Jacobian matrix for near-infrared remote sensing based on vector radiative transfer model     

Bai  Wenguang  Zhang  Peng  Zhang  Wenjian  Li  Jun  Ma  Gang  Qi  Chengli  Liu  Hui 《中国科学:地球科学(英文版)》2020,63(9):1353-1365

Due to the polarization effects of the Earth's surface reflection and atmospheric particles' scattering, high-precision retrieval of atmospheric parameters from near-infrared satellite data requires accurate vector atmospheric radiative transfer simulations. This paper presents a near-infrared vector radiative transfer model based on the doubling and adding method. This new model utilizes approximate calculations of the atmospheric transmittance, reflection, and solar scattering radiance for a finitely thin atmospheric layer. To verify its accuracy, the results for four typical scenarios(single molecular layer with Rayleigh scattering, single aerosol layer scattering, multi-layer Rayleigh scattering, and true atmospheric with multi-layer molecular absorption, Rayleigh and aerosol scattering) were compared with benchmarks from a well-known model. The comparison revealed an excellent agreement between the results and the reference data, with accuracy within a few thousandths. Besides, to fulfill the retrieval algorithm, a numerical differentiation-based Jacobian calculation method is developed for the atmospheric and surface parameters. This is coupled with the adding and doubling process for the radiative transfer calculation. The Jacobian matrix produced by the new algorithm is evaluated by comparison with that from the perturbation method. The relative Jacobian matrix deviations between the two methods are within a few thousandths for carbon dioxide and less than 1.0×10~(-3)% for aerosol optical depth. The two methods are consistent for surface albedo, with a deviation below 2.03×10~(-4)%. All validation results suggest that the accuracy of the proposed radiative transfer model is suitable for inversion applications. This model exhibits the potential for simulating near-infrared measurements of greenhouse gas monitoring instruments.  相似文献   

塔里木盆地苏盖特布拉克剖面寒武系第二统第三阶微生物岩结构类型^*          下载免费PDF全文

李莹  潘文庆  吴亚生  杨果  孙崇浩  姜红霞 《古地理学报》2020,22(4):663-679

塔里木盆地阿克苏地区寒武系第二统第三阶肖尔布拉克组主要由微生物白云岩组成,代表性的剖面在阿克苏市西南90 km处的苏盖特布拉克。由于成岩作用改造严重,对这套微生物碳酸盐岩的特征和形成环境的认识还存在很多分歧,制约了勘探工作。通过详细野外勘察和室内研究,将肖尔布拉克组微生物岩分为4种结构类型: 凝块结构、纹层结构、砂屑结构和骨架结构。首次对凝块结构和纹层结构进行了亚类型的划分,其中凝块结构可划分为蠕虫状、网状和斑点状3种亚类型,纹层结构可划分为致密纹层、短薄纹层、颗粒纹层以及单纹层、纹层组、复合纹层。肖Ⅰ段—肖Ⅲ段发育凝块石白云岩、凝块—层纹石白云岩和层纹石白云岩,肖Ⅳ段发育凝块石微生物丘,肖V段下部发育网状结构凝块石白云岩,肖V段上部发育砂屑白云岩和肾形菌骨架岩。白云石化作用、溶蚀作用、重结晶作用是改变肖尔布拉克组微生物岩结构最重要的成岩作用,且该组下部比上部遭受了更强的成岩作用改造;微生物岩结构对成岩作用改造的抵抗能力为: 砂屑结构>纹层结构>凝块结构。根据微生物岩结构,推测肖Ⅰ段—肖Ⅲ段形成于潮坪环境,肖Ⅳ段和肖V段下部形成于深水潮下环境,肖V段上部形成于浅水潮下环境。以上成果为认识塔里木盆地肖尔布拉克组微生物岩的平面分布规律和今后开展被成岩作用强烈改造的白云岩型微生物岩的研究提供了一个重要参考。  相似文献   

Discovery of Four New Clusters in the Cygnus Cloud     

秦松梅  李静  陈力  钟靖 《天文和天体物理学研究(英文版)》2021,(2)

We report the discovery of four new open clusters(named QC 1,QC 2,QC 3 and QC 4)in the direction of Cygnus Cloud and select their members based on five astrometric parameters(l,b,ω,μα*,μδ)of Gaia DR2.We also derive their astrophysical parameters for each new cluster.Structure parameters are generated by fitting the radial density distribution with a King’s profile.Using solar metallicity,we performed isochrone-fitting on their purified color-magnitude diagrams(CMDs)to derive the age of the clusters.The known cluster NGC 7062 in an adjacent area is chosen to verify our identification process.The estimated distance,reddening and age of NGC 7062 are in good agreement with the literature.  相似文献   

Hydrological management strategies for the control of algal blooms in regulated lowland rivers     

Jian Li  Wei Yin  Haiyan Jia  Xiaokang Xin 《水文研究》2021,35(6):e14171

Reservoirs of lowland floodplain rivers with eutrophic backgrounds cause variations in the hydrological and hydraulic conditions of estuaries and low-dam reservoir areas, which can promote planktonic algae to proliferate and algal bloom outbreaks. Understanding the ecological effects of variations in hydrological and hydraulic processes in lowland rivers is important for algal bloom control. In this study, the middle and lower reaches of the Han River, China, a typical regulated lowland river with a eutrophic background, are selected. Based on the effect of hydrological and hydraulic variability on algal blooms, a hydrological management strategy for river algal bloom control is proposed. The results showed that (a) differences in river morphology and background nutrient levels cause significant differences in the critical threshold flow velocities for algal bloom outbreaks between natural river and low-dam reservoir sections; there is no uniform threshold flow velocity for algal bloom control. (b) There are significant differences in the river hydrological/hydraulic conditions between years with and without algal blooms. The average river flow, water level and velocity in years with algal blooms are significantly lower than those in years without algal blooms. (c) For different river sections where algal blooms occur and to meet the threshold flow velocities, the joint operation of cascade reservoirs and diversion projects is an effective method to prevent and control algal blooms in regulated lowland rivers. This study is expected to deepen our understanding of the ecological significance of special hydrological processes and guide algal bloom management in regulated lowland rivers.  相似文献   

Binary Star Fractions from the LAMOST DR4     

Zhi-Jia Tian  Xiao-Wei Liu  Hai-Bo Yuan  Bing-Qiu Chen  Mao-Sheng Xiang  Yang Huang  Chun Wang  Hua-Wei Zhang  Jin-Cheng Guo  Juan-Juan Ren  Zhi-Ying Huo  Yong Yang  Meng Zhang  Shao-Lan Bi  Wu-Ming Yang  Kang Liu  Xian-Fei Zhang  Tan-Da Li  Ya-Qian Wu  Jing-Hua Zhang 《天文和天体物理学研究(英文版)》2018,(5)

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.  相似文献   

LAMOST CCD camera-control system based on RTS2     

Yuan Tian  Zheng Wang  Jian Li  Zi-Huang Cao  Wei Dai  Shou-Lin Wei  Yong-Heng Zhao 《天文和天体物理学研究(英文版)》2018,(5)

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) is the largest existing spectroscopic survey telescope, having 32 scientific charge-coupled-device(CCD) cameras for acquiring spectra. Stability and automation of the camera-control software are essential, but cannot be provided by the existing system. The Remote Telescope System 2 nd Version(RTS2) is an open-source and automatic observatory-control system. However, all previous RTS2 applications were developed for small telescopes. This paper focuses on implementation of an RTS2-based camera-control system for the 32 CCDs of LAMOST. A virtual camera module inherited from the RTS2 camera module is built as a device component working on the RTS2 framework. To improve the controllability and robustness, a virtualized layer is designed using the master-slave software paradigm, and the virtual camera module is mapped to the 32 real cameras of LAMOST. The new system is deployed in the actual environment and experimentally tested. Finally, multiple observations are conducted using this new RTS2-frameworkbased control system. The new camera-control system is found to satisfy the requirements for automatic camera control in LAMOST. This is the first time that RTS2 has been applied to a large telescope, and provides a referential solution for full RTS2 introduction to the LAMOST observatory control system.  相似文献   

近断层速度脉冲与震源机制的关系浅析   总被引：1，自引：1，他引：0  

罗全波  陈学良  高孟潭  李宗超  李铁飞  张振 《震灾防御技术》2018,13(3):646-661

本文初步分析了近断层速度脉冲的成因和特点，主要包括方向性效应与滑冲效应，并通过中国台湾集集地震的脉冲记录，分析了断层破裂方向和位移大小等震源参数对脉冲强度的影响。此外，基于有限移动源理论，说明了断层辐射与速度脉冲分布的关系，并探讨了利用运动学震源模型研究近断层地震动对速度脉冲影响的技术路线；评述了7种典型的等效速度脉冲模型，建议进一步研究等效速度脉冲函数与震源机制之间的关系。最后，简述了不同类型的断层引起速度脉冲的差异，并推测了产生脉冲型地震动的下限条件，同时展望该研究在地震预警方面的可能性。  相似文献   

南海北部琼东南海域活动冷泉特征及形成模式   总被引：3，自引：0，他引：3       下载免费PDF全文

杨力  刘斌  徐梦婕  刘胜旋  关永贤  顾元 《地球物理学报》2018,61(7):2905-2914

近年来，活动冷泉的研究越来越受到关注.本文利用多波束数据、多道地震数据以及底质取样结果研究琼东南海域活动冷泉系统，分析活动冷泉的羽状流特征、海底地貌与底质特征以及流体活动构造特征.多波束水体数据上，观测到多个延伸高度超过750 m的气泡羽状流，海底流体活动非常强烈；多道地震上识别出麻坑、流体运移通道、气烟囱等流体渗漏相关的构造，与其他海域观测到的反射特征不同，羽状流的下方流体运移通道呈强振幅"串珠"反射；重力活塞取样在两个站位上获得浅表层块状天然气水合物.其中一个站位位于活动冷泉附近，天然气水合物赋存于海底以下8 m左右.基于以上三方面的数据，笔者提出了一个用于描述活动冷泉系统的形成模式，游离气通过气烟囱向上运移到达浅层，一部分在天然气水合物稳定带内形成天然气水合物，另一部分穿透天然气水合物稳定带到达海底，形成活动冷泉的羽状流.  相似文献   

基于偏微分方程的模型光滑处理在偏移成像中的应用          下载免费PDF全文

韩复兴  孙建国  王坤 《地球物理学报》2018,61(11):4558-4567

本文针对射线类偏移成像当中的速度模型光滑处理问题，借鉴数字图像处理当中的偏微分方程法，基于能量泛函，应用变分方法导出基于速度模型的偏微分方程实现射线类偏移成像当中的速度模型的光滑处理.由于偏微分方程法具有线性叠加特性、模型解的唯一性和局部特征保持性，因此，应用该算法可以实现基于原始速度模型空间结构的模型光滑处理.通过在原始速度模型以及光滑处理后的速度模型上计算速度的空间分布以及地震波走时、射线路径可以得出，偏微分方程法对速度模型的光滑处理能够很好地保持原始模型的空间结构，偏移成像结果也证明了该方法的实用性.  相似文献   

超慢速扩张环境下超镁铁质岩系统的热液硫化物成矿机理以及启示     

曹红  孙治雷  刘昌岭  姜学钧  何拥军  黄威  尚鲁宁  王利波  张喜林  耿威  施美娟  李东义 《海洋学报》2018,40(4):61-75

西南印度洋63.5°E热液区是在超慢速扩张洋脊发现的首个超镁铁质岩热液系统。对取自该区的热液硫化物样品进行了系统的矿物学和地球化学分析，矿物学分析结果表明:该热液区硫化物为富Fe型高温硫化物，且经历了较深程度的氧化蚀变，大量中间态的Fe氧化物充填在硫化物矿物间的孔隙及内部解理中；这些硫化物相以白铁矿为主，其次是等轴古巴矿和少量铜蓝，缺乏黄铁矿、闪锌矿。据推断，该区的热液成矿作用分为4个阶段:低温白铁矿阶段→高温等轴古巴矿阶段→自形白铁矿阶段→后期海底风化阶段（少量铜蓝以及大量的Fe的羟氧化物）。与之相对应，地球化学分析结果表明这些硫化物的Fe含量较高（31.57%~44.59%），Cu含量次之（0.16%~7.24%），而Zn含量普遍较低（0.01%~0.11%）；微量元素较为富集Co（328×10-6~2 400×10-6）和Mn（48.5×10-6~1 730×10-6）。该区硫化物中较高含量的Fe、Co与超镁铁质岩热液系统相似，明显高于镁铁质岩热液系统。独特的热液硫化物矿物学特征和元素组成可能与该区普遍出露的地幔岩、橄榄岩蛇纹石化作用以及拆离断层的广泛发育的环境有关。  相似文献