Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in the Spitzer First Look Survey Field

We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506.     

预啁啾和脉冲沿锐度对光脉冲线性传输的影响

从忽略光纤非线性效应的光脉冲非线性薛定谔方程出发,在光纤正色散区,利用傅立叶变换和反傅立叶变换模拟了不同初始啁啾的二阶与四阶超高斯光脉冲波形随距离的三维演化.分析讨论了脉冲沿锐度以及脉冲预啁啾对脉冲波形演化的综合影响.结果表明:不论脉冲有无预啁啾,光脉冲波形最终都将随着传输距离的增大而展宽.但是负预啁啾将使脉冲波形在脉冲传输的初始阶段发生严重的畸变,即脉冲会分裂成尖峰结构,并且尖峰的数目和能量分布随距离而变.而当预啁啾为正或零时,脉冲前期的畸变很弱.随着脉冲沿锐度的增大,脉冲畸变会加强.此外,在脉冲的前后边缘会出现矮小的峰.整个脉冲波形都是中心对称的.     

黄海在有无潮作用下对“布拉万”不同响应的数值模拟研究

黄海是典型的强潮驱动的陆架浅海。为了研究黄海对台风的响应特点,本文利用区域海洋模式(Regional Ocean Modeling Systems,ROMS)分别模拟了在有潮和无潮作用下黄海对台风"布拉万"的响应过程。结果表明,不管潮存在与否,"布拉万"经过黄海后都引起了海表面降温和流速的近惯性振荡响应,这种响应主要分布于黄海中部较深区域,带通滤波提取的近惯性流速具有垂向第一模态特征。同时,研究发现强背景潮流能显著地影响黄海对"布拉万"的响应过程。主要结论如下:一方面,由于潮的存在,近岸垂向混合均匀的较暖水体与远岸较冷水体之间会形成潮混合温度锋面,"布拉万"过后,暖水发生了明显的离岸扩张,尽管路径右侧的混合层降温更显著,但是左侧即黄海西岸的暖水扩张更明显;另一方面,潮的存在减弱了布拉万产生的近惯性振荡响应,半日潮流在黄海仍然占据主导地位。在混合层中潮流的作用减弱了"布拉万"产生的近惯性能量,但也使其更易穿过跃层传入黄海内部。     

基于舟山外海连续测站的湍混合研究

利用2010年4月3日在舟山外海观测的25hLADCP海流数据与CTD连续观测数据,综合利用Thorpe方法、功率谱分析、交叉谱分析等方法对测站所在海域的小尺度湍混合参数进行估计,分析并讨论了其时空分布特征及影响因子。研究结果表明,上混合层湍流所致的垂向翻转尺度普遍大于下混合层,较大尺度翻转均出现在潮位峰值附近,涨潮时段混合明显大于落潮时段且半日周期,1/4周期显著。该站点存在明显的"上强下弱"双密度跃层现象,湍动能耗散率、湍混合率也呈现出"表强底弱"特征。弱跃层中近惯性频率的内波和近半日潮频率的内潮信号最为显著,而强跃层中则是高频内波和近半日潮频率的内潮信号明显,上下跃层及其之间伴有间歇性强湍流发生。上混合层平均的湍混合对风应力的响应要快于对海流的响应,底应力是下混合层水体湍混合的重要因子。     

一次江淮强暴雨过程的湿有效能量及其收支特征

利用高分辨率的WRF模式模拟结果,采用基于格点的湿有效能量计算方案,对一次江淮梅雨期强暴雨发生发展过程中湿有效能量的时空演变特征进行分析,并从定性和定量的角度探讨了能量方程转换项、平流项和垂直输送项对强暴雨过程中湿有效能量的输送和积聚作用。结果表明,强暴雨过程中湿有效能量的时空特征与强暴雨发生发展具有良好的对应关系,对流层低层800 h Pa湿有效能量40×104J·h Pa-1·m-2的等值线范围和该等值线伸展至500 h Pa附近可作为判断强暴雨发生的必要条件。暴雨发生前2~3 h的能量快速积聚及其对暴雨区移向的引导,对强暴雨预报具有良好的指示作用。湿有效能量的水平和垂直输送及转换确保了能量的积聚和对流层中层能量的增加,为强暴雨的发生和维持提供了充足的能量。     

2011年盛夏石家庄一次短时暴雨分析

2011年7月26日石家庄市出现一次暴雨冰雹天气,其特点是500 h Pa及以上高空强冷空气导致高空形势在12 h内发生剧变,短波槽快速南下,致使探空观测和数值预报失灵。本文对其他监测资料进行分析,发现这种剧烈变化的天气有明显特征:卫星云图上河套北部逗点云系尾长而粗壮,有向南发展趋势,云系后部的暗区表明干冷空气侵入,与低层暖湿空气形成对流云,尾部断裂表明冷空气加速南下。单站要素变化显示,石家庄地面假相当位温比正常值高了8℃,出现异常不稳定能量。强对流天气发生在假相当位温密集带内,能量中心假相当位温最高达到90℃以上,100 km内假相当位温温差超过25℃,最大降雨出现在假相当位温密集带内。雷达回波呈西南—东北带状排列,前部最大强度为65 d BZ,强回波前形成阵风锋,正负最大速度均超过20 m/s,飑线自西向东移动,它的移向和发展程度决定降雨和冰雹的路径和强度。石家庄市区风向转变和形成地面辐合线分别较降水起始时间提前21 min和30 min。     

Rainfall effect on wind waves and the turbulence beneath air-sea interface

Rainfall effects on wind waves and turbulence are investigated through the laboratory experiments in a large wind-wave tank. It is found that the wind waves are damped as a whole at low wind speeds, but are enhanced at high wind speeds. This dual effect of rain on the wind waves increases with the increase of rain rate, while the influence of rainfall-area length is not observable. At the low wind speed, the corresponding turbulence in terms of the turbulent kinetic energy （TKE） dissipation rate is significantly enhanced by rain- fall as the waves are damped severely. At the high wind speed, the augment of the TKE dissipation rate is suppressed while the wind waves are enhanced simultaneously. In the field, however, rainfall usually hin- ders the development of waves. In order to explain this contradiction of rainfall effect on waves, a possibility about energy transfer from turbulence to waves in case of the spectral peak of waves overlapping the inertial subrange of turbulence is assumed. It can be applied to interpret the damping phenomenon of gas trans- fer velocity in the laboratory experiments, and the variation of the TKE dissipation rates near sea surface compared with the law of wall.     

高精度初至自动拾取综合方法研究

初至拾取是地震信号处理的关键环节,其精度和效率是资料处理的重要指标。针对常规地震资料,特别是浅海地震资料信噪比相对较高的情况,探讨了改进的能量比法,来确保拾取精度的前提下,实现过程的自动化。在传统能量比方法的基础上,研究了两种改进方法:利用边界检测和稳定因子解决"起跳不干脆"现象,利用多时窗识别折射波与直达波交混处的初至;利用奇异值的处理方法和可变时移量相位推算技术,解决精度和效率问题。模型和实际资料处理结果表明:综合时窗、相位、能量等多种因素,改进后的方法针对常规地震资料具有拾取准确、计算速度快、自动化程度高等优势。     

Review on physical models of lunar brightness temperature

Brightness temperature is a main index to reflect the energy of microwave radiation of an object. Using lunar brightness temperature data, physical properties of lunar regolith, such as thickness, heat flow and dielectric permittivity, could be interpreted. There are two methods to study brightness temperature distribution of the moon: the first is used to measure lunar brightness temperature by radio observation or spaceborne microwave radiometers, and the second is used to simulate calculation by the physical model. On the basis of the measurements of lunar brightness temperature in the history, this study analyzed the main physical model of lunar brightness temperature, also including its theory and influence factors. The authors concluded that surface and subsurface temperatures of the moon, dielectric properties and layered structure of lunar regolith were the main factors affecting the global brightness temperature of the moon. These factors should be quantified in detail in the future research.