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31.
From the point of view of the non-parametric statistics, a general estimation method of the accuracy and con?dence interval of preliminary orbit determination is proposed for the occasion without any other information but observational data. Based on the bootstrap method, the estimation relies only on the observational data and does not require the precise orbit determination as a reference, or the assumption of normal distribution of observational errors. Numerical experiments show that this method is very simple in implementa- tion, and may serve as an easy accuracy evaluation for the preliminary orbit determination and for the follow-up employments. 相似文献
32.
Remote sensing image segmentation is the basis of image understanding and analysis. However, the precision and the speed of segmentation can not meet the need of image analysis, due to strong uncertainty and rich texture details of remote sensing images. We proposed a new segmentation method based on Adaptive Genetic Algorithm (AGA) and Alternative Fuzzy C-Means (AFCM). Segmentation thresholds were identified by AGA. Then the image was segmented by AFCM. The results indicate that the precision and the speed of segmentation have been greatly increased, and the accuracy of threshold selection is much higher compared with traditional Otsu and Fuzzy C-Means (FCM) segmentation methods. The segmentation results also show that multi-thresholds segmentation has been achieved by combining AGA with AFCM. 相似文献
33.
The nucleus, coma, and dust jets of short-period Comet 19P/Borrelly were imaged from the Deep Space 1 spacecraft during its close flyby in September 2001. A prominent jet dominated the near-nucleus coma and emanated roughly normal to the long axis of nucleus from a broad central cavity. We show it to have remained fixed in position for more than 34 hr, much longer than the 26-hr rotation period. This confirms earlier suggestions that it is co-aligned with the rotation axis. From a combination of fitting the nucleus light curve from approach images and the nucleus' orientation from stereo images at encounter, we conclude that the sense of rotation is right-handed around the main jet vector. The inferred rotation pole is approximately perpendicular to the long axis of the nucleus, consistent with a simple rotational state. Lacking an existing IAU comet-specific convention but applying a convention provisionally adopted for asteroids, we label this the north pole. This places the sub-solar latitude at ∼60° N at the time of the perihelion with the north pole in constant sunlight and thus receiving maximum average insolation. 相似文献
34.
G. Beskin N. Borisov V. Komarova S. Mitronova S. Neizvestny V. Plokhotnichenko M. Popova 《Astrophysics and Space Science》1997,248(1-2):51-57
I summarize fully-sampled observations of the 3 mm emission from CO and HCN in the inner arcminute of NGC 1068. The CO emission
is distributed in the form of a molecular bar, coincident with the infrared bar, from which emanate two spiral arms. A relatively
weak concentration of CO line emission is found at the nucleus. By contrast, the HCN emission is strongly concentrated at
the center, with relatively weak emission in the region of the star-forming arms. The ratio of HCN to CO integrated intensities
is about 0.6 over the central r ≉ 175 pc and is the highest ratio measured in the center of any galaxy; the ratio reflects
the high thermal pressure (TK ~ 50 K, n[H2] ~ 4 × 106 cm-3) in the few hundred parsecs surrounding the nucleus.
The kinematics in the star-forming arms are well described by circular orbits, with ordered noncircular motions of < 30 km
s-1 that may be attributed to spiral density wave streaming. Interior to the bar, noncircular motions dominate the gas kinematics.
A model of the CO kinematics contrains any Inner Lindblad Resonance to be close to the location of the hundred-parsec scale
HCN ‘disk’. At the nucleus, the spatially unresolved CO emission shows a triplet velocity structure characteristic of kinematically
independent regions.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
35.
《Planetary and Space Science》2002,50(9):871-876
C10H6-Fe+ complexes were observed by Fourier transform mass spectrometry by Marty et al. (Chem. Phys. Lett. 256 (1996) 669). In this article, we present the infra-red (IR) spectra of the two isomers calculated by ab initio methods of quantum chemistry. In the past, the same approach has predicted successfully unexpected features of the IR spectra of polycyclic aromatic hydrocarbon (PAH) cations which were confirmed by measurements in matrices (J. Phys. Chem. 98 (1994) 9187). The C10H6-Fe+ systems are models for larger PAHs-Fe+ complexes, which are believed to play a key rôle in space chemistry. 相似文献
36.
根据关联指数的定义,推导了GP法计算关联指数时的观测数据误差与关联指数误差的关系,导出了任意两个嵌入空间维上关联指数之差的表达式,并提出了一种确定样本容量限的方法。 相似文献
37.
讨论关于回转椭球静态场求解的一般方法,借助回转椭圆坐标系,静态场问题的一般解可以用实宗量和虚宗量勒让德函数以及余弦函数形式表出,使得结果更为简明和系统化。所得结果可以直接应用到椭球导体电场、尖端效应、介质椭球极化以至双极化雷达测量降水问题等,具有相当具体的实用价值。 相似文献
38.
39.
干旱区水资源约束下的生态退耕空间优化及权衡分析——以奇台县为例 总被引:1,自引:0,他引:1
干旱区耕地大规模扩张导致水资源超载、生态问题频发,亟须退地还水。因此,探索水资源约束下的生态退耕空间优化方案,不仅有助于解决干旱区面临的问题,还可为土地利用规划和决策提供参考。目前对退耕方案多效益矛盾的研究尚量化不足,有鉴于此,本文建立生态退耕空间优化配置及权衡分析模型,以新疆奇台县为研究区进行模型应用,构建了水资源约束下的生态退耕方案群,并设计保有耕地优先和保护生态优先等两种情景,利用蚁群优化算法实现了生态退耕的空间配置模拟与优化。结果表明:耕地面积在保有耕地优先情景将减至9.94万hm2,保护生态优先情景则为6.96万hm2;在此退耕过程中,河道内生态用水占水资源总量的比例从10%增加到30%,防固沙量由713.22万t增加至816.59万t,经济效益则由34.86亿元下降至24.75亿元。通过比较单位经济效益的减少比例可产生的生态效益增加比例,确定耕地面积退至8.35万hm2时是权衡生态和经济效益下的生态退耕最优方案。退耕还草主要发生在奇台县耕地集中区的东北、西北及西南部边缘,将有利于北部的沙漠化防控和南部的水源保护。本研究实现了干旱区水资源约束下生态退耕方案空间模拟和优化,对农业经营和生态保护具有重要参考意义。 相似文献
40.