南印度洋偶极子的变化特征及其与ENSO事件的联系

利用Hadley Center逐月海温资料以及NCEP/NCAR逐月风场、海平面气压场等资料探讨了南印度洋偶极子(Southern Indian Ocean Dipole,SIOD)的变化特征及其与ENSO事件的联系。结果表明:1)发生在南半球副热带印度洋地区的海温异常西南—东北反相的南印度洋偶极子现象,具有明显的季节锁相特征:10—12月发生发展,次年1—3月发展成熟达到盛期,4—6月减弱消亡;SIOD的形成主要受大尺度大气环流的影响,马斯克林高压以及澳大利亚低(高)压位置和强度的变化引起的副热带印度洋海表面风场的异常,影响了海温的变化,进而形成SIOD。2)南半球副热带印度洋地区的海温变化与赤道中东太平洋地区海温异常密切联系,前冬ENSO事件与SIOD有显著的负相关关系,大多数正SIOD发生在La Ni?a事件之后,大多数负SIOD发生在El Ni?o事件之后;也存在部分SIOD事件的发生既不伴随La Ni?a现象,也不伴随El Ni?o现象。3)ENSO事件产生的异常垂直运动和赤道异常纬向风对南半球副热带印度洋地区的海平面气压以及海表面风场的强度和位置的变化有重要作用,可以分别影响SIOD东西极子的演变,进而对SIOD产生影响。4)SIOD事件也可单独发生,一般负事件比正事件早一个月发生,同时由于没有ENSO事件的作用,海温异常反相的现象不能持续,单独发生的SIOD事件生命期较短。     

海洋再分析资料中IOD-ENSO遥相关的海洋通道机制分析

本文利用滞后相关分析,研究了海洋再分析资料（SODA、ORAS4和GODAS）中的IOD-ENSO滞后遥相关关系,并与观测资料进行对比。结果显示,3套再分析资料中热带东南印度洋秋季海表温度/海表高度异常和赤道太平洋冷舌次年秋季海表温度/海表高度异常之间显著相关,与观测结果一致。在次表层,观测和再分析资料均显示,热带东南印度洋秋季海表温度异常与赤道太平洋次表层海温异常之间的显著相关关系在冬季至次年秋季沿赤道太平洋垂向剖面向东移动,并于次年夏季和秋季在冷舌区上升至海表。热带东南印度洋和赤道太平洋冷舌滞后1年的相关关系是由海洋通道机制引起的,即IOD事件引起印尼贯穿流流量异常,导致赤道太平洋温跃层异常,激发赤道Kelvin波向东传播,从而影响赤道中-东太平洋冷舌海表温度异常。观测及SODA与ORAS4资料中,热带东南印度洋和赤道太平洋冷舌滞后1年的相关关系在去除ENSO信号后仍然显著,表明海洋通道机制是独立于ENSO事件的;而在GODAS资料中,这些显著相关关系在去除ENSO信号后消失。印尼贯穿流流量异常和Niño3.4及DMI（Dipole Mode Index）指数之间超前-滞后12个月的相关关系显示,在SODA和ORAS4资料中,印尼贯穿流流量同时受到ENSO和IOD的影响,与观测结果一致;而在GODAS中,印尼贯穿流流量异常仅与Niño3.4指数显著相关,极少受到IOD事件的影响,这部分解释了GODAS资料中去除ENSO信号后,IOD-ENSO滞后遥相关关系消失的原因。     

Teleconnection of IOD signal in the upper troposphere over southern high latitudes

Evidence has been found for the teleconnection of Indian Ocean Dipole mode (IOD) events in the southern high latitude sea surface pressure field, although the mechanisms that might lead to such far-reaching links remain unresolved. Based on the teleconnection pattern between IOD and the climate anomaly in the upper troposphere, we propose one such mechanism here: the energy propagation theory of the atmospheric planetary wave. Ray traces of the atmospheric planetary waves suggest that the energy propagation of the waves could be responsible for the teleconnection between IOD and tropospheric climate anomalies in southern high latitudes.     

Climate anomalies in the southern high latitudes associated with the Subtropical Dipole Mode

1　Introduction EnoughhasbeensaidabouttheteleconnectionofENSO(ElNi o SouthernOscilla tion)inthetropicalPacificOceanandtheclimateinthesouthernhighlatitudes(Fletcher etal.1982;SmithandStearns1993;SimmodsandJacka1995;Liuetal.2002;Kwok andComiso2002).Inres…     

偶极子假设引起的大回线源瞬变电磁响应偏差分析

偶极子假设下的场点近似解与场点的瞬变电磁精确解存在一定的误差,文中对偶极子假设引起的误差进行了探索性研究.首先分析了由恒定电流偶极子公式“比拟”出的谐变偶极子位函数解.分别计算了静态场中磁偶极子和电偶极子的近似解与各自对应的未做偶极子假设的电流环和载流导线的精确解之间的误差值,然后分析了谐变偶极子微元与点电荷微元的误差...     

NUMERICAL SIMULATION OF THE INFLUENCE OF INDIAN OCEAN DIPOLE ON CLIMATIC VARIATIONS OVER EAST ASIAN MONSOON REGION DURING EQUATORIAL EAST PACIFIC OCEAN SSTA

1 INTRODUCTION In the recent years, more and more researches have shown that the effect of Tropical Ocean is very evident in the process of ocean-air interaction; Sea-Surface Temperature Anomaly (SSTA) takes on global configuration and SSTA in different areas are interrelated and also have their respective characteristics. The SSTA over Indian Ocean and Pacific Ocean are interrelated. WU et al.[1] and MENG et al.[2] indicated that the evident positive correlation of inter-annual…     

地磁场长期变化速率的30年周期

地球主磁场B和它的长期变化都起源于地球外核的磁流体发电机过程，但是，它们的空间结构和时间演化特征却有很大差异. 本文采用全球平均的“无符号年变率”X〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、Y〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、Z〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗、H〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗和F〖DD(-*3〗〖KG*2/3〗·〖DD)〗〖DD(-*2〗〖KG*2/3〗—〖DD)〗来表征长期变化场〖WTHX〗〖AKB·〗〖WTBZ〗的总体强度，利用第9代国际参考地磁场模型IGRF 9，研究〖WTHX〗〖AKB·〗场的变化特征. 结果表明，在1900～2000年的100年当中，〖AKB·〗场经历了3幕变化，最大年变率分别发生在1910～1920、1940～1950、1970～1980年，显示出清晰的30年周期变化，而且，每一周期的上升段比其下降段短得多. 研究结果还表明，非偶极场对〖AKB·〗的贡献约为偶极场的2倍，因此，决定〖AKB·〗场周期特征的主要因素是非偶极场（特别是四极子场），而不是偶极子场. 这一特点与主磁场B〖WTBZ〗中偶极场占绝对优势的特点完全不同.     

The influence of Indian Ocean Dipole (IOD) on biogeochemistry of carbon in the Arabian Sea during 1997–1998

Data on ocean color chlorophylla (Chl a) obtained using Sea-viewing Wide Field of view Sensor (SeaWiFS), sea surface temperature (SST) by Advanced Very High Resolution Radiometer (AVHRR), and sea surface height (SSH) by TOPEX/POSEIDON were analyzed to examine the influence of Indian Ocean Dipole (IOD) on the physical and biogeochemical processes with special reference to phytoplankton primary production and air-sea fluxes of carbon dioxide in the Arabian Sea. Positive SST anomalies (SSTA) were found in the Arabian Sea (0.4 to 1.8°C) with higher values in the southwestern Arabian Sea that decreased towards north. The SSH anomalies (SSHA) and turbulent kinetic energy anomalies (TKEA) suggest decreased mixing during the IOD compared to the normal period. Chlorophylla displayed significant negative correlations with SSTA and SSHA in the Arabian Sea. Consistently, Chla showed negative anomalies (low Chl a) during the IOD period which could be due to reduced inputs of nutrients. The photic zone integrated primary production decreased by 30% during the IOD period compared to the normal whereas pCO₂ levels were higher (by 10–20μatm). However, sea to air fluxes were lower by 10% during the IOD period due to prevailing weaker winds. Primary production seems to be the key process controlling the surface pCO₂ levels in the Arabian Sea. In future, the influence of IOD on ecosystem structure, export production and bacterial respiration rates are to be probed throughin situ time-series observations.     

Continuation by integral equation methods: A note on surface integration over the double layer

Upward continuation from a non-level surface may be performed by an integral equation method as shown previously by Bhattacharyya and Chan. Integration over the double layer is often computed using a centroid rule quadrature formula, but under certain circumstances more accurate formulae are required. One such formula may be found using a geometric approach. The result is equivalent to an expression recently published by Hansen and Miyazaki.     

偶极子移动的三种类型

用β平面准地转正压模式,实施了１８组积分时间为４至６个模式日的试验。从偏离偶极子解析解的流型启动,得到了偶极子移动的３种类型,即东进型、西进型和经向型。在一定的参数集合,在涡旋对总体上向外频散能量的同时,偶极子气旋涡旋的强度不但不随时间衰减,而且可以增强。