生频移.     

基于伪距测量的钟差计算模型

基于伪距和钟差定义,讨论了无线电时间比对的基本原理。在此基础上,详细推导了地心非旋转坐标系中一般意义下基于伪码测距模式的钟差计算模型,并通过坐标变换,给出了地固系中的实用计算模型。对地回系计算模型的进一步分析表明：卫星在地固系运动速度引起的改正项与sagnac效应项是完全不同的两项改正;对于GEO卫星,sagnac效应项最大约为200ns,其地固系运动速度引起的改正约为1ns;而对于MEO卫星,sagnac效应项最大为120ns,其地固系运动速度引起的改正约为1200ns。     

XUV Photometer System (XPS): Improved Solar Irradiance Algorithm Using CHIANTI Spectral Models

Solar soft X-ray (XUV) radiation is highly variable on all time scales and strongly affects Earth’s ionosphere and upper atmosphere; consequently, the solar XUV irradiance is important for atmospheric studies and for space weather applications. Although there have been several recent measurements of the solar XUV irradiance, detailed understanding of the solar XUV irradiance, especially its variability during flares, has been hampered by the broad bands measured in the XUV range. In particular, the simple conversion of the XUV photometer signal into irradiance, in which a static solar spectrum is assumed, overestimates the flare variations by more than a factor of two as compared to the atmospheric response to the flares. To address this deficiency in the simple conversion, an improved algorithm using CHIANTI spectral models has been developed to process the XUV Photometer System (XPS) measurements with its broadband photometers. Model spectra representative of quiet Sun, active region, and flares are combined to match the signals from the XPS and produce spectra from 0.1 to 40 nm in 0.1-nm intervals for the XPS Level 4 data product. The two XPS instruments are aboard NASA’s Solar Radiation and Climate Experiment (SORCE) and Thermosphere, Ionosphere, Mesosphere, Energetics, and Dynamics (TIMED) satellites. In addition, the XPS responsivities have been updated for the latest XPS data processing version. The new XPS results are consistent with daily variations from the previous simple conversion technique used for XPS and are also consistent with spectral measurements made at wavelengths longer than 27 nm. Most importantly, the XPS flare variations are reduced by factors of 2 – 4 at wavelengths shorter than 14 nm and are more consistent, for the first time, with atmospheric response to solar flares. Along with the details of the new XPS algorithm, several comparisons to dayglow and photoelectron measurements and model results are also presented to help verify the accuracy of the new XUV irradiance spectra.