《明天历》日食算法分析

目的用数学公式将《明天历》的日食算法表达出来,并指出其天文学意义。方法文献分析与数学建模。结果《明天历》先求得合朔时交点离开冬至点的距离以及太阳到冬至点的距离,两者的差值就是"去交度分";常数中的"朔差"是一个朔望月中交点退行的距离;它以恒星年而不以回归年入算以及用太阳的去交分代替月亮的去交分都是其去交度分算法的不足之处。《明天历》的食甚时刻仅是对经朔时刻加入日月不均匀运动有关的修正,没有进行时差的修正。其他算法与主流算法基本相同。结论《明天历》的日食算法在宋代是比较特殊的,这些特殊之处大部分是正确的、合理的,但某些算法中仍存在不足。     

古代巴比伦塞琉古王朝时期食分算法初探

目的 探讨古代巴比伦塞琉古王朝时期(312B．C．-64B．C．)食分算法的合理性。方法 将古代巴比伦的食分算法与现代天意义下的食分算法进行比较。结果 给出了古代巴比伦的食分算法的几何解释；证明了古代巴比伦对食分的定义和现代天学关于食分的定义等价；证明了古代巴比伦的食分算法和北魏张龙祥《正光历》(522A．D．)推月食食分的算法形异实同；在巴比伦的食分算法模型下，求出了日月食限，分析了食分和食限所达到的精度。结论 古代巴比伦食分算法的数学模型是合理的，在此理论支持下所计算出的食分和食限是比较精确的。     

DHT网络eclipse攻击

分布式Hash表(distributed Hash table,DHT)是结构化对等网络的核心技术。实际P2P应用中,DHT网络规模已经达到上千万节点,但是其安全问题仍然很多。eclipse攻击是DHT网络中典型的安全威胁之一。本文介绍了DHT网络中eclipse攻击常见的攻击方法,总结归纳了近年来攻击检测和防御技术的研究工作进展,从适用场景、依赖条件和性能等方面对这些工作进行了对比分析,最后对未来的研究工作进行了展望。     

日月食限的计算

日月食的观测对太阳物理学、天文学及其它相关学科的研究有重要意义．然而准确的日月食预报却离不开日月食限的计算．本文研究了日月食计算方法，力求简单易懂，以便于课堂教学和进行科普教育．     

Gravity anomaly during the Mohe total solar eclipse

By using a high-precision LaCoste-Romberg (D-122#) gravimeter, continuous and precise measurements were carried out during the March 9, 1997 total solar eclipse in the Mohe region in Northeast China. The gravity variations were digitally recorded during the total solar eclipse so as to investigate the possible anomaly of the sun and the moon’s gravitational fields on the earth. After the careful processing and analysis of the observed data, no significant anomaly during the very solar eclipse has been found. However, there are two ‘gravity anomaly valleys’ with near symmetrical decrease of about 6–7 μGal at the first contact and the last contact. This is the anomaly phenomenon observed and reported for the first time in the literature. This note presents some analyses and discussions.     

日月食观测在科学研究上的意义

阐述了日月食观测在研究太阳大气结构、太阳活动，寻找近日彗星和水内行星，检验广义相对论理论以及校正历史中年日次序诸多方面的价值．     

基于Landsat8的世界各国南极内陆考察特征分析

利用南极地区夏季Landsat 8卫星短波红外影像获取近年世界各国南极内陆考察车辙印、机场跑道、中转站等考察足迹信息.一方面,深入分析我国南极考察内陆考察路线特征,并通过相邻3个年度南极考察内陆考察轨迹对比了解考察轨迹的变化特点;另一方面,对比分析世界各国内陆考察起止点、中转站和路线轨迹差异,并结合南极冰上、冰下地形数据,冰雪积累率和冰流速等辅助数据,探索各国南极考察路线特征,通过对各国南极内陆考察活动和路线断面特征的对比分析,了解世界各国的极地考察水平.     

Tomographic Study of Ionospheric Effects Associated with a Solar Eclipse

This paper studies the ionospheric effects associated with the solar eclipse of October 24th, 1995 by means of Computerized Ionospheric Tomography (CIT). Since the reconstructed profiles from experimental CIT are sporadically located in time, a time domain interpolation method based on Singular Value Decomposition (SVD) technique is proposed and applied to extract the ionospheric effects. The effects can be extracted by comparison analysis between the interpolated CIT profiles of the eclipse days and that of the reference day that are time-aligned. A series of figs have been obtained showing the attenuation of photonization effect at low altitudes and the weakening of plasma's transportation process at high altitudes, etc. The photonization effect recovered to normal level soon after the last contact. The maximum electron density diminishing is observed about 2 h after the eclipse maximum and the effects seem vanished in the hours followed. Analysis on vertical TEC's latitudinal-temporal variation gives     

Variation properties of ionospheric eclipse factor and ionospheric influence factor

The concepts and calculation methods of ionospheric eclipse factor (IEF) and ionospheric influence factor (IFF) are further illustrated. The temporal an d spacial variation properties of IEF and IFF are studied, which shows that the properties are influenced by the geographic position and season. The possibility of improving the precision of using GPS data to determine ionospheric delay bas ed on the above variation properties is also analysed.