ADS辅助实现线极化到圆极化的转换     

CHEN Songlin 《中国科学院上海天文台年刊》2005,(1):103-109

给出C波段双圆极化低噪声接收机中圆极化输出的实现方案,研究了利用90°电桥进行线- 圆极化转换时两个线极化通道增益及相位的平衡度对圆极化隔离的影响。分析了如何通过调节一对同轴电缆的长度差来补偿相位不平衡,并借助ADS软件计算了该长度差,实现了线-圆极化转换,取得接收机两个圆极化之间的隔离度好于20dB的效果。  相似文献   

CCD imaging polarimetry of Comet 2P/Encke     

Nikolai N. Kiselev  Klaus Jockers 《Icarus》2004,168(2):385-391

We present results and analysis of imaging polarimetric observations of Comet 2P/Encke. The observations were carried out at the 2-m RCC telescope of the Bulgarian National Astronomical Observatory on December 13, 1993 and on January 14, 1994, at phase angles 51.1° and 80.5°, respectively. A wide-band red filter 6940/790 Å was used. This filter is transparent for the continuum and the weak emission bands of NH₂ and H₂O⁺. There is a sunward dust fan with well-defined polarization, which peaks at≈13% in the image obtained on January 14, 1994. Along the sunward fan the degree of polarization decreases progressively. Outside of the fan the coma displays a low polarization of ≈3%. We suggest that this low polarization is caused by the NH₂ emission in the pass-band of the red wide-band filter. Assuming a spherically symmetric NH₂ coma we are able to correct the observed polarization for this effect. The correction leads to an increase of the observed polarization by 1 to 4% at distances 10,000 and 1500 km from the nucleus. A rough estimate shows that the polarization in the near nucleus region of Comet Encke is similar to that for the dusty comets. Even after correction the polarization of Comet Encke's dust fan is significantly less that the polarization observed in dusty comets. The reasons influencing the distribution of dust polarization in the coma are discussed. More polarimetric and colorimetric observations of the dust in Comet Encke on its return in 2003 are needed.  相似文献   

Brightness and Polarization Variations of S Per and T Per     

T. A. Polyakova 《Astrophysics》2003,46(4):465-474

Results of photoelectric BV observations of the brightness and polarization in the V band for S Per and T Per over a period of eight years are presented. An attempt is made to isolate the interstellar polarization. A comparison of the variations in the brightness and intrinsic polarization reveals some relationships among these quantities.  相似文献   

The solution of the vector radiative transfer equation using the discrete ordinates technique: Selected applications   总被引：2，自引：1，他引：1  

V.V. Rozanov  A.A. Kokhanovsky   《Atmospheric Research》2006,79(3-4):241-265

The paper is devoted to the presentation of a newly developed radiative transfer code SCIAPOL_1.0 for a plane-parallel turbid slab illuminated by the monodirectional wide beam. The SCIAPOL_1.0 is based on the discrete-ordinates solution of the vector radiative transfer equation.The code is applied to a number of problems, including studies of the applicability of the scalar approximation for the calculation of light reflectance from aerosols, clouds, and molecular atmospheres. We also study the accuracy of the single scattering approximation as applied to the calculation of light reflection from molecular and cloudy atmospheres and propose new approximations for the calculation of the reflection function and the degree of light polarization under unpolarized light illumination conditions.  相似文献   

Polarization Observation Experiments for Radio Flares of Stars at the 6 cm Band     

Bai Jian-yong  Han Jin-lin  Gao Xu-yang  Wang Chen  Zhang Li-yun 《Chinese Astronomy and Astrophysics》2013

We have performed radio polarization observation experiments of the stars V772 Her and β Per with the Urumqi 25 m radio telescope at the 6 cm waveband, and obtained light curves of the stars after data processing and calibration. A radio ?are from the star V772 Her was detected on 2011 April 13. The degree of linear polarization of this ?are is about 30%, and the polarization angle is about 4°. We have detected also the slowly-varying component of the radio radiation from β Per, as well as a short ?are superposed on it, which has a very weak linear polarization.  相似文献   

四川芦山M_S7.0和汶川M_S8.0地震前地电场变化研究          下载免费PDF全文

安张辉  杜学彬  谭大诚  范莹莹  刘君  崔腾发 《地球物理学报》2013,56(11):3868-3876

应用四川芦山M_S7.0和汶川M_S8.0震中周围部分地电场观测台站的资料,主要利用地电场波形比较和极化方位变化两种方法,并结合观测台站的工作日志,对两次地震前地电场观测资料进行了分析研究,并得出:芦山M_S7.0和汶川M_S8.0地震前部分台站地电场波形出现变异现象,主要表现为两种形式:日变波形的畸变(如盐源台和泸沽湖台)和相应时段地电场频谱特性出现变化,这些变异基本上出现在震前1~2个月内;利用两次地震前地电场观测的日均值计算了部分观测台站的地电场极化方位,发现在震前地电场的极化方位出现了大幅变化,最大变化幅度达160°,最小变化幅度也有10°;初步研究还发现,两次地震前夕,震中周围部分台站极化方位的正向或反向延长线,相汇集的区域与地震的震中有一定联系;对于研究所得结果,从地震电信号的产生机制和震源特性方面进行了尝试性理论解释.  相似文献   

A_3钢在MgCl_2溶液中腐蚀行为研究          下载免费PDF全文

李成栋  余红发 《盐湖研究》2010,18(3)

以MgCl2溶液模拟氯氧镁水泥孔隙液,研究了A3钢在MgCl2溶液中的腐蚀行为和腐蚀速率,并利用电化学测试仪对A3钢腐蚀过程的电化学特征进行了研究。实验结果表明,随着MgCl2浓度的减小以及在MgCl2溶液中浸泡时间的延长,A3钢的腐蚀失重速率逐渐变小;极化曲线测试与腐蚀失重试验结果相吻合;阻抗曲线(EIS)研究发现,随着A3钢在MgCl2溶液中浸泡时间的延长钝化膜的电阻变大;扫描电镜观察表明,经MgCl2溶液腐蚀后,在A3钢样品表面产生了许多腐蚀产物,XRD分析证实主要产物为Fe3O4和MgFe2O4。  相似文献   

地壳剪切波分裂研究及地震定位误差对剪切波分裂分析的影响   总被引：1，自引：0，他引：1  

赵博  高原 《地震》2010,30(1):115-124

地壳介质的各向异性主要是由大量充满液体的微裂隙的定向排列引起的, 剪切波穿过这种含有微裂隙的介质时会产生分裂。 剪切波分裂参数与地壳介质的物理性质有关, 与区域应力场有关。 在地壳剪切波分裂研究中, 地震的定位误差对剪切波分裂参数有影响。 本文简单介绍了几种影响定位精度的因素; 并对定位误差特别是深度方向的误差所引起的时间延迟变化进行了讨论, 比较了不同大小的深度误差对归一化后的时间延迟的影响, 定量分析结果显示, 深度定位误差对慢剪切波时间延迟影响很大。 剪切波分裂分析方法有多种, 本文还对不同的剪切波分裂分析方法做了简介。  相似文献   

SKS波对地壳裂隙各向异性的响应——理论地震图研究   总被引：2，自引：2，他引：0       下载免费PDF全文

姚陈  郝重涛  张广利 《地球物理学报》2016,59(7):2498-2509

穿透含裂隙、裂缝地壳8s视周期的SV波的理论地震图研究表明,当地壳平均裂隙密度高于0.01即横波各向异性高于1%时,非对称面内不同方位的SKS波均发生分裂;地震图中直接的记录显示是切向T分量上出现SKS波的振动,其振幅随地壳平均裂隙密度的增大而增强,甚至能与径向R分量上的振幅相当.局限于上地壳的强裂缝各向异性同样能引起SKS分裂.长周期SKS波分裂对地壳内裂隙、裂缝的分布缺乏分辨率.直立平行排列裂隙、裂缝使得SKS分裂T分量记录特征具有方位对称性,这来自于HTI介质中快、慢波偏振和到时差随方位变化的对称性;而倾斜裂隙、裂缝使得该方位对称性丧失.对实际观测SKS分裂的偏振解释需要考虑地壳裂隙各向异性,特别是断裂附近的强裂缝各向异性.  相似文献   

大地电磁测深二维反演方法求解复杂电性结构问题的适应性研究   总被引：3，自引：1，他引：2  

董浩  魏文博  叶高峰  金胜  景建恩  张乐天  张帆  谢成良 《地球物理学报》2012,55(12):4003-4014

为探讨二维反演方法在三维电性结构中的适应性问题,本研究中设计了一系列的二维/三维正演模型进行实验计算,分析了三维高阻/低阻异常体对模型响应的畸变作用,并从反演模式选择和数据旋转方向两个方面进行模型二维反演的对比分析,与三维反演的结果进行了比较,最后采用了实测数据进一步进行了二维和三维反演的比较实验.实验和研究结果表明,在剖面选择方面,在剖面方向与垂直主构造方向相差不大的情况下,截取剖面方向,将电性主轴旋转到垂直剖面方向的二维反演结果与垂直主构造方向的反演结果都可以较好地还原正演模型,在大的构造的反映上并无太大差异.在地下为二维或近三维条件时,正演模型的主要结构都可以较好地被二维和三维反演解析出来.二维的反演结果可能甚至会比三维的反演结果的边界更清晰,更精确.然而,对于具有较强的三维结构的模型而言,其二维反演结果与原始模型可能仍然存在较大差异,其中TM+TP或TM模式的二维反演结果相对更接近原始模型,而TE模式的结果往往会有较大误差,需要在解释时特别注意以免得出错误结论.  相似文献