大功率激电在鄂拉山口寻找隐伏矿体中的应用

鄂拉山口银多金属矿床位于鄂拉山成矿带东南端,第四系覆盖厚,沼泽发育,存在常年冻土层和碎石流,用常规物探在该区找矿效果不显著.后经大功率激电剖面测量,圈出了具一定规模的激电异常带1条,推断为矿异常,经工程验证,发现隐伏银铅锌矿（化）体多条,说明本区采用大功率激电指导找矿效果显著.     

由束流不稳定性直接放大电磁波的弱磁化修正

本文在文［３］的基础上，考虑背景电磁波色散方程的弱磁化修正，在１＜ωｐｅ／Ωｅ＜１０的范围内（主委适用于太阳高日冕、行星际空间及星系射电喷流等），计算了由束流不稳定性直接放大正常模和反常模的增长率。增长率随着频率、ωｐｅ／Ωｅ、电磁波传播角以及非热电子入射角等参数的变化规律，和忽略磁场时的结果与文［３］大体相同，但是反常模的增长，则随着ωｐｅ／Ωｅ的增大而受到明显的抑制，因而在本文参数范围内，束流不稳定性所放大的电磁波以正常模为主，可以解释太阳ＩＩＩ型爆发和星系射电喷流的偏振性质。     

Rapid reversals of polarization in spikes and fast fine structures

We briefly describe the polarization state of the spike groups and fast fine structures superimposed on the 47GB microwave burst of 1991 May 16. At two frequencies 100 MHz apart, namely, 2645 and 2545 MHz, the polarization showed rapid reversals on short time scales of the order of 50 100ms. We think this is probably related to fluctuations on both short time and small spatial scales, in the plasma density and magnetic field of the emission region. Thése oscillations cause the plasma and cyclotron frequency ratio to vary around the value of , thus making the electron cyclotron maser instability growth rate to be dominated alternately by the X mode and the O mode and the polarization state to switch from one sign to the other.     

Brightness,polarization and electron density of the solar corona of 1980 february 16

During the eclipse of 1980 February 16 we photographed the solar corona at an effective wavelength of 6300 å. Using a quadruple camera we also obtained the coronal pictures in polarized light for four Polaroid orientations. We have used these observations to derive the coronal brightness and polarization and from these the electron densities in the corona out to a distance of about 2.5 R⊙ from the centre of the disc. The coronal brightness matches well with that of the corona of 1958 October 12.     

X波段双偏振雷达垂直指向法标定的应用

垂直指向法标定是双偏振雷达的差分反射率因子ZDR标定有效方法的一种,可以订正ZDR测量误差,提高雷达数据的质量。本文基于双发双收模式的X波段双线偏振天气雷达系统,通过分析雷达硬件系统和垂直指向法标定的数据,诊断了观测数值的一些质量问题,初步判断是方位旋转关节损坏而导致ZDR的数值在某一固定区域上出现较大偏差。更换新的方位旋转关节后,对比处理问题前后的垂直指向标定数据证明能有效解决此问题。最后,经过多次试验分析表明,当垂直指向法标定在回波强度为25.5~30.5dB之间的中等范围稳定的层状云降水情况下使用时,其标定的数据能有效订正系统ZDR偏移量。     

基于多源探测资料的一次广州局地强对流垂直结构分析

基于X波段相控阵雷达、S波段双偏振雷达、微波辐射计、风廓线雷达、毫米波云雷达等多源高时空分辨率新型遥感探测资料,对广州后汛期一次局地强对流过程的大气热力、动力及云物理结构变化特征进行了综合分析。结果表明：(1)强对流前8小时前,局地LI、CAPE、SI等对流参数就达到并远远超过了短时强降水的阈值;临近降水大气层结仍向不稳定发展,水汽条件向有利的方向发展;(2)午后局地风形成辐合,上升气流加强,近地层出现弱垂直风切变和低空急流脉动,对强对流的发生发展有一定的指示意义;(3) CINRAD/SA-D雷达CR、DBZM HT、TOPS、VIL等变化与强降水和地面大风的发展有很好的对应关系,同时低层风场观测到阵风锋特征;XPAR-D雷达更高时空分辨率的探测可清晰显示对流发展旺盛阶段的Z_DR弧、K_DP柱、Z_DR柱、V型缺口等特征,为判断雷暴云团的发展程度和预警提供重要信息。     

一种基于改进频域最小均方算法的少模光纤模式复用系统均衡

基于少模光纤的模式复用传输在近些年由于其超过单模光纤非线性香农极限的高传输容量而受到广泛关注,同时偏振复用在不改变光纤链路的情况下,使得系统传输容量翻倍.因此模式复用和偏振复用的结合为下一代超100 Gb／s光网络提供了一种可行的解决方案.然而,该系统的性能受到模式耦合和不同模式的群延时的影响.本文主要讨论基于频域最小均方（LMS）算法的数字均衡技术在少模光纤的偏振模式复用系统中的应用,提出了一种以蝶形复数有限冲激响应滤波器为基本结构的改进频域最小均方算法.该算法通过改进在每一频域柜中的平均功率方程来获得更好的均衡效果.仿真结果表明：采用改进频域LMS算法后在收敛效果上优于传统频域LMS算法,同时提高了系统性能.     

牡丹江和海拉尔台下方地幔间断面结构及推论

利用牡丹江(MDJ)和海拉尔(HIA)台1988-2000年的宽频带三分量数字地震记录,通过地幔间断面产生的P-SV转换波,研究台站下方地幔间断面的分布以及日本海俯冲带对660km间断面的影响.为了提高所得结果的可靠性,采用了线性-偏振滤波方法和修正的N次根倾斜叠加方法来提取P-SV转换波.前一方法通过实验选取适当的光滑平均和提出立体角的约束;对后一方法进行了震源深度校正和间断面倾斜的修正.结果表明,在MDJ和HIA台下方,除在660,410,220和520km深度附近均存有间断面外,在140,350,570,740和1080km深度附近也存在间断面,显示了地幔中径向分层的复杂性;另外,MDJ台下方660-840km之间的间断面结果比HIA台下方的复杂,似有分层结构,可能反映了俯冲带的影响.     

The role of spatial effects in the empirical analysis of regional concentration

 Economists have recently devoted an increasing attention to the issue of spatial concentration of economic activities. However, surprisingly enough, most of the empirical work is still based on the computation of very basic statistical measures in which the geographical characteristics of data play no role. By making use of a series of empirical examples we show that spatial concentration consists of two different features that are rarely kept as separate in the statistical analysis: an a-spatial concept of variability which is invariant to permutations, and the concept of polarization that refers to the geographical position of observations. Received: 8 August 2000 / Accepted: 20 June 2001     

P-wave traveltime and polarization tomography of VSP data

The presence of anisotropy requires that tomographic methods be generalized to account for anisotropy. This generalization allows geological structure to be correctly imaged and allows the anisotropic parameters to be estimated. Use of isotropic inversion for imaging anisotropic structures gives systematic trends in the traveltime and polarization residuals. However, due to the limited directional coverage, the traveltimes along may not be sufficient to study the anisotropic properties of the structure. Polarizations can provide independent information on the structure. Traveltime and polarization inversion are applied to synthetic examples simulating VSP experiments. Transverse isotropy and 1-D structure are assumed. Plots of traveltime and polarization residuals are an important tool to detect the anomalies due to the presence of anisotropy. For receivers located in anisotropic layers, polarization residuals display consistent anomalies of several degrees. The synthetic examples show that even the simple 1-D problem is difficult, when using direct arrivals only. Large a posteriori errors in anisotropic parameters are obtained by traveltime inversion in layers where available incidence angles are less than 45°. Resolution of the tomographic image of VSP data is greatly improved by a combination of traveltime and polarization information. In order to obtain accurate inversion results, the measurement error of polarization data should be kept to within a few degrees.