孟加拉湾障碍层年际变化及其与印度洋偶极子事件的联系

利用1980?2015年SODA温盐资料，结合Argo数据分析了印度洋偶极子(IOD)事件年份孟加拉湾障碍层的变化特征及其形成机制。结果表明，IOD事件年份孟加拉湾障碍层变化显著。纯的正IOD(纯pIOD)年份及伴随型pIOD年份盛期(9?11月)，除孟加拉湾内西南海域障碍层厚度略变厚约5 m外，赤道海域、安达曼海至孟加拉湾北部障碍层厚度均变薄5～15 m，此障碍层距平盛期形态在纯pIOD年份随pIOD消亡迅速消退，但在伴随型pIOD年份维持至翌年3?5月才开始弱化。纯的负IOD (纯nIOD)年份障碍层厚度变化特征与pIOD年份大体相反。进一步分析表明，IOD事件年份赤道风场距平的远地强迫造成等温层深度的变化是湾内障碍层变化的主因。在伴随型IOD年份，受ENSO事件的影响，赤道风场距平在IOD消亡后仍得以维持3个月以上，使得湾内障碍层距平形态持续更久。除赤道远地强迫外，湾内局地风场的Ekman抽吸作用以及混合盐度变化对障碍层厚度年际变化也有一定影响。     

印度洋—西太平洋对流涛动的季节内特征

本文利用30~60天带通滤波资料, 考察了不同季节印度洋—西太平洋区域对流活动季节内尺度变率的主要模态, 发现在不同季节赤道东印度洋(5°S~10°N, 70°E~100°E)和西北太平洋(5°N~20°N, 110°E~160°E)对流活动均存在反相变化的关系, 将之称为季节内尺度的印度洋—西太平洋对流涛动(Indo-West Pacific Convection Oscillation), 简称IPCO。对IPCO两极子区域对流活动进行超前滞后相关分析, 发现IPCO事件形成—发展—消亡的生命周期是由对流活动季节内振荡及其传播造成的。对流扰动首先在赤道中西印度洋形成, 随后逐渐向东发展变强, 在其继续变强的过程中将分两支传播:一支由赤道印度洋向北传播, 至印度半岛南部后逐渐减弱消失;另一支沿赤道继续东传, 在海洋大陆受到抑制, 快速越过海洋大陆到达赤道西太平洋后又开始发展变强, 随后北传至西北太平洋区域逐渐减弱, 最终至我国长江流域中下游到日本区域消失。将这一过程划分为8个位相, 详细分析了不同位相对应的环流场和降水场特征, 最后给出了IPCO事件演化示意图。     

An assessment of Indo-Pacific oceanic channel dynamics in the FGOALS-g2 coupled climate system model

Lag correlations of sea surface temperature anomalies (SSTAs), sea surface height anomalies (SSHAs), subsurface temperature anomalies, and surface zonal wind anomalies (SZWAs) produced by the Flexible Global Ocean-Atmosphere-Land System model: Grid-point Version 2 (FGOALS-g2) are analyzed and compared with observations. The insignificant, albeit positive, lag correlations between the SSTAs in the southeastern tropical Indian Ocean (STIO) in fall and the SSTAs in the central-eastern Pacific cold tongue in the following summer through fall are found to be not in agreement with the observational analysis. The model, however, does reproduce the significant lag correlations between the SSHAs in the STIO in fall and those in the cold tongue at the one-year time lag in the observations. These, along with the significant lag correlations between the SSTAs in the STIO in fall and the subsurface temperature anomalies in the equatorial Pacific vertical section in the following year, suggest that the Indonesian Throughflow plays an important role in propagating the Indian Ocean anomalies into the equatorial Pacific Ocean. Analyses of the interannual anomalies of the Indonesian Throughflow transport suggest that the FGOALS-g2 climate system simulates, but underestimates, the oceanic channel dynamics between the Indian and Pacific Oceans. FGOALS-g2 is shown to produce lag correlations between the SZWAs over the western equatorial Pacific in fall and the cold tongue SSTAs at the one-year time lag that are too strong to be realistic in comparison with observations. The analyses suggest that the atmospheric bridge over the Indo-Pacific Ocean is overestimated in the FGOALS-g2 coupled climate model.     

南印度洋偶极子的特征及其与ENSO的关系

利用逐月OISST、ERSST及NCEP2表面风场等资料探讨了南印度洋偶极子(Southern Indian Ocean Dipole,SIOD)的结构特征、形成原因及其与ENSO的关系。结果表明:在南印度洋,偶极子形态的年际海表面温度异常在10—12月出现,次年2月达到极值,随后的4—6月消亡。SIOD的形成主要是风场、潜热通量和短波辐射通量起作用,混合层深度异常加厚或变浅有助于SIOD的形成。近30 a资料表明,SIOD的盛期超前ENSO 9~10个月,且具有季节锁相特征。20世纪70年代中期发生年代际气候突变后,SIOD与ENSO的相关关系显著增强。正SIOD事件之后一般都有El Nio事件发生,负SIOD事件之后都有La Nia事件发生。     

热带印度洋秋季偶极子模态与南海夏季风强度变化的关系

利用多年的Reynolds月平均海表温度资料和NCEP／NCAR全球大气再分析资料，采用经验正交函数（EOF）分析和滑动相关方法，研究了热带印度洋秋季偶极子模态和南海夏季风强度变化的关系。结果表明：（1）热带印度洋秋季海表温度距平（SSTA）的主要模态是全区一致型和偶极子（IOD）型，全区一致型模态主要代表了秋季SSTA全海盆一致的年代际及其以上时间尺度的变化，IOD型模态主要反映热带印度洋秋季SSTA年际时间尺度的变化。（2）当前期秋季热带印度洋存在正（负）IOD模态时，南海的夏季风强度减弱（增强）。二者年际变化的负相关关系在长期趋势的冷位相期不显著，而在暖位相期显著。（3）当南海夏季风强度增强（减弱）时，后期秋季热带印度洋出现正（负）IOD模态。二者年际变化的正相关关系在长期趋势的冷、暖位相期显著，在冷、暖位相转换期前后不显著。     

赤道东太平洋海温异常期间印度洋偶极子对东亚季风区影响的数值模拟

利用中科院大气所的IAP AGCM-Ⅱ大气环流模式，模拟了在存在和没有赤道东太平洋海温异常影响下，印度洋偶极子对东亚季风区天气气候的影响。结果表明：后者东亚地区西南季风的爆发偏晚，南海夏季风增强，此时我国大陆降水偏多；而前者西南季风的爆发将更偏晚，南海夏季风减弱，此时华北降水偏少；赤道东太平洋海温异常和印度洋偶极子有协同作用。     

Interannual Variability of Sea Surface Temperature in the Northern Indian Ocean Associated with ENSO and IOD

The Northern Indian Ocean(NIO) sea surface temperature(SST) warming,associated with the El Ni o/Southern Oscillations(ENSO) and the Indian Ocean Dipole(IOD) mode,is investigated using the International Comprehensive Ocean-Atmosphere Data Set(ICOADS) monthly data for the period 1979 2010.Statistical analyses are used to identify respective contribution from ENSO and IOD.The results indicate that the first NIO SST warming in September November is associated with an IOD event,while the second NIO SST warming in spring-summer following the mature phase of ENSO is associated with an ENSO event.In the year that IOD co-occurred with ENSO,NIO SST warms twice,rising in the ENSO developing year and decay year.Both shortwave radiation and latent heat flux contribute to the NIO SST variation.The change in shortwave radiation is due to the change in cloudiness.A cloud-SST feedback plays an important role in NIO SST warming.The latent heat flux is related to the change in monsoonal wind.In the first NIO warming,the SST anomaly is mainly due to the change in the latent heat flux.In the second NIO warming,both factors are important.     

随钻偶极远探测声场的辐射特性

本文对偶极横波远探测技术在随钻测井中的应用进行了探讨.对于随钻远探测而言,井中声源向井外地层中的辐射性能是它的主控因素.本文从井孔内外声场出发,考察了随钻和电缆测井中偶极声源的辐射效率,即声源产生的辐射波能流与沿井传播的导波能流之比;分析了声源的远场辐射指向性;基于声源辐射与接收之间的互易性,快速模拟和处理了随钻测井下SH和SV横波远探测波形.研究结果表明,随钻条件下SH和SV横波的最大辐射效率受钻铤的影响较电缆的情况降低了70%左右,且横波最大辐射效率对应的优势激发频率也从电缆的3.5kHz降为2.5kHz左右;虽然随钻偶极的横波辐射效率明显降低,但由理论模拟的随钻远探测数据的成像结果可知,声源辐射到地层中的横波能量仍足以探测井外反射体,表明随钻偶极远探测技术在理论上是可行的,本文结果为随钻偶极远探测测井提供了理论依据.     

First and second baroclinic mode responses of the tropical Indian Ocean to interannual equatorial wind anomalies

The combined and individual responses of the first and second baroclinic mode dynamics of the tropical Indian Ocean to the well-known Indian Ocean Dipole mode (IOD) wind anomalies are investigated. The IOD forced first baroclinic Rossby waves arrive at the western boundary in three months, while the reflected component from the eastern boundary with opposite phase arrives in five to six months, both carry input energy to the west. The inclusion of the second baroclinic mode slows down the wave propagation by mode coupling and stretches the energy spectrum to a relatively longer time scale. The total energy exists in the equatorial wave guide for at least five months from the forcing, as much as 10% of that of the atmospheric input, which mainly dissipates at the western boundary. The individual responses of the ocean to IOD interannual wind anomaly show that the significant modes of oceanic anomalies are confined to a wave guide of 10° on either side of the equator.     

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.