略论海洋测高卫星GPS厘米级定轨的实施基础

基于对多种飞机的机载GPS测量实践,认为我国HY-2海洋二号卫星实现厘米级精度的星载GPS定轨测量的基础是:选择适合天线,捕获多颗在视GPS卫星;注重天线安装位置,减弱多路径效应影响;选择适合GPS信号接收机,确保星载GPS测量数据优质。     

Research on Autonomous Orbit Determination of Navigation Satellite Based on Crosslink Range and Orientation Parameters Constraining

Introduction Thepotentialvulnerabilityofsatellitenaviga tionsystemthatreliesongroundstationsisthat thesystemwouldbreakdownifgroundstations weredestroyed,whichcannotmeettherequire mentofnavigationwarfare[1].Withthedevelop mentofsuchspace basedsystemsasgrou…     

基于混合回归模型的夏季高温日数预测

本文以变化比较激烈的高温日数为对象,通过加权叠加、周期波动以及尺度比较等理论分析提出一种短期气候预测观点,即长周期波动可用当地前期各种气象要素的长周期波动的某种函数表示,而短周期波动依然与大范围周边环境因子的变化有关。采用功率谱分析、逐步回归、方差分析等常用统计手段和二项式平滑方法,建立长周期波动和波动偏差比的预报方程,在此基础上得到高温日数的预报方程。应用该方法对合肥地区的高温日数进行了预测试验,利用滚动预报得到13个预报样本。在13个试测样本中,有11个样本试测较为准确,试测准确率达到84．6％。在试测不准确的2个样本中,误差有5～6d,而且它们出现在高温日数相对较多的年份,因此试测效果令人满意。     

江淮入梅前后气象因子变化特征及预报着眼点探析

针对2010年江淮地区入梅日预报偏差情况,利用2010年6—7月高低空实况资料和NCEP再分析资料,分析了入梅前后湿度、经向风、地转西风急流的变化特征,并结合1985—2005年21 a历史平均状况和近几年的变化特征,分析了江淮地区入梅前后气象因子变化的规律性、普遍性,丰富了江淮地区入梅预报着眼点。研究发现:有些年份地转西风急流从30°N以南北跳到30~37.5°N区域,对江淮地区进入梅雨期有很好的预示作用,且其稳定维持,有利于江淮梅雨期降水的持续。70%湿度区北跳到30°N的时间及持续时间对江淮地区入梅日的预报和梅雨期长度有着较好的指示作用。在30~35°N区域内v850 hPa-v200 hPa风速差值的突然增大和江淮地区入梅有着较好对应关系。这为梅雨的预报提供了新的思路和方法。     

高应力区破裂岩体回采巷道一次强化支护技术及其应用研究

基于对高应力区破裂岩体回采巷道支护 10多年的经验和教训 ,本文首次提出了相对于主次承载区协调作用关系的关键支护技术 ,即一次强化支护技术。该支护技术不仅强调了对于高应力区破裂岩巷道支护时间的及时性 ,支护强度一次到位 ,更重要的是区别于先让后抗、二次支护的指导思想 ;同时 ,一次强化支护技术还详细明确了支护类型、支护结构以及施工工艺。该支护技术在小官庄铁矿高应力区的应用成功 ,表明该支护关键技术是正确的。     

Intrusion and its implication for subsidence: A case from the Baiyun Sag, on the northern margin of the South China Sea

We develop a series of simple numerical models to explain the anomalous subsidence and deposition phenomena on the northern continental margin of the South China Sea, in particular in the Baiyun Sag. The results suggest that a short-period high rate deposition of around 17 Ma is related to a rapid subsidence event, which may be due to episodic emplacement of a dense intrusion. Necking and gravity models indicate that in the basement of the Baiyun Sag, there is a dense zone that is 100–200 kg/m³ more dense than the surrounding country rock. Considering its high magnetic intensity and regional igneous activity, the dense zone is thought to be related to a phase of basalt intrusion that may have taken place around 17 Ma. Thermal and subsidence models indicate that a hot denser intrusion can cause significant subsidence immediately after the intrusion. The subsidence rate then slows down with cooling, thus becoming consistent with the observed subsidence curves at around 17 Ma. The results also indicate that the lithospheric strength under the Baiyun Sag is negligible, and that the high-velocity layer in the lowermost crust may be not an original part of the pre-rift crust. Instead, it is thought to be underplated intrusion emplaced at around 30 Ma when the continental margin broke up.     

1997年昆明日偏食射电快速过程的观测

介绍了１９９７年３月９日昆明日偏食过程中云南天文台四波段射电高时间分辨率同步观测结果,通过掩食和露放黑子前后射电快速起伏率的变化现象,推测日冕缓变源存在电子加速过程,它可能对射电快速起伏率的增强有贡献。     

On the motion around the centre of mass of a viscously elastic sphere in the restricted elliptic three-body problem

In the restricted three-body problem we consider the motion of a viscously elastic sphere (planet) with its centre of mass moving in a conditionally-periodic orbit. The approximate equations describing the rotational motion of the sphere in terms of the Andoyer variables are obtained by the method of the separation of motion and averaging; the evolution of the motion is also analysed.     

Symmetries and Rank Deficiency in the Orbit Determination Around Another Planet

We study the possible degeneracies for the normal matrix of the observations from the Earth of the motion of a satellite around a planet, and give the possible solutions to the loss of precision in the orbit determination caused by the rank deficiency. Finally we discuss the methods available to control the instability in the orbit determination resulting from the degeneracy.     

由土卫九(Phoebe)轨道数值改进求解土星质量

为测定土星质量,对收集到的1905年至2006年期间的686次观测[其中包括182次照相观测和504次CCD(电荷耦合器件)观测]通过数值积分进行拟合来改进土星的暗弱的外卫星Phoebe的轨道,并得到土星系总质量msa的新的测定值:3 497.0-1msun(太阳质量),为更精确地测定土星质量提供了一个有价值的参考值。