用前期海温预报四川夏季气温的EOF迭代方案     

李跃清  张波 《成都信息工程学院学报》1996,(4)

应用ＥＯＦ（经验正交函数）迭代方案，考虑多时次历史资料，在全球海区海温与四川盆地气温非同步联系的基础上，以海温为预报因子进行了夏季气温的长期预报。结果表明：西太平洋高温区等关键海区海温的异常对未来四川盆地夏季气温变化有重要影响，由此建立的引入多时次海温的ＥＯＦ迭代长期温度预报方法，具有较强的预报能力  相似文献   

Determination of copper complexation in surface microlayer of Daya Bay and Jiaozhou Bay     

张正斌  刘春颖  于志刚  刘莲生  王肇鼎  宫海东 《中国海洋湖沼学报》2005,23(2):238-245

1 INTRODUCTION Bioavailability to the biota and the biogeo-chemistry of trace metals in marine environment areaffected by their chemical speciation in the naturalsystem (Bruland et al., 1991; Van den Berg andDonat, 1992; Wells et al., 1998). Therefore, thesetwo parameters, the ligands concentrations andconditional stability constants, are important todetermine the complexing capacity. Sea surface microlayer (SML), the thin interfa-cial boundary between ocean and atmosphere, playsan imp…  相似文献   

校院两级管理下的排课软件设计与实现     

肖洪生  陈善雄 《广东海洋大学学报》2005,25(6):65-68

阐述了排课系统的管理层次、操作权限分配、资源管理、网络排课的具体实现过程。本系统较好地解决了多个校区、多个学院之间的分配资源和排课冲突问题。其特点是资源统一管理、分散使用,利用校园网进行教学管理,不受时间、空间的限制。  相似文献   

激光时间传递技术的进展   总被引：4，自引：0，他引：4  

李鑫  杨福民 《天文学进展》2004,22(1):10-22

激光时间传递技术是通过激光脉冲在空间的传播来实现地面与卫星时钟或地球上远距离两地时钟的同步，它具有很高的准确度和稳定度。一些国家已经成功进行了激光时间传递的试验，结果证明利用激光进行时钟之间的同步是有效可行的。介绍国内外已有的激光时间传递试验的情况和结果，重点介绍美国地面与机载原子钟之间的激光时间比对，以及法国的LASSO(LAser Synchronization from Stationary Orbit)和T2L2(Time Transfer by Laser Link)计划。  相似文献   

影响鸢乌贼手钓上钩率的因子探讨     

吴国峰  陈新军 《广东海洋大学学报》2006,26(6):35-38

根据印度洋西北部鸢乌贼(Symplectoteuthis oualaniensis)作业渔场的现场调查数据,分析了作业水深、作业时段、摄食等级和月相等因子对手钓上钩率的影响。统计表明,晚上、午夜和凌晨3个不同时段和不同作业水深对手钓上钩率均有显著性影响。3个时段中,其摄食等级呈先低后高再低的现象。午夜和凌晨,上钩率的变化趋势与摄食等级的变化趋势呈显著的负相关。在月相的影响下,离朔日三四天之前,手钓产量呈上升趋势;离望日五六天之前,手钓产量呈明显的下降趋势。  相似文献   

Geoeffective Analysis of CMEs Under Current Sheet Magnetic Coordinates   总被引：1，自引：0，他引：1  

Xueshang Feng  Xinhua Zhao 《Astrophysics and Space Science》2006,305(1):37-47

Using 100 CME–ICME events during 1997.01–2002.11, based on the eruptive source locations of CMEs and solar magnetic field observations at the photosphere, a current sheet magnetic coordinate (CMC) system is established in order to statistically study the characteristics of the CME–ICME events and the corresponding geomagnetic storm intensity. The transit times of CMEs from the Sun to the Earth are also investigated, by taking into account of the angle between the CME eruption normal (defined as the vector from the Sun center to the CME eruption source) and the Sun-Earth line. Our preliminary conclusions are: 1. The distribution of the CME sources in our CMC system is obviously different from that in the ordinary heliographic coordinate system. The sources of CMEs are mainly centralized near the heliospheric current sheet (HCS), and the number of events decreases with the increment of the angular distance from the CME source to the HCS on the solar surface; 2. A large portion of the total events belong to the same–side events (referring to the CME source located on the same side of the HCS as the Earth), while only a small portion belong to the opposite–side events (the CME source located on the opposite side of the HCS as the Earth). 3. The intense geomagnetic storms are usually induced by the same–side events, while the opposite side events are commonly associated with relatively weak geomagnetic storms; 4. The angle between the CME normal and the Sun–Earth line is used to estimate the transit time of the CME in order to reflect the influence of propagation characteristic of the CME along the Sun–Earth direction. With our new prediction method in context of the CMC coordinate, the averaged absolute error for these 100 events is 10.33 hours and the resulting relative error is not larger than 30% for 91% of all the events.  相似文献   

Modelling residence‐time response to freshwater input in Apalachicola Bay,Florida, USA     

Wenrui Huang  M. Spaulding 《水文研究》2002,16(15):3051-3064

Residence time of an estuary can be used to estimate the rate of removal of freshwater and pollutants from river inflow. In this study, a calibrated three‐dimensional hydrodynamic model was used to determine residence time in response to the change of freshwater input in Apalachicola Bay. The bay is about 40 km long and 7 km wide, with an average 3 m water depth. Through hydrodynamic model simulations, the spatial and temporal salinity and the total freshwater volume in the bay were calculated. Then the freshwater fraction method was used to estimate the residence time. Results indicate that the residence time in Apalachicola Bay typically ranges between 3 and 10 days for the daily freshwater input ranging from 177 m³/s to 4561 m³/s. Regression analysis of model results shows that an exponential regression equation can be used to correlate the estuarine residence time to changes of freshwater input. Copyright © 2002 John Wiley & Sons, Ltd.  相似文献   

中国地壳运动观测网络基准站GPS观测的位移时间序列结果   总被引：32，自引：9，他引：23  

顾国华  张晶 《大地测量与地球动力学》2002,22(2):61-67

对中国地壳运动观测网络基准网于1998年9月－2001年10月GPS连续观测结果所获得的位移时间序列进行了初步分析，讨论了适用于地震分析预报的位移时间序列生成中的基准选择。选东部长期相对水平位移很小的9个站组成的一组稳定点作为基准，得到水平位移时间序列；选分布于不同区域相对垂直位移较小的7个站为稳定点组，得到垂直位移时间序列。2000－2001年我国西部的基准站出现2次明显的水平与垂直位移异常变化，这种异常变化有可能与南北地震带上云南地区发生的6级左右地震活动有一定的关系。  相似文献   

罗兰C自主TOC同步的研究     

吴海涛  边玉敬  李志刚 《时间频率学报》2002,25(1):1-8,17

研究了罗兰C自主实现TOC同步的原理。根据TOC的特点 ,分析了罗兰C自主TOC同步的基本要求。定义了TOC信息的概念 ,提出了一种新的信息类型和相应的通信规约。分析了GRI脉冲序列与参考脉冲 ,以及调制码组与罗兰C脉冲组的时间关系。最后详细研究了在连续传输 (TOC信息和DGNSS交替 )方式下TOC同步的原理和方法。  相似文献   

毫秒脉冲星定时研究进展   总被引：1，自引：0，他引：1  

杨廷高  潘炼德  倪广仁  柯熙政 《天文学进展》2002,20(2):167-174

毫秒脉冲星守时的理论和方法研究己取得重要进展,利用现有2颗毫秒脉冲星约10yr的计时观测资料分析得到的 TAI-PT,其长期稳定度为 2×10－14。采用合适的长期稳定度算法,由多颗毫秒脉冲星计时观测可以建立综合脉冲星时间尺度。它可以成为与原子时系统比较的重要手段,并对原子时长期稳定度的改进做出贡献。介绍了该领域研究的基本状况,重点对毫秒脉冲星守时的理论方法,综合脉冲星时间及与原子时的关系等进行了讨论和评述。对由双星系统内毫秒脉冲星的轨道运动定义的双星脉冲星时也做了介绍。  相似文献