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31.
应用高光谱图像进行异常目标检测是高光谱遥感最重要的应用之一,而异常目标检测算法最为关键的是对背景的描述。rx 等经典算法受制于对背景分布的高斯假设,因而在复杂背景条件下不能有效地提取出感兴趣的异常目标。本文提出了一种新的异常目标检测算法,不仅能够有效地检测出亚像元的异常目 标,同时以新的方式描述背景。算法首先针对异常检测先验信息不足的问题,采用盲分解方法建立描述背景的冗余字典,该字典是根据像元的纯净性定义估计的背景类端元束构成;然后采用稀疏回归计算每个像元的重建误差,以误差特征作为异常指数,误差越大越可能是异常;为了增强对可能异常目标的描述能力,应用了局 部近邻分析来增强目标在图像邻域的离群表达,从而获得最终的异常检测特征。算法将字典构造的全局性与地物的局部连续性结合,提高了异常目标检测的可靠性。采用不同混合比例模拟的亚像元数据和两幅真实数据进行实验,结果表明,算法不仅仅获得了比 rx 等经典算法更高的精度,同时在不同信噪比条件下表现稳健且抗噪能力强。 相似文献
32.
D. Kilkenny D. O'Donoghue L. Crause C. Engelbrecht N. Hambly H. MacGillivray 《Monthly notices of the Royal Astronomical Society》2009,396(1):548-552
We report the discovery of very rapid pulsations in two hot subdwarf stars from the Edinburgh-Cape blue object survey. The short periods, small amplitudes and multiperiodicity establish these stars as members of the class of rapidly-pulsating sdB stars. The spectrograms of both stars, however, show relatively strong He ii 4686 and they are therefore more properly classified as sdOB. The light curve of EC 01541−1409 is dominated by two strong (∼1 per cent) variations with frequencies near 7114 and 7870 μHz (periods near 140.6 and 127.1 s), though at least five frequencies are present with amplitudes above about 0.002 mag. The light curve of EC 22221−3152 appears to be generated by at least 10 frequencies in the range 5670–11850 μHz (about 175–85 s) with amplitudes between about 0.01 and 0.001 mag, including the first overtone of the strongest variation. Somewhat surprisingly, this number of frequencies is detectable in observing runs as short as 3 h, probably due to the fact that the detected frequencies are well-separated. 相似文献
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河南省煤田地质局经济的持续快速发展,得益于不断推进科技进步。表现为着力巩固发展地勘优势,使核心技术得到不断升级和创新,形成强势竞争力。科技进步的核心问题是人。尊重人才的关键是改革用人机制,用事业留人,用待遇留人,用感情留人。 相似文献
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G. Handler E. Romero-Colmenero J. L. Provencal K. Sanchawala M. A. Wood I. Silver W.-P. Chen 《Monthly notices of the Royal Astronomical Society》2008,388(3):1444-1456
The pulsating DA white dwarfs are the coolest degenerate stars that undergo self-driven oscillations. Understanding their interior structure will help us to understand the previous evolution of the star. To this end, we report the analysis of more than 200 h of time-resolved CCD photometry of the pulsating DA white dwarf star EC 14012−1446 acquired during four observing epochs in three different years, including a coordinated three-site campaign. A total of 19 independent frequencies in the star's light variations together with 148 combination signals up to fifth order could be detected. We are unable to obtain the period spacing of the normal modes and therefore a mass estimate of the star, but we infer a fairly short rotation period of 0.61 ±0.03 d , assuming the rotationally split modes are ℓ= 1 . The pulsation modes of the star undergo amplitude and frequency variations, in the sense that modes with higher radial overtone show more pronounced variability and that amplitude changes are always accompanied by frequency variations. Most of the second-order combination frequencies detected have amplitudes that are a function of their parent mode amplitudes, but we found a few cases of possible resonantly excited modes. We point out the complications in the analysis and interpretation of data sets of pulsating white dwarfs that are affected by combination frequencies of the form f A + f B − f C intruding into the frequency range of the independent modes. 相似文献
36.
《Marine Policy》2017
Transition to low carbon sea transport is a logical response to the extreme dependency of the Pacific Islands region on imported fossil fuel, its significant vulnerability to the effects of climate change and the critical shipping needs of Pacific Island countries (PICs). Building on previous work in low carbon sea transport in the Pacific, this paper further considers the barriers to achieving such transition by assessing, through a ‘post-Paris Agreement’ lens, the Intended Nationally Determined Contributions (INDCs) submitted by PICs and contrasting these to the near total lack of investment and planning for low carbon transition in the transport sector with the parallel occurrence in the electricity sector where ~USD 2 billion of donor investment is deployed or queued despite electricity using only ~20% of fossil fuel across the region. Consistent with recent international studies, inadequate and inappropriate financing and policy have been identified as dominant transition barriers for low carbon sea transport development in PICs. This paper further examines the regional level barriers to policy development, and finds them inhibited by the silo nature of the major regional actors. The implications that the Paris Agreement has for climate financing to support the essential research and capacity development needed to underpin a successful low carbon sea transport transition strategy at any useful scale and speed are also considered in this paper. 相似文献
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本文应用动态系统时间连续模型建立的新方法(DM(n,h)模型),通过对唐山老震区ML>4.7级地震的建模,讨论DM(n,h)模型对唐山老震区晚期强余震预测的可行性。并比较了DM(n,h)模型与GM(n,h)模型,发现DM(n,h)模型优于GM(n,h)模型,同时,给出了唐山老震区晚期强余震的预报结果。 相似文献
40.
The effect of extraordinary degradation of phenol organics on the SnO2‐Sb2O3/Ti electrode is investigated through experimental research and theoretical analysis. The phenol organics contained 4‐chloro‐phenol, 4‐bromo‐phenol, and 2‐iodo‐phenol. At a current density of 4 mA cm–2 and an electrolysis time of 12 h, the degradation efficiency of the phenols was over 98% with a relatively short degradation time, whereas the degradation time of the PbO2/Ti electrode surpassed 40 h while delivering 100% disposal efficiency. Therefore, the effectiveness of electrochemical (EC) oxidation by the SnO2‐Sb2O3/Ti was superior to that of the PbO2/Ti electrode. At the same time, the SnO2‐Sb2O3/Ti had higher oxygen generation potential and lower electron consumption than the other electrodes. This was mainly due to the effect of the middle Sb2O3 layer, which due to its high porosity and good catalytic effect, contributed to a better catalysis than the SnO2 part. 相似文献