The reciprocity properties of geometrical spreading     

Roel Snieder  & Chris Chapman 《Geophysical Journal International》1998,132(1):89-95

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米仓山叠加型推覆构造几何结构及演化   总被引：14，自引：0，他引：14  

《矿物岩石》1998,(Z1)

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The role of seawater constituents in light backscattering in the ocean   总被引：2，自引：0，他引：2  

Dariusz Stramski  Emmanuel Boss 《Progress in Oceanography》2004,61(1):27-56

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Coastal Bathymetry from Hyperspectral Remote Sensing Data: Comparisons with High Resolution Multibeam Bathymetry     

Michelle L. McIntyre  David F. Naar  Kendall L. Carder  Brian T. Donahue  David J. Mallinson 《Marine Geophysical Researches》2006,27(2):129-136

We present a large-scale quantitative test of a hyperspectral remote-sensing reflectance algorithm. We show that coastal bathymetry can be adequately derived through model inversions using data from the Airborne Visible-Infrared Imaging Spectrometer instrument. Data are analyzed from a shore-perpendicular transect 5 km offshore Sarasota, Florida at water depths ranging from 10 m to 15.5 m. Derived bottom depths are compared to a high-resolution multibeam bathymetry survey. Model-derived depths are biased 4.9% shallower than the mean of the multibeam depths with an RMS error of 7.83%. These results suggest that the model performs well for retrieving bottom depths from hyperspectral data in subtropical coastal areas in water depths ranging from 10 m to 15.5 m.  相似文献   

建筑物上侧击雷电的三维数值模拟   总被引：6，自引：6，他引：0       下载免费PDF全文

谭涌波  张鑫  向春燕  夏艳羚  马肖 《应用气象学报》2017,28(2):227-236

基于三维近地面闪电先导发展随机模式,通过改变先导初始电位和建筑物几何特性,分析各种情况下的侧击雷电发生概率,探讨侧击雷电产生原因及影响因素。结果发现:建筑物尖端电场畸变值是影响侧击雷电产生的重要参量,当下行先导靠近建筑物且传播位置低于建筑物的高度时,建筑侧面电场畸变值达到触发阈值,侧击雷电易产生;下行先导的初始电位以及建筑物几何特性（高度和宽度）是影响侧击雷电发生概率的重要因素,当下行先导初始电位在-9~-3 MV范围内,侧击雷电发生概率呈先增加后降低的趋势,当初始电位为-4.5 MV时,侧击雷电的发生概率达到峰值;当建筑物高度在50~150 m范围内,侧击雷电发生概率随着高度增加呈先增加后减少的趋势;当建筑物高度为100 m时,侧击雷电发生概率达到峰值;当建筑物宽度在30~70 m范围内,侧击雷电发生概率随建筑物宽度呈递减趋势;当建筑物宽度为30 m时,侧击雷电的发生概率达到峰值。  相似文献   

摄影测量与遥感的融合影像质量评价方法探讨   总被引：3，自引：2，他引：1  

杨晋强  武坚  程宝琴  王智 《测绘科学》2008,33(5)

遥感融合图像作为一种产品,其质量如何是图像使用者关心的一个重要问题。图像融合可为摄影测量与遥感提供高质量的遥感融合图像。本文运用主观评价、客观评价、几何质量等三种评价方法对融合后的遥感图像的质量展开讨论。通过实践这些评价方法能够达到融合后图像高质量地应用于摄影测量与遥感生产。  相似文献   

不同形状冰晶权重假定对冰云光学和辐射特性的影响   总被引：1，自引：0，他引：1  

陈琪  张华 《气象学报》2018,76(2):279-288

在BCC_RAD辐射传输模式和包含多形状冰晶粒子的冰云光学性质参数化方案的基础上,详细分析了不同冰晶粒子权重选取对冰云光学和辐射特性的影响。结果显示,不同形状冰晶粒子权重的选取对长波带平均消光系数、单次散射比、不对称因子和短波带平均不对称因子均有较大的影响。冰晶粒子权重选取对长波辐射通量有很大影响:对长波向下辐射通量,权重选择不同可在云底处造成高达10.50 W/m2的差别;对长波向上辐射通量,权重选择不同可在云顶处造成高达15.05 W/m2的差别。冰晶粒子权重选择对短波辐射通量也存在较大影响:对短波向下辐射通量,权重选择不同可在云底处造成高达12.48 W/m2的差别;对短波向上辐射通量,权重选择不同可在云顶处造成高达10.23 W/m2的差别。冰晶粒子权重选择对长波加热率影响较大,在云顶处和云底处分别可达1.31和-2.06 K/d。研究表明,不同形状冰晶粒子权重的选取对冰云光学性质和辐射计算均有较大的影响,在长波区间尤其明显。   相似文献   

基于相似特征点集的SIFT匹配改进算法     

高放  陆频频  王旭 《测绘工程》2016,25(6):19-23

当影像中存在相似或重复场景时,传统SIFT匹配算法存在匹配成功率低,目前改进的SIFT匹配算法计算量大。基于相似特征点集的SIFT匹配改进算法,依据相似性或重复场景的影像纹理特点,在SIFT特征点匹配过程中,通过设定阈值提取初始同名点,建立针对未成功匹配参考特征点的相似特征点集,利用已获取初始同名点建立仿射几何约束模型构建参考特征点的匹配约束窗口,在该窗口内利用特征点相对主方向及尺度约束,对特征相似点集进行匹配获得同名点,最后采用RANSAC算法剔除误匹配点。对比实验结果表明,在影像像对间存在较多相似性场景,同时存在较大尺度缩放、旋转变换、视角及模糊差异的情况下,文中算法在匹配成功率和计算复杂度上具有明显的优势。  相似文献   

SAR主从影像的几何配准     

廖强强  张立亭  刘洋 《测绘与空间地理信息》2016,(4):28-31

对于SAR主影像(master)和从影像(slave)的几何配准,文中采用三次基本多项式与斜距-多普勒定位模型,解算出主影像中心像素点在从影像中的同名点,最后得出主从影像中心像素点的初级配准偏移量。本文以上海地区ERS-1影像数据为例,在Matlab环境下,对SAR主从影像的几何配准偏移量进行解算。实验结果表明,采用文中初级配准方法,初级配准相对精度可达到0.1%~0.9%。  相似文献   

Post-equinox observations of Uranus: Berg’s evolution, vertical structure, and track towards the equator     

Imke de Pater  L.A. Sromovsky  P.M. Fry  Kathy Rages  Keith Matthews 《Icarus》2011,215(1):332-345

We present observations of Uranus taken with the near-infrared camera NIRC2 on the 10-m W.M. Keck II telescope, the Wide Field Planetary Camera 2 (WFPC2) and the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST) from July 2007 through November 2009. In this paper we focus on a bright southern feature, referred to as the “Berg.” In Sromovsky et al. (Sromovsky, L.A., Fry, P.M., Hammel, H.B., Ahue, A.W., de Pater, I., Rages, K.A., Showalter, M.R., van Dam, M. [2009]. Icarus 203, 265-286), we reported that this feature, which oscillated between latitudes of −32° and −36° for several decades, suddenly started on a northward track in 2005. In this paper we show the complete record of observations of this feature’s track towards the equator, including its demise. After an initially slow linear drift, the feature’s drift rate accelerated at latitudes ∣θ∣ < 25°. By late 2009 the feature, very faint by then, was spotted at a latitude of −5° before disappearing from view. During its northward track, the feature’s morphology changed dramatically, and several small bright unresolved features were occasionally visible poleward of the main “streak.” These small features were sometimes visible at a wavelength of 2.2 μm, indicative that the clouds reached altitudes of ∼0.6 bar. The main part of the Berg, which is generally a long sometimes multipart streak, is estimated to be much deeper in the atmosphere, near 3.5 bars in 2004, but rising to 1.8-2.5 bars in 2007 after it began its northward drift. Through comparisons with Neptune’s Great Dark Spot and simulations of the latter, we discuss why the Berg may be tied to a vortex, an anticyclone deeper in the atmosphere that is visible only through orographic companion clouds.  相似文献