斑岩型钼矿激电测深的找矿模式

近年来在新县吴陈河风响山钼(金、银)矿区开展地质和物探普查,发现了明显的激电异常。经钻探验证,揭示了风响山钼矿化带,得出了斑岩型钼矿“三位一体”——构造、斑岩体、激电异常的找矿模式。     

Medium-scale traveling ionospheric disturbances observed by GPS receiver network in Japan: a short review

Medium-scale traveling ionospheric disturbances (MSTID) are wave-like perturbations of the ionospheric plasma with wavelengths of several hundred kilometres and velocities of several hundred metres per second. MSTID is one of the most common ionospheric phenomena that generally induce the perturbations of ionospheric total electron content (TEC) by ∼10¹⁶ electron/m², which corresponds to ∼54 ns (16.2 cm) delay at GPS L1 signal. In the past decade, several new characteristics on MSTIDs have been revealed by the TEC observations using the dense GPS receiver network in Japan. In this paper, we provide a short review of these new observations and summarize the morphological characteristics of MSTIDs in Japan.     

九十年代广东省不同经济地域差异分析

在改革开放以来的第二个十年里,广东省区域差异在不断深化的同时出现了一些新的特征,由此导致广东省的空间结构进入一个新的层次。文中以美国学者Ｊ．Ｆｒｉｅｄｍａｎ的核心－边缘模式作为理论基础,分析了广东省四大经济地域发展水平的差异,探讨了空间极化与空间扩散趋势。研究表明,９０年代以来,广东省在极化作用持续加强、区域差异不断扩大的同时,扩散效应已 开始显现,即在不平稳发展中出现了平稳的趋势,从而使核心－边     

高分五号卫星大气参数探测综述

高分五号卫星搭载了大气痕量气体差分吸收光谱仪、主要温室气体探测仪、大气多角度偏振探测仪、大气环境红外甚高分辨率探测仪、可见短波红外高光谱相机和全谱段光谱成像仪共6台载荷,对全球环境监测及中国大气气溶胶、臭氧、二氧化硫、二氧化氮、二氧化碳、甲烷和云等多个环境与气象综合监测方面有着重要的意义。为了更好的了解高分五号卫星任务的大气监测内容,本文对高分五号卫星其中的4个大气探测载荷特征和数据处理算法进展进行了总结,涉及各个载荷参数信息、算法介绍和产品初步结果等相关内容。高分五号卫星是中国专门用于大气环境监测任务的遥感卫星,随着后续卫星的发射升空,将对中国乃至全球大气环境监测提供强有力的数据支撑。     

汶川地震前地脉动信号的单台法研究

汶川地震前,我国及周边地区地震台站记录的地脉动信号显著增强,对这段时期内的地脉动信号进行频谱分析发现,它们的能量主要集中在0.20Hz附近.通过单台法对该频段信号进行定向,发现多个大陆和海岛台站记录的地脉动信号来源方向均指向我国东部海域,且方向变化与同期的威马逊台风路径保持很好的一致性.结合已有的地脉动信号强度随与台风...     

A circular statistical method for extracting rotation measures

We propose a new method for the extraction of Rotation Measures from spectral polarization data. The method is based on maximum likelihood analysis and takes into account the circular nature of the polarization data. The method is unbiased and statistically more efficient than the standard χ² procedure.     

The Cosmic Foreground Explorer (COFE): A balloon-borne microwave polarimeter to characterize polarized foregrounds

The COsmic Foreground Explorer (COFE) is a balloon-borne microwave polarimeter designed to measure the low-frequency and low-ℓ characteristics of dominant diffuse polarized foregrounds. Short duration balloon flights from the Northern and Southern Hemispheres will allow the telescope to cover up to 80% of the sky with an expected sensitivity per pixel better than 100 μK/deg² from 10 GHz to 20 GHz. This is an important effort toward characterizing the polarized foregrounds for future CMB experiments, in particular the ones that aim to detect primordial gravity wave signatures in the CMB polarization angular power spectrum.     

2006年3月29日日全食白光日冕偏振测量

报告了在埃及赛路姆观测到的2006年3月29日日全食白光偏振测量的基本结果.我们使用的是一架便携式反射望远镜,焦距为640mm(F/D=8).在物镜前方安置可旋转线偏振片,每次旋转角度45°,终端为尼康数码相机.观测过程中,改变曝光时间并旋转偏振片,总共获取20张数码照片.文中讨论并呈现了介于 1.3 R⊙＜r ＜3.0 R⊙范围内的白光偏振方向和偏振度的大小分布.     

Site evaluation and RFI spectrum measurements in Portugal at the frequency range 0.408–10 GHz for a GEM polarized galactic radio emission experiment

We probed for radio frequency interference (RFI) at three potential galactic emission mapping experiment (GEM) sites in Portugal using custom made omnidirectional disconic antennas and directional pyramidal horn antennas. For the installation of a 10-m dish dedicated to the mapping of polarized galactic emission foreground planned for 2005–2007 in the 5–10 GHz band, the three sites chosen as suitable to host the antenna were surveyed for local radio pollution in the frequency range 0.01–10 GHz. Tests were done to look for radio broadcasting and mobile phone emission lines in the radio spectrum. The results show one of the sites to be almost entirely RFI clean and showing good conditions to host the experiment.     

PAPPA: Primordial anisotropy polarization pathfinder array

The primordial anisotropy polarization pathfinder array (PAPPA) is a balloon-based instrument to measure the polarization of the cosmic microwave background and search for the signal from gravity waves excited during an inflationary epoch in the early universe. PAPPA will survey a 20° × 20° patch at the North Celestial Pole using 32 pixels in 3 passbands centered at 89, 212, and 302 GHz. Each pixel uses MEMS switches in a superconducting microstrip transmission line to combine the phase modulation techniques used in radio astronomy with the sensitivity of transition-edge superconducting bolometers. Each switched circuit modulates the incident polarization on a single detector, allowing nearly instantaneous characterization of the Stokes I, Q, and U parameters. We describe the instrument design and status.