AMSR-E微波极化指数与MODIS植被指数关系研究     

毛克彪  唐华俊  周清波  陈仲新  陈佑启  赵登忠 《国土资源遥感》2007,18(1):27-31

首先，利用辐射传输方程对微波极化指数（MPI，Microwave Polarization Index)进行推导，以AMSR-E像元经纬度为控制条件，采集与之对应的MODIS植被指数（ LAI/NDVI），并将其平均值作为AMSR-E对应像元的值； 然后，对AMSR-E微波极化指数与LAI/NDVI进行相关分析。结果表明，MPI与LAI/NDVI之间存在着指数关系，而且频率越低，相关性越好。  相似文献   

中国大陆及邻区海域地壳上地幔各向异性研究   总被引：11，自引：6，他引：11       下载免费PDF全文

彭艳菊  黄忠贤  苏伟  郑月军 《地球物理学报》2007,50(3):752-759

利用分别由Love波和Rayleigh波得到的S波速度结构的差值（VSH-VSV）对中国大陆及邻区海域（70°E～145°E，15°N～55°N）地壳上地幔中的偏振各向异性进行研究.初步研究结果表明，各向异性在空间分布上存在不均匀性：（1）在小于150 km的深度范围内，VSH>VSV的各向异性体占主导地位，反映出在地球的浅部岩石圈内的水平应力作用及软流圈顶部物质的水平向流动对各向异性的形成起主导作用.在大陆地区，各向异性的强度随深度有显著变化.上地壳和上地幔盖层中的各向异性普遍较弱，而在流变性较强的下地壳和软流圈存在较大范围的各向异性.这一现象说明下地壳在岩石圈变形中可能有解耦作用.（2）在大于200 km深度的软流圈下部主要表现为VSH<VSV的各向异性，说明地幔物质垂直运动相对占优势地位.（3）在中国大陆东部可以看出一个大致趋势：在构造比较稳定的地区，岩石圈中VSH>VSV的各向异性比较显著，而软流圈中VSH<VSV的各向异性较弱；在构造活动比较强烈的地区，软流圈中VSH<VSV的各向异性占主导地位.（4）印度板块低角度向青藏高原下俯冲影响了中国大陆西部地区各向异性的特征.印度板块向北运动水平挤压中国西部大陆，使得物质定向重结晶，从而在岩石圈下部产生显著的VSH>VSV各向异性.  相似文献   

太阳光谱望远镜散射光初步测定     

李如凤  张霄宇  陈学昆 《天文研究与技术》1998,(2)

报告了云南天文台太阳光谱望远镜散射光的测定,用零级光谱测定仪器轮廓的方法得到白光散射光最大为８％,平均为５％,估计光路系统改进后仪器散射光将减少。  相似文献   

FDY—9601微机测氡仪     

张彪  梁树红 《铀矿地质》1998,14(4):241-243

本文介绍了由核工业北京地质研究院仪器研究中心研制的FDY－9601微机测氡仪。它是一种借助于经过加压极化处理过的聚酯薄膜片收集氡衰变产生的子体218Po（RaA）,并测量其放出的α射线强度的微机测氡仪。  相似文献   

双频激电法在云南禄劝新发铜矿区的应用     

杨剑  王永华  艾斯卡尔  李华 《云南地质》2010,29(4):458-460,455

以禄劝新发铜矿区为例,研究在山区运用双频激电法进行矿产远景调查的效果。结果表明:在交通不便、自然条件差的山区,双频激电法具有轻便、快速等优点。找矿效果理想,与地质、化探结果吻合,为双频激电法研究提供了一个可供参考的实例。  相似文献   

Partial redistribution effects on line polarization in the presence of velocity fields     

K. N. Nagendra 《Solar physics》1996,164(1-2):67-78

Velocity fields in line formation regions strongly affect the line polarization. The conventionally used observer's frame method of solving the polarized transfer equation becomes expensive and inaccurate for partial redistribution problems, when large amplitude velocity fields have to be considered in the observer's frame. An alternative method of solution is the comoving frame method. Partial redistribution problems are solved using comoving frame formalism for line polarization caused by resonance scattering.  相似文献   

The QUaD experiment     

C. Pryke   《New Astronomy Reviews》2006,50(11-12):984

QUaD is a 31 pixel array of polarization sensitive bolometer pairs coupled to a 2.6 m Cassegrain radio telescope. The telescope is attached to the mount originally built for the DASI experiment and located at the South Pole. The telescope system is described along with details of instrumental characterization studies which we have performed. A first season of CMB observations is complete and the second season underway. Details of the current status of these observations and their analysis are presented.  相似文献   

Advances in radiative transfer     

Rainer Wehrse  Wolfgang Kalkofen 《Astronomy and Astrophysics Review》2006,13(1-2):3-29

This review describes advances in radiative transfer theory since about 1985. We stress fundamental aspects and emphasize modern methods for the numerical solution of the transfer equation for spatially multidimensional problems, for both unpolarized and polarized radiation. We restrict the discussion to two-level atoms with noninverted populations for given temperature, density and velocity fields. Unfortunately this article was originally published with typesetter's errors: The correct publication date was 25 February 2006, not 3 January 2006. The content was not in the final form. The publishers wish to apologize for this mistake. The online version of the original version can be found at /10.1007/s00159-005-0025-8.  相似文献   

Pure pseudo-C_ℓ estimators for CMB B-modes     

Kendrick M. Smith   《New Astronomy Reviews》2006,50(11-12):1025

Fast heuristically weighted, or pseudo-C_ℓ, estimators are a frequently used method for estimating power spectra in CMB surveys with large numbers of pixels. Recently, Challinor and Chon showed that the E–B mixing in these estimators can become a dominant contaminant at low noise levels, ultimately limiting the gravity wave signal which can be detected on a finite patch of sky. We define a modified version of the estimators which eliminates E–B mixing and is near-optimal at all noise levels.  相似文献   

X波段双极化多普勒天气雷达极限降水的估计能力     

史朝  何建新  刘艳 《气象科学》2010,30(2):245-249

首先分析了X波段双极化多普勒天气雷达降水估计的误差来源及其影响,然后分析了信比、积累阶数对降水估计精度的影响,明确雷达系统本身的测量误差所能达到的理想程度,结果表明在双通道的积累次数M=64,信噪比SNR=10dB的条件下差分反射率的σ(ZDR)=0.32dB,则相应R(Z,ZDR)的降水估计精度最好能达到44%,同样条件下差分相位的σ(ΦDP)=0.08°,那么在降水率R=50mm/h时R(KDP)的降水估计精度最好能达8.6%。  相似文献