雷达遥感图像分类新技术发展研究   总被引：6，自引：0，他引：6  

谭衢霖  邵芸 《国土资源遥感》2001,12(3):1-7

总结了雷达遥感图像分类技术的发展过程,指出新的分类技术正朝着采用新特征(如雷达极化信息与干涉信息、多参数极化干涉信息、多时相信息、DEM与地理信息等),应用新理论(如小波理论、分形理论、模糊理论),设计新算法(如改进的最大似然法、上下文分类法、改进的神经网络分类算法等)的方向发展.  相似文献   

Discovery of six high-redshift quasars with the Lijiang 2.4 m telescope and the Multiple Mirror Telescope     

Xue-Bing Wu  Wen-Wen Zuo  Qian Yang  Wei-Min Yi  Chen-Wei Yang  Wen-Juan Liu  Peng Jiang  Xin-Wen Shu  and Hong-Yan Zhou 《天文和天体物理学研究(英文版)》2012,(9):1185-1190

Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution of the early universe. Here we report the discovery of six new quasars with i-band magnitudes brighter than 19.5 and redshifts between 2.4 and 4.6 from spectroscopy with the Yunnan Faint Object Spectrograph and Camera (YFOSC) at the Lijiang 2.4 m telescope in February, 2012. These quasars are in the list of z > 3.6 quasar candidates selected by using our proposed J K/i Y criterion and the photometric redshift estimations from the SDSS optical and UKIDSS near-IR photometric data. Nine candidates were observed by YFOSC, and five among six new quasars were identified as z > 3.6 quasars. One of the other three objects was identified as a star and the other two were unidentified due to the lower signal-to-noise ratio of their spectra. This is the first time that z > 4 quasars have been discovered using a telescope in China. Thanks to the Chinese Telescope Access Program (TAP), the redshift of 4.6 for one of these quasars was confirmed by the Multiple Mirror Telescope (MMT) Red Channel spectroscopy. The continuum and emission line properties of these six quasars, as well as their central black hole masses and Eddington ratios, were obtained.  相似文献   

Investigation of the correlation between morphology and luminosity for two classes of main galaxies     

Xin-Fa Deng  Xiao-Xia Qian  Cheng-Hong Luo  Ping Wu 《Astrophysics》2012,55(1):45-52

Using an apparent-magnitude limited Main galaxy sample of the Sloan Digital Sky Survey Data Release 7(SDSS DR7), we investigate the correlation between morphologies and luminosity for the Main galaxy sample. Our Main galaxy sample is divided into two classes: Main galaxies only with TARGET_GALAXY flag (bestPrimtarget = 64), and ones also with other flags. It is found that for the second class Main galaxies, the early-type proportion monotonously increases with increasing luminosity nearly in the whole luminosity region. But for the first class Main galaxies, the early-type proportion increases with increasing luminosity only within a certain luminosity region (−22.2 < M _r  < −19.8). In the high luminosity region (M _r  < −22.2), the early-type proportion of the first class Main galaxies even decreases dramatically with increasing luminosity. We also analyze the correlation between morphologies and luminosity of galaxies around the peak of the redshift distribution ( 0.07 ≤ z ≤ 0.08 ). In such a narrow redshift region, we still observe strong correlation between morphologies and luminosity, which shows that this correlation is fundamental.  相似文献   

三维井间地震侧面波传播特征及其分离研究     

金聪  吴遵红  王薇  林松  邓小虎  程邈  谭凯 《地球物理学进展》2021,36(4):1531-1540

井间地震与常规地震相比具有较高的分辨率,同时波场也更加复杂.利用视速度特征的差异很容易地分离井间上下行波场,根据纵横波偏振特征的不同可将纵横波完全分离,但是针对井间地震侧面波的研究并不多.本文构建高速透镜体和断层模型进行波场数值模拟,通过对三维地震波场的传播特征进行分析可知,井间地震接收的波场既有岩性分界面的响应,还会有侧向地质不均匀体产生的干扰,严重影响成像的质量和精度.经偏振旋转后的T分量记录对物性横向变化较为敏感,综合分析X、Y、Z分量和T分量上不同连井剖面的波场传播特征,可对侧向传播的干扰波进行有效识别,利用线性Radon变换可以在一定程度上将侧面波进行压制,为后续井间地震资料处理提供高信噪比的数据.本文通过理论模型进行试算研究,验证了该方法的有效性,并对理论记录取得了较好的分离效果.  相似文献   

利用PS-InSAR研究合肥地区活动构造变形     

董雅竹  谭颖  张朋辉  查显杰 《地球物理学进展》2021,36(5):1822-1833

合肥地区位于我国大陆中部,其内展布有多条活动断裂,包括著名的郯庐断裂带.由于该地区大部分断裂是隐伏的,其分布位置、活动特性及构造仍存在争议.本文利用PS-InSAR技术处理了合肥地区2017年10月至2019年8月共52景Sentinel-1A卫星升轨SAR数据,获取了该区域的平均形变速率图.我们发现池河—太湖断裂、桥头集—东关断裂和肥中断裂构成的三角形块体内存在与断层活动相关的地壳InSAR形变.利用贝叶斯方法,本文分别对三条断裂附近区域的形变进行了反演.结果 显示:池河—太湖断裂的走向为北北东,倾向南东,运动特性以右旋走滑为主兼具少许拉张分量;桥头集—东关断裂的走向为北西,倾向北东,活动特性以右旋走滑为主兼具部分逆冲分量;肥中断裂为一条走向近东西、倾向向南的左旋走滑兼具逆冲运动的断裂.综合三条断裂的运动特征,我们推断该三角形块体受到郯庐断裂的活动和北西方向挤压作用的综合影响,整体有轻微旋转趋势.这可能是该地区小震聚集的原因,应引起足够的重视.  相似文献   

含水量和含盐量对粉质黏土热导率影响的试验研究     

段钊  谭轩  孙强  闫旭升 《地球物理学进展》2021,36(5):1834-1841

土壤传热性能作为地热资源开发的基础研究课题,近年来已经成为能源、工程、地球科学和地质学等领域的研究热点.然而有关盐渍黄土的热导率研究却很少被发表.针对关中地区地热资源开发的迫切需要,本研究借助瞬态平面热源法对黄土的热导率做了测量,得到了不同含水量(8％,10％,12％,14％,16％,18％)和不同含盐量(0％,2％,4％,6％)的黄土热导率数据.结合导热路径理论,双电层理论和"絮凝"现象对含水量和含盐量影响下的黄土热导率进行了讨论.获得了如下结论:(1)含水量的变化会引起黄土内部热量传导路径的变化,同时引起"液桥"现象对热量传递产生影响;(2) NaCl盐分对热导率的影响主要体现在对黄土颗粒周围双电层的改变,同时引起的"絮凝"作用会对导热路径产生不利影响进而降低黄土热导率;(3)总的来说,固-固传导,固-液传导和液-液传导作为三种典型的热量传导路径与黄土的含水量和舍盐量密切相关.  相似文献   

改进的标准化累积绝对速度及其在高速铁路地震报警应用中阈值的确定     

崔恩文  郭恩栋  王倩  孙逊 《震灾防御技术》2021,16(3):527-532

为降低无破坏性的近震小震对高速铁路地震报警的干扰,本文引入改进的标准化累积绝对速度作为报警参数,研究基于改进的标准化累积绝对速度地震报警阈值计算方法。通过建立车轨模型,分析不同周期横向简谐波作用下的列车安全运行极限状态,得出不同车速下改进的标准化累积绝对速度的起算阈值。参照标准化累积绝对速度CAV_STD计算公式,给出不同车速下改进的标准化累积绝对速度计算公式,并计算不同时速下列车分别在6条不同场地地震波作用下改进的标准化累积绝对速度报警阈值。  相似文献   

略阳县农居房屋抗震现状调查与评价研究     

郭光玲  郭瑞  徐乾 《震灾防御技术》2021,16(3):492-500

为精准识别贫困山区农居房屋结构现状完好程度,本文开展略阳县境内41894栋农居房屋抗震现状实地调查,搜集整理域内孕灾环境和致灾因子强度,统计分析域内各行政镇（办）经济水平、农居房屋抗震结构类型和震害等级,预测震害矩阵,计算平均震害指数,并评价抗震能力。研究结果表明:域内农居房屋抗震结构类型包括土木结构、砖木结构和砖混结构;域内农居房屋在VI度地震作用下基本完好的比例为74.04%,在VII度地震作用下发生轻微破坏以下震害等级的比例为83.45%,在VIII度地震作用下发生中等破坏以下震害等级的比例为85.46%;域内农居房屋在地震烈度为VI、VII、VIII、IX、X度时的平均震害指数分别为0.13、0.23、0.32、0.49、0.71,抗震性能较差,不满足“小震不坏、中震可修、大震不倒”的抗震设防目标。  相似文献   

柴达木盆地石炭系烃源岩和煤岩生物标志物特征及其地球化学意义   总被引：34，自引：7，他引：27  

孟仟祥  房嬛  徐永昌  沈平 《沉积学报》2004,22(4):729-736

采自柴达木盆地东北部石炭系烃源岩和煤岩的生物标志化合物研究表明,研究样品的有机质演化已达高成熟阶段,其母质来源以水生生物为主,同时有较丰富的陆源物质输入。除煤岩的沉积古环境较氧化且经历过较强的降解过程外,其余样品的沉积古环境均属于较还原环境,沉积介质为咸水环境,有机质总体丰度高。因此该区石炭系海陆交互相含煤沉积是一套较一般侏罗系为好的烃源岩系,有较好的生烃潜力。  相似文献   

XUV Photometer System (XPS): Improved Solar Irradiance Algorithm Using CHIANTI Spectral Models     

Thomas N. Woods  Phillip C. Chamberlin  W. K. Peterson  R. R. Meier  Phil G. Richards  Douglas J. Strickland  Gang Lu  Liying Qian  Stanley C. Solomon  B. A. Iijima  A. J. Mannucci  B. T. Tsurutani 《Solar physics》2008,250(2):235-267

Solar soft X-ray (XUV) radiation is highly variable on all time scales and strongly affects Earth’s ionosphere and upper atmosphere; consequently, the solar XUV irradiance is important for atmospheric studies and for space weather applications. Although there have been several recent measurements of the solar XUV irradiance, detailed understanding of the solar XUV irradiance, especially its variability during flares, has been hampered by the broad bands measured in the XUV range. In particular, the simple conversion of the XUV photometer signal into irradiance, in which a static solar spectrum is assumed, overestimates the flare variations by more than a factor of two as compared to the atmospheric response to the flares. To address this deficiency in the simple conversion, an improved algorithm using CHIANTI spectral models has been developed to process the XUV Photometer System (XPS) measurements with its broadband photometers. Model spectra representative of quiet Sun, active region, and flares are combined to match the signals from the XPS and produce spectra from 0.1 to 40 nm in 0.1-nm intervals for the XPS Level 4 data product. The two XPS instruments are aboard NASA’s Solar Radiation and Climate Experiment (SORCE) and Thermosphere, Ionosphere, Mesosphere, Energetics, and Dynamics (TIMED) satellites. In addition, the XPS responsivities have been updated for the latest XPS data processing version. The new XPS results are consistent with daily variations from the previous simple conversion technique used for XPS and are also consistent with spectral measurements made at wavelengths longer than 27 nm. Most importantly, the XPS flare variations are reduced by factors of 2 – 4 at wavelengths shorter than 14 nm and are more consistent, for the first time, with atmospheric response to solar flares. Along with the details of the new XPS algorithm, several comparisons to dayglow and photoelectron measurements and model results are also presented to help verify the accuracy of the new XUV irradiance spectra.  相似文献