Noise reduction methods in the analysis of near infrared lunar occultation light curves for high angular resolution measurements

A lunar occultation （LO） technique in the near-infrared （NIR） provides angular resolution down to milliarcseconds for an occulted source, even with ground- based 1 m class telescopes. LO observations are limited to brighter objects because they require a high signal-to-noise ratio （S/N ~40） for proper extraction of angular diameter values. Hence, methods to improve the S/N ratio by reducing noise using Fourier and wavelet transforms have been explored in this study. A sample of 54 NIR LO light curves observed with the IR camera at Mt Abu Observatory has been used. It is seen that both Fourier and wavelet methods have shown an improvement in S/N compared to the original data. However, the application of wavelet transforms causes a slight smoothing of the fringes and results in a higher value for angular diameter. Fourier transforms which reduce discrete noise frequencies do not distort the fringe. The Fourier transform method seems to be effective in improving the S/N, as well as improving the model fit, particularly in the fainter regime of our sample. These methods also provide a better model fit for brighter sources in some cases, though there may not be a significant imorovement in S/N.     

Numerical investigation of the control factors driving Zhe-Min Coastal Current

During the northeast monsoon season, Zhe-Min Coastal Current(ZMCC) travels along the Chinese mainland coast and carries fresh, cold, and eutrophic water. ZMCC is significantly important for the hydrodynamic processes and marine ecosystems along its path. Thus, this bottom-trapped plume deserves to be further discussed in terms of the major driving factor, for which different opinions exist. For this purpose, in this study, a high resolution Semi-implicit Cross-scale Hydroscience Integrated Syste...     

核爆炸与地震识别研究进展

综述了近年来核爆炸与天然地震识别研究的进展, 揭示了从频谱比、震级比到综合因素的概率方法的发展过程, 特别指出小当量核爆炸识别的重要性. 文章借助量子场论和相变理论分析讨论了地震波波长与动量的关系. 同时, 根据地壳介质的复杂性, 指出地震波传播过程中由于介质的非线性与弥散的联合作用, 导致产生孤波的可能性.     

天球有效大气角动量中的周年和半年项估计

为了讨论大气对非刚体地球章动周年和半年项的贡献,本文将大气有效角动量(1980.0～1998.33)从地面参考系转换至空间参考系得到大气的天球有效角动量CEAM,低通滤波后用最小二乘方法拟合得到顺、逆向周年和半年项的振幅估计。     

由地球自转的年际变化预测El Nino事件

分析了地球自转、大气角动量和太阳黑子相对数的年际变化与Ｅｌ Ｎｉｏ的关系。结果表明：当地球自转速率的年际变化由快向慢转变,即表示年际变化的△ＬＯＤ１的数值由极小逐渐增加并转变为正值约半年后,Ｅｌ Ｎｉｏ的初期开始出现。此期间大气角动量的年际变化也呈现从小到大的过程。通过分析新的地球自转变化测值,预测２００１年将出现Ｅｌ Ｎｉｏ。结果还表明Ｅｌ Ｎｉｏ可能与太阳活动有一定的关系。     

近相接双星室女座BF的轨道周期变化

收集了近相接双星ＢＦ Ｖｉｒ的光极小时刻,并对其轨道周期进行分析。结果表明该星的轨道周期在长期减小的财时也含有３０年的周期性变化,对引起轨道周期变化的各种物理机制的分析研究表明：一个质量为０．２８１Ｍ⊙、绕公共质心的轨道半径为１０．２ＵＡ的第３天体的存在能对轨道周期的周期性变化成份作出解释,如果轨道周期的周期性变化成份是由于次子星的周期性磁活动引起,那么系统总光度就应该有振幅０．０９７Ｌ⊙的周期性     

A note on Earth's rotation angular velocity in the general-relativity framework

 The value of the Earth's rotational angular velocity determined from observations is given in the GCRS (geocentric celestial reference system) defined by Resolution B1 of the 2000 IAU General Assembly. The same quantity derived from dynamical theories of the Earth's rotation, such as SMART97, is referred to the␣DGRSC (dynamically non-rotating ecliptical reference system). The relativistic theory of reference systems (RSs) enables unambiguous general-relativity relations between these quantities to be derived. Received: 9 November 2000 / Accepted: 9 July 2001     

卫星遥感结合地面资料对区域表面动量粗糙度的估算

利用地面湍流观测资料估算了黑河实验区几个典型下垫面的局地地表动量粗糙度，与卫星观测Landsat TM资料相结合得到了由标准化差值植被指数(NDVI)计算地表动量粗糙度的经验关系式，进而估算了实验区夏季和近冬季的地表粗糙度的区域分布，并对所得关系式进行了合理性检验。