Warming in the Northwestern Indian Ocean Associated with the El Nio Event

This paper investigates possible warming effects of an El Nino event on the sea surface temperature anomaly (SSTA) in the northwestern Indian Ocean. Most pure positive Indian Ocean dipole (IOD) events (without an El Nino event co-occurring) have a maximum positive SSTA mainly in the central Indian Ocean south of the equator, while most co-occurrences with an El Nino event exhibit a northwest-southeast typical dipole mode. It is therefore inferred that warming in the northwestern Indian Ocean is closely related to the El Nino event. Based on the atmospheric bridge theory, warming in the northwestern Indian Ocean during co-occurring cases may be primarily caused by relatively less latent heat loss from the ocean due to reduced wind speed. The deepened thermocline also contributes to the warming along the east coast of Africa through the suppressed upwelling of the cold water. Therefore, the El Nino event is suggested to have a modulating effect on the structure of the dipole mode in the tropical Indian Ocean.     

Warming in the northwestern Indian Ocean associated with the El Niño event

This paper investigates possible warming effects of an E1 Nifio event on the sea surface temperature anomaly （SSTA） in the northwestern Indian Ocean. Most pure positive Indian Ocean dipole （IOD） events （without an E1 Nifio event co-occurring） have a maximum positive SSTA mainly in the central Indian Ocean south of the equator, while most co-occurrences with an E1 Nifio event exhibit a northwest-southeast typical dipole mode. It is therefore inferred that warming in the northwestern Indian Ocean is closely related to the E1 Nifio event. Based on the atmospheric bridge theory, warming in the northwestern Indian Ocean during co-occurring cases may be primarily caused by relatively less latent heat loss from the ocean due to reduced wind speed. The deepened thermocline also contributes to the warming along the east coast of Africa through the suppressed upwelling of the cold water. Therefore, the E1 Nifio event is suggested to have a modulating effect on the structure of the dipole mode in the tropical Indian Ocean.     

两类El Ni?o对应的印度洋偶极子事件的比较研究

利用多种大气和海洋再分析资料,采用合成分析及2.5层简化海洋模型数值模拟等方法,研究了1951—2012年期间,与东部和中部型El Ni?o事件相伴随的热带印度洋海温偶极子(Indian Ocean Dipole,IOD)出现时,热带印度洋海温异常增暖及其上空海气耦合特征的物理机制。结果表明:夏秋季节,伴随东部型El Ni?o而发生的IOD事件(EP-IOD)和伴随中部型El Ni?o而发生的IOD事件(CP-IOD)中,热带印度洋海温正异常的强度与空间分布具有很大差异。对于EP-IOD事件,夏季,海温正异常中心最先出现在热带西北印度洋;随后秋季,海温正异常向东南发展并扩大至热带中南印度洋,强度较强。对于CP-IOD事件,夏季和秋季,海温正异常中心都位于热带中南印度洋,呈东西向带状分布,但海温正异常强度较EP-IOD事件中弱。进一步分析表明,在EP-IOD事件中,夏季,热带西北印度洋海区西南季风偏弱,通过影响夹卷混合过程导致热带西北印度洋海温上升;秋季,热带西北印度洋上空的异常偏东风导致垂向夹卷混合的正异常,对热带西北印度洋增暖的维持起到重要作用;热带中南印度洋的增暖主要受赤道东南印度洋西传的暖性Rossby波影响。而在CP-IOD事件中,夏秋两季,热带中南印度洋海区出现显著的西北风异常,其上空风速的负异常是增温的主要原因;同时赤道东南印度洋西传的暖性Rossby波对热带中南印度洋的增暖也起到重要作用。      

海温异常对东亚夏季风影响机理的研究进展

从短期气候预测关注的外强迫信号角度出发,回顾了国内外在海温异常对东亚夏季风和我国汛期降水影响机理方面的主要研究进展,重点评述了热带太平洋ENSO循环、热带印度洋全区一致型海温模态、热带印度洋海温异常偶极子、南印度洋偶极子和北大西洋海温三极子模态的年际变化及其对东亚夏季风年际变率的影响。从研究成果在短期气候预测业务中应用的角度,重点关注海温异常和东亚夏季风年际变率以及我国汛期降水多雨带位置的关系,总结了海温异常作为外强迫信号对我国汛期降水预测的指示意义以及汛期降水预测的难度。最后指出气候预测业务对东亚夏季风影响的机理研究和动力气候模式发展方面的需求。     

Decadal and interannual variability of the Indian Ocean Dipole

This study investigates the decadal and interannual variability of the Indian Ocean Dipole （IOD）. It is found that the long-term IOD index displays a decadal phase variation. Prior to 1920 negative phase dominates but after 1960 positive phase prevails. Under the warming background of the tropical ocean, a larger warming trend in the western Indian Ocean is responsible for the decadal phase variation of the IOD mode. Due to reduced latent heat loss from the local ocean, the western Indian Ocean warming may be caused by the weakened Indian Ocean westerly summer monsoon. The interannual air-sea coupled IOD mode varies on the background of its decadal variability. During the earlier period （1948-1969）, IOD events are characterized by opposing SST anomaly （SSTA） in the western and eastern Indian Ocean, with a single vertical circulation above the equatorial Indian Ocean. But in the later period （1980-2003）, with positive IOD dominating, most IOD events have a zonal gradient perturbation on a uniform positive SSTA. However, there are three exceptionally strong positive IOD events （1982, 1994, and 1997）, with opposite SSTA in the western and eastern Indian Ocean, accompanied by an El Nifio event. Consequently, two anomalous reversed Walker cells are located separately over the Indian Ocean and western-eastern Pacific; the one over the Indian Ocean is much stronger than that during other positive IOD events.     

Tropical Indian Ocean variability revealed by self-organizing maps

The tropical Indian Ocean climate variability is investigated using an artificial neural network analysis called self-organizing map (SOM) for both observational data and coupled model outputs. The SOM successfully captures the dipole sea surface temperature anomaly (SSTA) pattern associated with the Indian Ocean Dipole (IOD) and basin-wide warming/cooling associated with ENSO. The dipole SSTA pattern appears only in boreal summer and fall, whereas the basin-wide warming/cooling appears mostly in boreal winter and spring owing to the phase-locking nature of these phenomena. Their occurrence also undergoes significant decadal variation. Composite diagrams constructed for nodes in the SOM array based on the simulated SSTA reveal interesting features. For the nodes with the basin-wide warming, a strong positive SSTA in the eastern equatorial Pacific, a negative Southern Oscillation, and a negative precipitation anomaly in East Africa are found. The nodes with the positive IOD are associated with a weak positive SSTA in the central equatorial Pacific or positive SSTA in the eastern equatorial Pacific, a positive (negative) sea level pressure anomaly in the eastern (western) tropical Indian Ocean, and a positive precipitation anomaly over East Africa. The warming in the central equatorial Pacific appears to correspond to El Niño Modoki discussed recently. These results suggest usefulness of SOM in studying large-scale ocean–atmosphere coupled phenomena.     

有无El Ni?o情况下印度洋偶极子演变特征及机理研究

基于NCEP、SODA等再分析资料,采用合成分析和2.5层简化海洋模型数值模拟等方法,分析了El Ni?o和正印度洋偶极子(IOD)事件不同配置情形下印度洋海温异常的演变特征,并重点探讨了联合IOD和独立IOD事件中,关键海区海温异常的发展演变及其可能机制。对于联合IOD事件,初期马里沿岸的增暖可能对其发生起主要的激发作用;而对于独立IOD事件的发生,则可能是赤道东南印度洋的降温起主导作用。不同类型IOD事件中,热带印度洋海表温度异常(SSTA)和海面高度异常(SSHA)的演变特征有明显差别,孟加拉湾上空降水异常所起的作用也不一样,印度洋不同海区混合层温度异常的演变机制也有显著不同。基于2.5层简化海洋模式结果的分析表明,各个海区的热力、动力过程在不同IOD事件有着不同的作用。例如在索马里沿岸海区:对于联合IOD事件,西印度洋赤道东风异常和索马里沿岸东北风异常,有利于该海区出现纬向平流热输送和海表热通量正异常,从而增暖。而对于独立IOD事件,阿拉伯海上空的强西南风异常,加强了索马里沿岸底层冷水的上翻和海表的热通量损失,导致前期纬向平流和夹卷混合的负异常以及后期海表热通量的负异常,使得该海区变冷。      

前冬印度洋海盆一致模对ENSO衰减期华南春季降水的影响

利用逐月台站观测降水、HadISST1.1海温和ERA5大气再分析资料,研究了前冬印度洋海盆一致模（Indian Ocean Basin,IOB）对华南春季降水（SCSR）与ENSO关系的影响,并分析了IOB通过调控ENSO环流异常进而影响SCSR的可能机制。结果表明：当前冬El Niño（La Niña）与IOB暖（冷）位相同时发生时,SCSR显著增多（减少）;而当El Niño或La Niña单独发生而IOB处于中性时,SCSR并无明显多寡倾向。其原因在于,当El Niño与IOB暖相位并存时,前冬热带印度洋和赤道中东太平洋均为正海温异常（Sea-Surface Temperature Anomaly,SSTA）,且印度洋SSTA强度可一直维持至春季。在对流层低层,春季赤道中东太平洋的正SSTA激发出异常西北太平洋反气旋（Western North Pacific Anticyclone,WNPAC）。而热带印度洋的正SSTA在副热带印度洋激发出赤道南北反对称环流,赤道以北的东风异常有利于异常WNPAC西伸;赤道以南的西风异常与来自赤道西太平洋的东风异常在东印度洋辐合上升,气流至西北太平洋下沉,形成经向垂直环流,有利于春季WNPAC维持。在对流层高层,印度洋的正SSTA在热带印度洋上空激发出位势高度正异常,随之形成的气压经向梯度加强了东亚高空副热带西风急流,进而在华南上空形成异常辐散环流。WNPAC的西伸和加强可为华南提供充足的水汽,同时高空辐散在华南引发水汽上升运动,共同导致SCSR正异常。而若El Niño发生时IOB处于中性状态,El Niño相关的SSTA衰减较快,春季WNPAC不显著,SCSR无明显多寡趋势。     

与不同El Nino相伴的IOD事件的季节演变特征对比

基于1951—2012年逐月海洋和大气多种要素的再分析资料,分析了与两类El Nino相伴的IOD(Indian Ocean Dipole,印度洋偶极子)事件盛期的海洋和大气异常特征,并进一步对比了与不同类型El Nino相伴的IOD事件的季节演变及对应的海气耦合过程。结果表明:两类IOD事件盛期时,暖海温强度和位置有显著差异。发生在东部型El Nino期间的IOD事件(简称EP-IOD)盛期,正(负)SSTA中心出现在热带西北(赤道东南)印度洋,强度相当,对应的热带印度洋—海洋大陆异常Walker环流强度较强、范围较大;与中部型CP El Nino相伴的IOD事件(简称CP-IOD)的正SSTA相对较弱,且偏于南印度洋,异常Walker环流较弱、较窄。在季节演变中,两类IOD事件期间的局地海气过程差异显著,伴随着西印度洋西南季风减弱和东印度洋异常东风加强,EP-IOD事件的发展以西正东负的偶极型异常海温的出现及加强为主要特征;而CP-IOD事件的发生发展则与西北印度洋异常冷海温的生消及南印度洋暖水的堆积相伴,表现为"-+-"三极型SSTA的出现并转为西正东负偶极型的过程,夏季时出现在东印度洋的异常东风以及赤道中印度洋低层负涡度异常水平环流对其发展具有重要作用。     

Future change of the Indian Ocean basin-wide and dipole modes in the CMIP5

The Indian Ocean sea surface temperature (SST) variability has been represented with the two dominant variability modes: the Indian Ocean basin-wide (IOBW) and dipole (IOD) modes. Here we investigate future changes of the two modes together with mean state and El Niño and Southern Oscillation (ENSO) relationship under the anthropogenic global warming using 20 coupled models that participated in the phase five of Coupled Model Intercomparison Project by comparing the historical run from 1950 to 2005 and the RCP 4.5 run from 2050 to 2099. The five best models are selected based on the evaluation of the 20 models’ performances in simulating the two modes and Indian Ocean basic state for the latest 56 years. They are capable of capturing the IOBW and IOD modes in their spatial distribution, seasonal cycle, major periodicity, and relationship with ENSO to some extent. The five best models project the significant changes in the Indian Ocean mean state and variability including the two dominant modes in the latter part of twenty-first century under the anthropogenic warming scenario. First, the annual mean climatological SST displays an IOD-like pattern change over the Indian Ocean with enhanced warming in the northwestern Indian Ocean and relatively weaker warming off the Sumatra–Java coast. It is also noted that the monthly SST variance is increased over the eastern and southwestern Indian Ocean. Second, the IOBW variability on a quasi-biennial time scale will be enhanced due to the strengthening of the ENSO–IOBW mode relationship although the total variance of the IOBW mode will be significantly reduced particularly during late summer and fall. The enhanced air-sea coupling over the Indian-western Pacific climate in response to El Nino activity in the future projection makes favorable condition for a positive IOD while it tends to derive relatively cold temperature over the eastern Indian Ocean. This positive IOD-like ENSO response weakens the relationship between the eastern Indian Ocean and El Nino while strengthens the relationship with western Indian Ocean. Third, the IOD mode, intrinsic coupled mode of the Indian Ocean may not be changed appreciably under the anthropogenic global warming.     

Decadal Changes in Interannual Dependence of the Bay of Bengal Summer Monsoon Onset on ENSO Modulated by the Pacific Decadal Oscillation

Interannual variations of the Bay of Bengal summer monsoon (BOBSM) onset in association with El Ni?o?Southern Oscillation (ENSO) are reexamined using NCEP1, JRA-55 and ERA20C atmospheric and Hadley sea surface temperature (SST) reanalysis datasets over the period 1900?2017. Decadal changes exist in the dependence of the BOBSM onset on ENSO, varying with the Pacific Decadal Oscillation (PDO). A higher correlation between the BOBSM onset and ENSO arises during the warm PDO epochs, with distinct late (early) onsets following El Ni?o (La Ni?a) events. In contrast, less significant correlations occur during the cold PDO epochs. The mechanism for the PDO modulating the ENSO?BOBSM onset relationship is through the variations in SST anomaly (SSTA) patterns. During the warm PDO epochs, the superimpositions of the PDO-related and ENSO-related SSTAs lead to the SSTA distribution of an El Ni?o (La Ni?a) event exhibiting significant positive (negative) SSTAs over the tropical central?eastern Pacific and Indian Ocean along with negative (positive) SSTAs, especially over the tropical western Pacific (TWP), forming a strong zonal interoceanic SSTA gradient between the TWP and tropical Indian Ocean. Significant anomalous lower tropospheric easterlies (westerlies) together with upper-tropospheric westerlies (easterlies) are thus induced over the BOB, favoring an abnormally late (early) BOBSM onset. During the cold PDO epochs, however, the superimpositions of PDO-related SSTAs with El Ni?o-related (La Ni?a-related) SSTAs lead to insignificant SSTAs over the TWP and a weak zonal SSTA gradient, without distinct circulation anomalies over the BOB favoring early or late BOBSM onsets.     

夏季西北太平洋热带气旋生成频次与热带海温关系的年代际变化

探讨了夏季(6—8月)西北太平洋(Western North Pacific,WNP)热带气旋生成频次(Tropical Cyclone Genesis Frequency,TCGF)与热带海温关系的年代际变化,发现影响WNP TCGF的热带海温型在1991/1992年发生了年代际变化。在1990年代初之前,TCGF正异常对应的热带海温异常(Sea Surface Temperature Anomaly,SSTA)呈现东部型La Ni?a衰减位相,前冬至春季WNP局地暖SSTA在其西北侧激发气旋异常,夏季时由热带印度洋冷SSTA继续维持。在1990年代初之后,TCGF正异常对应的热带SSTA呈现东部型La Ni?a向中部型El Ni?o快速转换的位相,夏季中太平洋暖SSTA在其西北侧激发气旋异常,同时热带东印度洋至海洋性大陆以及热带大西洋的冷SSTA通过垂直环流圈加强中太平洋的辐合上升运动,进一步维持其西北侧气旋异常。由于激发气旋异常的暖SSTA在第二个年代相较第一个年代明显偏南偏东,气旋异常和TCGF正异常在第二个年代也整体偏南且向东扩展至更远的区域。WNP TCGF与热带海温关系的年代际变化与1990年代初之后厄尔尼诺-南方涛动演变速率加快有关。      

观测分析El Ni?o衰减早晚对南亚与青藏高原夏季降水和气温的影响

El Ni?o（厄尔尼诺）事件对东亚和南亚次年夏季降水影响及其机理已经得到充分研究,但其对夏季青藏高原降水是否有显著影响还不清楚。本研究根据1950年后El Ni?o事件次年衰减期演变速度,对比分析衰减早型与晚型El Ni?o事件对南亚季风区与青藏高原夏季（6～9月）季节平均和月平均气候影响差异。结果显示在衰减早型次年夏季热带太平洋海温转为La Ni?a（拉尼娜）型且持续发展,引起Walker环流上升支西移,印度洋和南亚季风区上升运动加强,同时激发异常西北太平洋反气旋（NWPAC）,阿拉伯海异常气旋和伊朗高原异常反气旋性环流响应,增加7～9月对流层偏南气流和印度洋水汽输送,导致南亚和高原西南侧降水偏多。衰减晚型次年6～8月热带太平洋El Ni?o型海温仍维持,印度洋暖异常海温显著,对应的印度洋和南亚季风区上升运动较弱,NWPAC西伸控制南亚季风区,阿拉伯海和中西亚分别呈现异常反气旋和气旋性环流,导致青藏高原西风加强,水汽输送减少,南亚北部和高原降水一致偏少。结果表明:（1）El Ni?o显著影响次年青藏高原西南部夏季季节和月平均降水与温度,是印度和高原西南部夏季降水显著相关的重要原因;（2）El Ni?o衰减快慢速度对南亚和青藏高原西南部夏季季节内降水的影响有着重要差异。     

El Nino 位相期间印度洋海温异常对中国南部初夏降水及初夏亚洲季风影响的数值模拟研究

基于中国科学院大气物理研究所的IAP 9L大气环流模式，设计并完成了赤道太平洋暖异常海温和印度洋地区的不同结构异常海温的强迫试验，以研究在El Ni o位相期间印度洋不同海温异常分布对初夏亚洲季风及我国南部地区初夏降水的影响。结果表明：El Ni o位相期间印度洋异常海温的作用是不可忽视的。在El Ni o位相期间，印度洋不同的海温结构对越赤道气流异常，对印度、中南半岛及中国南方的降水分布有重要的影响。利用NCEP的资料进行合成分析，进一步证实了数值模拟结果的可靠性。     

ENSO多样性研究进展

El Ni?o是热带中东太平洋异常偏暖的现象,发展过程具有显著的季节锁相特征。近年来,新形态事件更频繁发生引起了科学界广泛关注。学者们根据空间分布形态或爆发时间将ENSO事件分为两类,虽然选取标准不同,分类结果却有诸多相似点:中太平洋(Dateline、Modoki、CP、WP及SU型)El Ni?o事件发展至成熟时,正SSTA中心位于赤道太平洋中部;东太平洋(传统、EP、CT及SP型)El Ni?o发展至成熟时,正SSTA中心位于赤道东太平洋,低层西风异常更强,向东传输的距离也更远。研究结果显示,东太平洋El Ni?o比中太平洋El Ni?o持续时间更长,强度也更强;两类事件对全球气候的影响模态有很大的差异。近几十年,中太平洋El Ni?o出现频率有所增加,但其原因尚未清楚。关于两类事件生成发展和位相转换的动力原因,目前科学界普遍认为东太平洋El Ni?o是一个海盆尺度的海气耦合过程,其生消过程与温跃层的变化有紧密联系,但对中太平洋El Ni?o的动力机制尚未有统一的认识。      

热带印度洋海温异常单、偶极模态及其相互作用

利用最近50多年的GISST和NCEP的OISST海表温度资料研究了印度洋海温变化的空间分布型和多重时间尺度及其相互作用.结果表明,热带印度洋海温主要存在两种空间分布型,即全海盆符号一致的单极和东、西部符号相反的偶极.单极既存在长期增暖趋势,也存在年际振荡;偶极则以年际变化为主.在去掉由EOF重建的单极后,热带印度洋东、西部海温表现为显著的反相关关系;对17次典型偶极子个例的分析表明,对偶极子本身而言,偶极子的演变更像是一种翘翘板似的局地振荡.单极在长期趋势和年际时间尺度上对偶极的影响是不同的.长期趋势缩短了偶极子的生命期,在冷期,印度洋海温经历了由负单极到正偶极再到负单极的演变,偶极子的异常信号最早出现在热带西印度洋;在暖期,印度洋海温经历了由正单极到正偶极再到正单极的演变,偶极子的异常信号最早出现在热带东印度洋.对年际时间尺度的变化而言,印度洋海温异常由负单极向正偶极再到正单极转换,偶极子位于一种单极向另一种单极的转换过程之中,在此过程中,印度洋海温表现为明显自西向东的传播特征.     

On the Second-Year Warming in Late 2019 over the Tropical Pacific and Its Attribution to an Indian Ocean Dipole Event※

After its maturity, El Ni?o usually decays rapidly in the following summer and evolves into a La Ni?a pattern. However, this was not the case for the 2018/19 El Ni?o event. Based on multiple reanalysis data sets, the space-time evolution and triggering mechanism for the unusual second-year warming in late 2019, after the 2018/19 El Ni?o event, are investigated in the tropical Pacific. After a short decaying period associated with the 2018/19 El Ni?o condition, positive sea surface temperature anomalies (SSTAs) re-intensified in the eastern equatorial Pacific in late 2019. Compared with the composite pattern of El Ni?o in the following year, two key differences are evident in the evolution of SSTAs in 2019. First, is the persistence of the surface warming over the central equatorial Pacific in May, and second, is the re-intensification of the positive SSTAs over the eastern equatorial Pacific in September. Observational results suggest that the re-intensification of anomalous westerly winds over the western and central Pacific, induced remotely by an extreme Indian Ocean Dipole (IOD) event, acted as a triggering mechanism for the second-year warming in late 2019. That is, the IOD-related cold SSTAs in the eastern Indian Ocean established and sustained anomalous surface westerly winds over the western equatorial Pacific, which induced downwelling Kelvin waves propagating eastward along the equator. At the same time, the subsurface ocean provided plenty of warm water in the western and central equatorial Pacific. Mixed-layer heat budget analyses further confirm that positive zonal advection, induced by the anomalous westerly winds, and thermocline feedback played important roles in leading to the second-year warming in late 2019. This study provides new insights into the processes responsible for the diversity of El Ni?o evolution, which is important for improving the physical understanding and seasonal prediction of El Ni?o events.     

冬季和春季印度洋海温异常年际变率模态对中国东部夏季降水的可能影响过程

印度洋热力状况是影响全球气候变化和亚洲季风变异的一个重要的因素,但以往研究更多关注热带印度洋海温的变化,对南印度洋中高纬地区海温变化关注不够,由此限制了我们对印度洋的全面认识.本文研究了年际尺度上整个印度洋海温异常主导模态的特征及其对我国东部地区夏季降水的可能影响过程,以期望为气候变异研究及预测提供理论依据.研究结果表明:全印度洋海温异常年际变率的主导模态特征是在南印度洋副热带地区海温异常呈现西南—东北反向变化的偶极子模态,西极子位于马达加斯加以东南洋面,东极子位于澳大利亚以西洋面;同时,热带印度洋海温异常与东极子一致.当西极子为正的海温异常,东极子、热带印度洋为负异常时定义为正的印度洋海温异常年际变率模态;反之,则为负的印度洋海温异常年际变率模态.从冬至春,印度洋海温异常年际变率模态具有较好的季节持续性;与我国长江中游地区夏季降水显著负相关,而与我国华南地区夏季降水显著正相关.其可能的影响过程为:对于正的冬、春季印度洋海温异常年际变率模态事件,印度洋地区异常纬向风的经向大气遥相关使得热带印度洋盛行西风异常,导致春、夏季海洋性大陆对流减弱,使夏季西太平洋副热带高压强度偏弱、位置偏东偏北,造成华南地区夏季降水增多,长江中游地区降水减少;反之亦然.同时,印度洋海温异常年际变率模态可通过改变印度洋和孟加拉湾向长江中游地区的水汽输送而影响其夏季降水.     

超强与普通厄尔尼诺海-气特征差异及对西太平洋副热带高压的不同影响

利用NCEP/NCAR再分析资料、GODAS海洋资料、哈得来中心海表温度（SST）以及中国国家气候中心（NCC）环流指数数据,依据美国气候预测中心的厄尔尼诺事件标准筛选出1980-2016年的超强与普通厄尔尼诺事件,对比了两类事件的不同生命阶段内海表及次表层温度特征的差异,并探讨了其对西太平洋副热带高压（西太副高）的不同影响。结果表明,对超强厄尔尼诺事件而言,海表温度正距平发展早且迅速,其大值中心偏东,纬向梯度强,但对普通厄尔尼诺事件而言,海表温度正距平中心偏西,纬向梯度小。厄尔尼诺事件的发展源于次表层海温距平（SOTA）随开尔文波东传并沿温跃层上升到达海表,其波动前部区域异常垂直海流对次表层海温距平的变化起重要作用;当海气激烈耦合时,可在温跃层激发出更强的海洋波动,使得次表层变暖更明显,激发出强的厄尔尼诺事件。海温异常强迫出的大气异常环流的强度与强迫源的强度关系密切。两类厄尔尼诺均能通过异常的沃克环流引起大气Gill型响应,使得西太副高偏强、西伸,且当超强厄尔尼诺发生时,异常沃克环流更强,海洋性大陆区域上空的异常强辐散导致Gill型响应而产生的反气旋更强,对西太副高的影响更甚。印度洋海表温度对厄尔尼诺的滞后变暖所带来的影响在上述亚太大气环流的持续异常中起重要作用。这些结果有利于加深对不同类型厄尔尼诺事件及影响西太副高机理的认识。      

影响南海夏季风爆发年际变化的关键海区及机制初探

利用1958—2011年NCEP/ NCAR再分析资料和ERSST资料,采用Lanczos时间滤波器、相关分析、回归分析、合成分析和交叉检验等方法,研究了影响南海夏季风爆发年际变化的关键海区海温异常的来源与可能机制。结果表明,前冬(12—2月)热带西南印度洋和热带西北太平洋是影响南海夏季风爆发年际变化的关键海区。冬季热带西南印度洋(热带西北太平洋)的异常增暖是由前一年夏季El Ni?o早爆发(强印度季风异常驱动的行星尺度东-西向环流)触发、热带印度洋(西北太平洋)局地海气正反馈过程引起并维持到春季。冬季热带西北太平洋反气旋性环流(气旋性环流)及印度洋(热带西北太平洋)的暖海区局地海气相互作用使得印度洋(热带西北太平洋)海温异常维持到春末。春季,逐渐加强北移到10 °N附近的低层大气对北印度洋(热带西北太平洋)暖海温异常响应的东风急流(异常西风)及南海-热带西北太平洋维持的反气旋性环流(气旋性环流)异常,使得南海夏季风晚(早)爆发。