基于多时相冠层结构参数对冠层光谱的敏感性分析     

齐腊  赵春江  黄文江  刘含海 《地理与地理信息科学》2009,25(6)

遥感反演的前提需对模型的输入参数进行敏感性分析.该文选取冬小麦返青期、拔节期、孕穗期和抽穗期,考虑输入参数之间的相关性,以辐射传输模型(PROSAIL)为研究对象,对比分析了局部敏感性和全局敏感性方法在模型不确定性和LAI敏感性上的差异.结果表明,随着冬小麦的生长,模拟光谱与实测光谱吻合度提高,模型模拟的不确定性降低;与局部敏感性方法相比,全局敏感性方法的模型不确定性降低,模拟精度提高,冠层光谱对LAI的敏感性有明显变化,植被指数对LAI的敏感性则相对稳定;与NDVI相比,TGDVI对LAI更敏感.  相似文献   

太阳诱导叶绿素荧光的卫星遥感反演方法   总被引：3，自引：0，他引：3  

张立福  王思恒  黄长平 《遥感学报》2018,22(1):1-12

利用卫星遥感探测区域和全球尺度太阳诱导叶绿素荧光SIF(Solar-Inducedchlorophyll Fluorescence)近年来成为研究热点。由于地球大气吸收和散射的影响,卫星尺度的SIF反演问题较为复杂,科学界对该问题一直存在争议,不同科学团队提出了众多方法。本文介绍了大气层顶SIF反演的机理、难点及思路,总结了近10年来最新发展的大气层顶SIF反演算法,并将这些算法归纳为3类:基于辐射传输方程的算法、简化的物理模型算法和数据驱动算法,分析讨论了各算法的特点及适用性;以应用最广泛的数据驱动算法为例,基于GOME-2数据详细介绍了算法的中间环节及注意事项;最后回顾了卫星遥感反演SIF的发展历程,汇总了目前及未来具有荧光探测能力的星载传感器,并依据数据源的特点相应地给出了适用的SIF反演算法,为今后基于航空和卫星高光谱数据的SIF反演提供了依据。  相似文献   

阴影区提取对高分辨率影像地形辐射校正的影响与分析     

宋丽瑶  张浩  林峰 《测绘通报》2017,(3):29

利用辐射传输机理对复杂山区进行地形辐射校正,可以全面地考虑太阳直接辐射亮度、天空散射辐射亮度及邻近地表反射辐射亮度3部分因素,从而取得较好的校正结果。遮蔽因子的准确提取是决定地形校正结果的关键因素。本文使用同一个辐射传输模型,针对同一片地表裸露山区的SPOT-5全色影像,分别使用对应的DEM和直方图阈值分割法计算遮蔽因子,并将得到的校正结果进行对比发现：在DEM精度不够高的情况下,使用直方图阈值分割法计算遮蔽因子,可以得到更好的地形校正效果,充分证明了直方图阈值分割法计算遮蔽因子的优势及使用价值。  相似文献   

Multilevel Line Transfer with the Implicit Integral Method     

L. Crivellari  O. Cardona  E. Simonneau 《Astrophysics》2002,45(4):480-488

Once the need for an iterative procedure in order to solve the problem of the formation of spectral lines in the case of a model atom with many energy levels, the sequel is to seek for the most effective form of such an iterative scheme. It is an almost universal is assumed within all the iterative methods for the solution of those radiative transfer problems, in which the transfer equations are coupled to the state of the matter, to take as the input of each step of iterations the values of the opacity coefficients obtained as a result of the previous one. This is, for instance, the procedure used to correct the temperature in the computation of stellar atmosphere models, or that to build the -operator (either the exact or the approximated one) within the Accelerated Lambda Iteration methods. Yet, if we assume, in order to solve the multilevel line transfer problem, that at each step of iterations the line opacities are known, we can express via the statistical equilibrium equations the populations of the energy levels - and consequently the source functions of the relevant spectral lines - as a linear function of the full set of the corresponding mean intensities of the radiation field. Once such linear forms for the source functions, we are able to solve without the need of any further approximation the radiative transfer equations for are obtained lines, now linearly coupled through the above linear forms of the statistical equilibrium equations. This is achieved by means of the Implicit Integral Method that we already presented in a series of previous papers.  相似文献   

AN ERROR ANALYSIS ON THE SIMULATED DATA OF TOVS HIRS BY RTTOV5 MODEL^*     

MA Gang  FANG Zongyi  ZHANG Fengying 《Acta Meteorologica Sinica》2002,16(2):226-241

The sounding data of meteorological satellites provide not only the real time weather information about the distribution of both cloud and rainfall,but also some others about the movement and state of atmosphere.They are important variables and parameters for NWP model used to simulate and predict atmospheric state.In order to introduce remote sensing information from satellites into NWP model,there is an efficient way of establishing an RT model by use of the atmosphere radiation sounding data of meteorological satellites to get the variables and parameters valuable to NWP model.In this paper,we set up profiles of air temperature and water vapor from the surface to upper (0.1 hPa) using the radiosounding data and the surface data from May to August 1998 atmosphere East Asia.A TOVS RT model (RTTOV5) is provided to compute the value of radiation value of HIRS channels in NOAA14.Then the radiation values of 19 HIRS channels are gotten.After matching these data computed by the RT model and the corresponding values coming from satellite sounding in time,the statistic distribution of bias between tile model output and the satellite sounding at each sounding channel can be gotten.At the same time.the distribution of RMS to every TOVS HIRS channel,the standard biases to different scanning angle to each channel are also obtained.  相似文献   

Modelling the H Lyman lines in evolved late-type stars     

S.A. Sim 《Monthly notices of the Royal Astronomical Society》2001,326(2):821-832

The importance of partial redistribution (PRD) in the modelling of the Lyman α and Lyman β emission lines of hydrogen in stellar atmospheres is examined using simple atmospheric models of a range of late-type stars. These models represent the subgiant Procyon (F5 IV–V), and the two giants β Gem (K0 III) and α Tau (K5 III). These stars are selected to span a wide range of surface gravities: 1.25< log  g <4.00 . The calculations are performed using the computer code multi with the modifications made by Hubeny & Lites. It is found that PRD effects are highly significant, both in the direct prediction of the Lyman line profiles and in the application of hydrostatic equilibrium to calculate the atmospheric electron density in static atmospheric models.  相似文献   

回旋同步辐射自吸收的特性     

周爱华 《天文学报》2005,46(1):12-18

详细研究了高能电子产生的回旋同步辐射自吸收的特性,并用磁偶极子场的 射电微波源模型计算了它的光学厚度.发现: (1)自吸率Kv随谐波数s的增加迅速地 下降,以致只有低次谐波(s<5)上的自吸收才会对微波爆发谱产生实质性的影响; (2) 自吸率κv随暗波数s下降的陡度还随高能电子的能谱指数δ的增加和其低能截止能量 E0的下降而迅速增加; (3)κv值还随传播角的增大而增加,并在70°至75°范围内达到 极值; (4)假设高能电子数密度为103cm-3,则在2≤s≤5范围内的自吸收的光学厚 度τvself在101-10-2之间变化,这些值约比回旋共振吸收的光学厚度τvgyro小3至4 个数量级.τvself在均匀磁场情况下可能被高估.只有当被加速的高能电子的数密度大于 104cm-3时,自吸收的光学厚度才开始能与回旋共振吸收的光学厚度相比较.  相似文献   

Radiative Transfer in Inhomogeneous Atmospheres. I     

A. G. Nikoghossian 《Astrophysics》2004,47(1):104-116

This series of papers is devoted to multiple scattering of light in plane parallel, inhomogeneous atmospheres. The approach proposed here is based on Ambartsumyan's method of adding layers. The main purpose is to show that one can avoid difficulties with solving various boundary value problems in the theory of radiative transfer, including some standard problems, by reducing them to initial value problems. In this paper the simplest one dimensional problem of diffuse reflection and transmission of radiation in inhomogeneous atmospheres with finite optical thicknesses is considered as an example. This approach essentially involves first determining the reflection and transmission coefficients of the atmosphere, which, as is known, are a solution of the Cauchy problem for a system of nonlinear differential equations. In particular, it is shown that this system can be replaced with a system of linear equations by introducing auxiliary functions P and S. After the reflectivity and transmissivity of the atmosphere are determined, the radiation field in it is found directly without solving any new equations. We note that this approach can be used to obtain the required intensities simultaneously for a family of atmospheres with different optical thicknesses. Two special cases of the functional dependence of the scattering coefficient on the optical thickness, for which the solutions of the corresponding equations can be expressed in terms of elementary functions, are examined in detail. Some numerical calculations are presented and interpreted physically to illustrate specific features of radiative transport in inhomogeneous atmospheres.  相似文献   

Radiative transfer effects on the Lyα forest     

A. Maselli  A. Ferrara 《Monthly notices of the Royal Astronomical Society》2005,364(4):1429-1440

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Reflection effect in close binaries. III. Distribution of radiation incident from an extended source     

A. Peraiah 《Journal of Astrophysics and Astronomy》1983,4(2):151-159

We have studied the effects of irradiation from an extended surface of the secondary component on the atmosphere of the primary. We have considered an isothermal and purely scattering medium. The resultant radiation field due to irradiation from an extended surface and self-radiation is different from that due to irradiation from a point source and self-radiation. In the case of the point source the middle layers of the exposed part of the atmosphere show maximum reflection while in the former case the reflection gradually decreases from the centre of the component towards the surface of the outermost layers of the atmosphere. The reflection effect appears to be strongly dependent on the density distribution of the electrons.  相似文献