从地质遥感迈向国土资源普查

概略回顾了中国20世纪遥感地质的辉煌成就,列举4项重大突破:极块构造的论证与线性形迹分析,数字地质与找矿、第四纪地质与地貌学的新发现、工程地质选线与选址。指出21世纪面对国土普查的新任务,需要加强遥感信息机理研究,信息融合与共享,学科交叉,社会经济统计空间分析的能力,关注探月计划与遥感制图。     

土地利用更新调查需要注意的几个问题

以土地利用更新调查生产中的体会．从工作前期准备、技术路线、正射影像图制作、权属界线调查几种特殊情况和表示方法的处理，提出了土地利用更新调查需要注意的几个问题和建议。     

无人机在重大地质灾害应急调查中的应用

传统的地质灾害应急调查受限于地形、天气等外界条件,不能快速全面地获取灾害的详细信息,而无人机具有灵活性强、时效性高和不受复杂地形影响等特点,在地质灾害应急调查中有独特的优势。本文以“6·24”新磨村滑坡和“10·11”白格滑坡为例,阐述了无人机数据获取及处理流程,重点介绍了无人机获取的数字地形产品在地质灾害精确描述、定性及定量分析中的应用。结果表明：无人机摄影测量技术为重大地质灾害应急调查提供了更加科学高效的现场影像采集和遥感成果处理及应用方案,为应急救灾工作的顺利实施及分析研判提供了重要数据支撑,科学有效地保证了现场施工救援人员的安全。     

旋翼无人机载激光雷达在农村不动产权籍调查中的应用

我国越来越重视农村的发展,目前各地都在积极开展农村不动产权籍调查工作,该工作时间紧迫,对数据精度要求较高。在农村不动产权籍调查中,本文针对传统外业全野外调绘所带来的低效率问题,提出了利用旋翼无人机载激光雷达进行调绘的方法,并且通过实例验证了该方法相较于传统测绘方式能够提高测绘的效率且测绘精度符合最终要求。     

基于低空无人机倾斜摄影测量在农村房屋不动产登记权籍调查中的应用

低空无人机倾斜摄影测量技术可以快速获取实景三维影像,具有可量测、现实感逼真、纹理清晰等特点。该技术应用于农村房屋不动产登记权籍调查中,减少了外业实地丈量的工作量,克服了不通视房屋拐点量边的困难,可快速生成数字线划图,通过三维不动产模型可以查看测量三维数据,解决了外业调查耗时费力、界址边丈量人为误差等问题。     

Bayesian foreground analysis with CMB data

The quality of CMB observations has improved dramatically in the last few years, and will continue to do so in the coming decade. Over a wide range of angular scales, the uncertainty due to instrumental noise is now small compared to the cosmic variance. One may claim with some justification that we have entered the era of precision CMB cosmology. However, some caution is still warranted: The errors due to residual foreground contamination in the CMB power spectrum and cosmological parameters remain largely unquantified, and the effect of these errors on important cosmological parameters such as the optical depth τ and spectral index n_s is not obvious. A major goal for current CMB analysis efforts must therefore be to develop methods that allow us to propagate such uncertainties from the raw data through to the final products. Here we review a recently proposed method that may be a first step towards that goal.     

Quantum peculiarities of the primordial hydrogen recombination

Some problems of the two-photon decay of highly excited atomic hydrogen and helium levels are considered. The necessary accuracy of calculating the transition probabilities is shown to require abandoning the purely dipole approximation in the theory of atomic hydrogen radiation. The range of applicability of the perturbation theory to this process is discussed. We suggest a new mechanism of the Lyman photon redistribution due to very close locations of the 20P and 19P levels in the hydrogen and deuterium atoms, respectively (hydrogen-deuterium resonance).     

Constraining the nature of dark energy using the Square Kilometer Array Telescope

We investigate the potential of the Square Kilometer Array Telescope (SKA) to constrain the sound speed of dark energy. The Integrated Sachs Wolfe (ISW) effect results in a significant power spectrum signal when Cosmic Microwave Background (CMB) temperature anisotropies are cross-correlated with galaxies detectable with the SKA in H  i . We consider using this measurement, the autocorrelation of H  i galaxies and the CMB temperature power spectrum to derive constraints on the sound speed. We study the contributions to the cross-correlation signal made by galaxies at different redshifts and use redshift tomography to improve the signal-to-noise. We use a  χ²  analysis to estimate the significance of detecting a sound speed different from that expected in quintessence models, finding that there is potential to distinguish very low sound speeds from the quintessence value.