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41.
线性光谱混合模型的适用观测尺度分析   总被引:1,自引:1,他引:0  
线性光谱混合模型是目前应用最广泛的光谱混合模型,但由于遥感观测多分辨率的特点,模型的适用性会受到尺度效应的影响。为探索该模型在不同观测尺度下的适用程度,本文从地物辐射原理出发,通过理论推导微面元辐射通量表达式,得出地物辐射通量除了与端元反射率和面积比有关外,也与天顶角存在显著的非线性关系。因此,在线性光谱混合模型和微面元辐射通量的基础上,推导了更具普适性的积分线性光谱混合模型的表达式,再采用数值模拟的方法,计算了两模型的相对差值Δρ,结果表明Δρ的大小仅与探测单元的半瞬时视场角β有关,并通过实测光谱实验对上述推论进行了验证。研究表明,当β13°时,Δρ较小,线性光谱混合模型是积分线性光谱混合模型的一种近似表达形式,β完全可作为确定线性光谱混合模型适用观测尺度的关键依据,并且该模型的适用程度随β的增大而降低。  相似文献   
42.
The results of field work on drift ice during wave propagation are analyzed and presented. The field work was performed in the Barents Sea, and the main focus of the paper is on wave processes in the MIZ. A model of wave damping in broken ice is formulated and applied to interpret the field work results. It is confirmed that waves of higher frequencies are subjected to stronger damping when they propagate below the ice. This reduces the frequency of most energetic wave with increasing distance from the ice edge. Difference of wave spectra measured in two relatively close locations within the MIZ is discussed. The complicated geometry and dynamics of the MIZ in the North-West Barents Sea allow waves from the Atlantic Ocean and south regions of the Barents Sea to penetrate into different locations of the MIZ.  相似文献   
43.
超声辅助方法是制备纳米材料的有效手段,可提高纳米材料的磁学、光学等特殊性能。本文在不同p H条件下超声辅助合成GdPO_4:Ce,Tb三元体系荧光粉,采用X射线粉末衍射、傅里叶变换红外光谱、扫描电镜、透射电子显微镜及光致发光荧光光谱分析方法对样品进行了表征。结果表明:①样品仅在p H=1时,才能生成规则的15 nm×104nm六方晶系纳米棒状正磷酸盐绿色荧光粉,晶体优先选择(102)及(200)晶面生长;p H1无法得到样品;p H1为颗粒状的正磷酸盐绿色荧光粉。②进一步验证了Gd、Ce、Tb三元体系中Ce~(3+)离子能量较高的5d组态将能量传递给Gd~(3+)离子,而Gd~(3+)离子的跃迁发射与Tb~(3+)离子的吸收峰有较大的光谱重叠,故传递途径是Ce~(3+)→Gd~(3+)→Tb~(3+);少量Ce~(3+)的引入可提高以GdPO_4基质发光材料的发光强度。此结果可为开发稀土材料提供理论依据。  相似文献   
44.
Usually,because of the Starkbroadening for the spectrum lines,the half widths of hydrogen higher Balmer emission lines of the solar flare increase with the principal quantum number N. Their variation curve,as observed before,has a minimum value near N=8 or 9. However,a curve for the solar flare which occurred at the limb of solar disk on June 12,1982shows an all-time decline with increasing N. How to explain this phenomena remains to be discussed.  相似文献   
45.
A statistical method is proposed for estimation of the corner frequency. It is based on inference for a stochastic model whose short-term behavior resembles the established source time functions. Properties of the estimates are investigated and some numerical examples are presented. A discussion concerning earthquake–explosion discrimination and the way corner frequency can be related to the rate of zero-crossings is also included. The paper is concluded with some numerical examples.  相似文献   
46.
The contribution of modal interaction in the various available spectrum superposition methods is accounted via the modal cross-correlation coefficient, which has been defined in several different approximate ways. Further, in these methods, to define the final expressions directly in terms of the response spectrum amplitudes, the peak factors for all the modal responses are approximated to be equal to the peak factor for the total structural response. However, these assumptions have been found to be violated significantly in many cases and do not hold good in general. Therefore, some recent studies have attempted to improve upon these assumptions. In this paper, detailed investigations are made to study the relative performance of the various available methods considering the modal interaction effects. To find out which of the available methods, in general, gives the better results, the response of a five-storey asymmetric hypothetical building, characterized by significant interaction effects, has been computed from different methods for several widely differing input excitations and the results have been compared with the exact time-history solution.  相似文献   
47.
We study a generic class of models for ultra-high energy cosmic ray (UHECR) phenomenology, in which the sources accelerate protons and nuclei with a power-law spectrum having the same index, but with different values for the maximum proton energies, distributed according to a power-law. We show that, for energies sufficiently lower than the maximum proton energy, such models are equivalent to single-type source models, with a larger effective power law index and a heavier composition at the source. We calculate the resulting enhancement of the abundance of nuclei, and find typical values of a factor 2-10 for Fe nuclei. At the highest energies, the heavy nuclei enhancement ratios become larger, and the granularity of the sources must also be taken into account. We conclude that the effect of a distribution of maximum energies among sources must be considered in order to understand both the energy spectrum and the composition of UHECRs, as measured on Earth.  相似文献   
48.
During Rosetta’s flyby of the asteroid (2867) Šteins in 2008, we used the ALICE instrument to measure the first far-ultraviolet (FUV) reflectivity spectrum of an asteroid (850-2000 Å). It is very dark in the FUV, ∼4%, compared to its very high reflectivity (40%) at optical wavelengths. The FUV albedo does not exhibit a systematic color trend across the spectral range, but there is a broad absorption feature, not yet identified with a specific mineral, with maximum depth near 1650 Å. The shape of this feature implies a very low abundance of Fe2+ ions in the surface minerals. The FUV brightness exhibits a significant opposition surge at phases below 10°. The visible/FUV color gets much redder with increasing phase angle inside the opposition surge and gets gradually redder at larger phase angles. We also conducted a deep search for an exosphere of atoms sputtered from the surface and set upper limits on any column densities of oxygen and hydrogen atoms at the time of our observations. The upper limit for H is comparable to that predicted by the only theoretical prediction of which we are aware, while that for O is higher than predicted by about an order of magnitude.  相似文献   
49.
提出了一种基于多相滤波器的新型宽带射电频谱仪的设计方案。通过多相滤波器实现宽带射电信号的滤波,对滤波后的基带信号进行数字功率检波,再通过积分控制,最终得到射电信号的频谱强度。仿真分析表明,这一设计具有很好的效果,通过多相滤波器,使信号的速率大为降低,克服了传统频谱仪以及采用FFT实现频谱变换方法的缺点,可以实现对超宽带射电信号的实时频谱分析。  相似文献   
50.
一次多回击闪电过程的物理特性分析   总被引:1,自引:0,他引:1  
利用西藏那曲无狭缝光栅摄谱仪获得的一次多回击云对地闪电光谱,研究了各放电通道的温度及其变化。结果表明,一次闪电不同回击过程的通道温度有明显差异,闪电前期的温度通常较高,之后呈逐渐降低趋势。将闪电光谱与同步电学观测资料相结合,讨论了光谱特征、通道温度与闪电放电特性、电流热效应的相关性。数据分析显示,光谱总强度与辐射电场的变化幅度成正比;光谱总强度与放电电流的大小成正比;通道温度与回击过程传输的能量为正相关。  相似文献   
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