遥感技术在西北生态脆弱区生态地质勘查中的应用研究

生态地质勘查正在成为煤炭地质勘查工作的主要发展方向。遥感技术作为“非接触式”勘查技术,在生态地质勘查中应有一席之地。通过阐述遥感技术在煤炭、天然气水合物、油页岩等资源勘查中的工作程序及勘查实例,认为在西北生态脆弱区资源勘查领域遥感技术具有独特的优势:通过不同比例尺的遥感煤田地质填图,可快速高效圈定含煤远景区;利用遥感图像的热红外波段数据可以快速获取与水合物相关的温度异常信息,圈定热异常分布区,为天然气水合物进一步勘探指明方向;通过对遥感图像的处理可直接提取与油页岩相关的成矿异常信息,圈定找矿远景区。在西北生态脆弱区应用遥感技术进行资源勘查具有好的经济效益和生态效益。     

An optimal extraction algorithm for imaging photometry

This paper is primarily an investigation of whether the 'optimal extraction' techniques used in CCD spectroscopy can be applied to imaging photometry. It is found that using such techniques provides a gain of around 10 per cent in signal-to-noise ratio over normal aperture photometry. Formally, it is shown to be equivalent to profile fitting, but offers advantages of robust error estimation, freedom from bias introduced by mis-estimating the point spread function, and convenience. In addition some other techniques are presented, which can be applied to profile fitting, aperture photometry and the 'optimal' photometry. Code implementing these algorithms is available at http://www.astro.keele.ac.uk/~timn/.     

High-resolution bispectrum speckle interferometry and two-dimensional radiative transfer modeling of the Red Rectangle

We present the first diffraction-limited K-band image of the Red Rectangle with 76 mas resolution, an H-band image with 75 mas resolution, and an RG 715 filter image ( 800 nm wavelength) with 78 mas resolution (corresponding to 25 AU for a distance of 330 pc). The H and K images were reconstructed from 6 m telescope speckle data and the RG 715 image from 2.2 m telescope data using the speckle masking bispectrum method. At all wavelengths the images show a compact, highly symmetric bipolar nebula, suggesting a toroidal density distribution of the circumstellar material. No direct light from the central binary can be seen as it is obscured by a dust disk or circumbinary torus. Our first high-resolution H−K color image of the nebula shows a broad red plateau of H−K≈ 2^m in the bright inner regions.The optical and near-infrared images and the available photometric continuum observations in a wide range of ultraviolet to centimeter wavelengths enabled us to model the Red Rectangle in detail using a two-dimensional radiative transfer code. Our model matches both the high-resolution images and the spectral energy distribution of this object very well, making the following picture much more certain. The central close binary system with a total luminosity of 3000 L is embedded in a very dense, compact circumbinary torus which has an average number density n_H ≈5×10¹² cm⁻³, an outer radius of the dense inner region of R≈30 AU (91 mas), and a ρ∝r⁻² density distribution. The full opening angle of the bipolar outflow cavities in our model is 70°. By comparing the observed and theoretical images, we derived an inclination angle of the torus to the line of sight of 7°±1°.The radiative transfer calculations show that the dust properties in the Red Rectangle are spatially inhomogeneous. The modeling confirms that the idea of large grains in the long-lived disk around the Red Rectangle (Jura et al., 1997 [ApJ, 474, 741]) is quantitatively consistent with the observations. In our models, unusually large, approximately millimeter-sized grains dominate the emission of the compact, massive torus. Models with smaller average grain sizes can possibly be found in future studies, for instance, if it turns out that the radio spectrum is not mainly caused by continuum dust emission. Therefore, the large grains suggested by our models require further confirmation by both new observations and radiative transfer calculations. Assuming a dust-to-gas ratio ρ_d/ρ_g of 0.005, the dense torus mass is 0.25 M. The model gives a lower limit of 0.0018 M, for the mass of the large particles, which produce a gray extinction of A≈ 28^m, towards the center. A much smaller mass of submicron-sized dust grains is presumably located in the polar outflow cavities, their conical surface layers, and in the outer low-density parts of the torus (where ρ∝r⁻⁴, in the region of 30 AUr 2000 AU corresponding to 0.^′′09–6^′′).     

遥感支持下的景洪巴卡少数民族土地利用空间变化研究

土地利用是人类活动最直观的反应,人地关系是影响环境变化的主体因素,是制定区域可持续发展、实施生物多样性保护的内核;航空航天遥感（ＲＳ）从时间和空间上扩大了人们的视野,是监测自然因素和人为作用所引起森林植被及土地利用动态变化的有力、高效的手段。在ＲＳ技术支持下,采用不同年代、不同分辨率、不同比例尺,时间跨度为３０年的航空航天遥感,对热带雨林景洪巴卡土地结构及变迁进行分析研究,探索森林土地空间动态变化对土地利用、可持续发展的影响,对区域环境的影响等,为当地政府提供决策依据。     

绍兴市城镇用地扩展的遥感监测

随着我国改革开放政策的实施,绍兴市的经济得到飞速发展,城市规模迅速扩大。城市扩展趋势如何,土地的开发利用现状如何是制定今后土地利用规划,进行土地管理、开发的重要依据。为此绍兴市土地局开展了以TM影像为基本信息源的城镇遥感监测工作,本文对此工作进行了分析探讨。     

航天遥感技术在叶尔羌河中下游地区Au、Cu等多金属矿找矿有利地段预测中的应用研究

板块构造成矿理论认为西昆仑叶尔羌河中下游地区属于Ａｕ、Ｃｕ及多金属矿成矿远景区,但因其野外地质条件恶劣,交通状况差,地质勘探极其困难而影响了找矿工作的深入开展,为此我们利用航天遥感技术的优势进行了找矿有利地段预测研究。在研究中首先对区域地质遥感影像特征进行了综合分析,并根据板块构造成矿理论对矿化作用进行了空间划分和成矿条件总结。在此基础上,通过成矿相关影像特征信息的提取,圈定出Ａｕ、Ｃｕ及多金属矿成矿有利地段。     

多覆盖地区花岗岩接触带及其控矿特征的遥感研究

本文主要介绍应用TM图像对西秦岭地区的中川岩体进行研究的成果,即研究在多植被、多黄土覆盖的复杂条件下,如何依据接触带蚀变岩的遥感图像像元亮度值及实验室测得的光谱曲线特征,区分不同的岩体接触带类型,并探讨它们对金矿的控制作用。     

大比例尺卫片在土地利用动态变化监测中的应用——以黑龙江省阿城监测区为例

以黑龙江省阿城市为监测试验区,采用1:5万的TM假彩色合成图像,对该市土地利用现状进行解译调查,并与历史资料比较,对该市土地利用动态变化情况进行监测,同时对这种方法的可行性和该市地类变化情况以及监测结果进行了分析。     

应用遥感图像提取煤层自燃信息时必须考虑的几个影响因素

煤层自燃是中国北方煤田中普遍存在的灾害现象,它不但烧掉了大量的煤炭资源,而且还污染了环境。实践证明,利用遥感影像判别火区位置、圈定火区范围和对火区进行动态监测,及时为灭火工程提供信息,是一项经济和社会意义很大的工作。由于受多种因素的制约,不同地区、不同波段、不同时相、不同空间分辨率的遥感图像,其影像特征（含与煤层自燃有关的热异常影像特征）都有较大的差异,因而从图像上分析和提取地物的热红外辐射特征时,需要考虑遥感图像类型、成像时间、地形条件、气象条件和岩性特征等因素的影响。本文着重讨论了地表辐射温度与上述各项因素之间的关系。     

利用遥感和GIS研究塔里木河下游阿拉干地区土地沙漠化

新疆塔里木河流域受人类活动的影响,特别是由于水资源利用的不合理,不同区域出现了一系列生态环境问题,下游地区普遍存在的沙漠化现象表现得尤为突出。通过应用多时相（１９５９年、１９８３年、１９９２年）、多波段、多平台的遥感信息,在野外调研的基础上编制阿拉干地区不同年代沙漠化类型图,并在ＡＲＣ／ＩＮＦＯ软件支持下,对图件进行编辑处理,制作沙漠化动态图;通过ＧＩＳ数据库提供的资源环境定量数据,应用系统论、信息论及控制论的观点分析阿拉干地区沙漠化的演化过程,并借助于ＧＭ（１,１）模型,预测阿拉干地区土地沙漠化的发展趋势。