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西北太平洋低频振荡对热带气旋生成的动力作用及其物理机制 总被引：20，自引：4，他引：16
利用全球再分析资料以及美国联合台风预报中心的热带气旋(TC)数据, 从动力和能量转换方面深入分析了西北太平洋上空30～60天大气低频振荡(MJO)对西北太平洋区域TC生成的调制作用。研究结果表明, 当西北太平洋西侧为MJO的西风位相所控制时, MJO通过纬向风的辐合作用使得在辐合区传播的波动发生波数增加, 波长减短的结构改变, 从而触发较大尺度波动向天气尺度波动的演变; 西风位相期间纬向风的纬向辐合与经向切变可以使得低频波动动能向高频波动的转换得到加强, 从而使得在此区域TC生成的数量明显偏多。相反, 当西北太平洋西侧为MJO的东风位相时, TC生成的数量得到抑制。此外, 随着西风位相中西风的加强(东风位相中东风的加强), TC的生成概率将得到增加 (减少)。但是, 在西北太平洋东侧海域, MJO对TC活动的调制作用要减弱许多。对MJO活动年际变化的研究表明, 在西太暖池处于暖状态年时, 西北太平洋西侧的MJO活动频繁, 西风位相活跃, 从而有利于此区域TC的生成, 而冷年的情况正好相反。 相似文献
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利用1978-2013年美国NOAA逐候MJO指数和中国气象局上海台风研究所热带气旋资料,研究了MJO与影响广西热带气旋发生发展的联系。结果表明,当MJO处于非洲大陆和西印度洋时,热带气旋生成区域上空为异常东风带;而当MJO处于西太平洋时,热带气旋生成区域北侧为东风异常带、南侧为西风异常带,有利于季风槽或气旋性环流加强,导致影响广西热带气旋频数偏多。当MJO处于东印度洋时,南海上空风场存在明显的向南分量,热带气旋生成数少、位置偏南;而当MJO处于东太平洋时,热带西太平洋对流受到抑制,导致影响广西热带气旋偏少。 相似文献
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《气象研究与应用》2021,(3)
使用1951—2020年热带气旋资料、NCEP/NCAR再分析、PDO指数、NOAA OLR、副热带高压指数等资料,从海洋大气低频振荡角度分析影响广西热带气旋气候异常可能原因。结果表明,90年代以来影响广西热带气旋年际变化幅度增大,表现出向极端异常变化的趋势。从印度洋到西太平洋存在明显的MJO向东传播,对流抑制位相较弱、持续时间短,对流增强位相较强,影响广西热带气旋偏多。反之,从印度洋到西太平洋无MJO活动或强度较弱,存在较强的低频对流抑制带向东传播、持续时间长,较强的低频对流带位于东太平洋,影响广西热带气旋偏少。影响广西热带气旋减少趋势与PDO指数增大有密切的联系,可能与在印度洋、太平洋海温增暖背景下副热带高压强度偏强及西伸脊点偏西有关。 相似文献
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在分析研究太平洋海气耦合经向模（Pacific Meridional Mode——PMM）和西北太平洋生成热带气旋频数变化关系的基础上,利用NCAR的大气环流模式CAM3模拟研究了太平洋海气耦合经向模态对西北太平洋生成热带气旋的影响。结果表明,海气耦合的经向模态通过影响热带气旋生成的大尺度环境从而影响热带气旋的频数和强度。在模式中当增加了PMM的海温强迫后,纬向风切变变小,对流层中低层相对湿度变大,热带西太平洋对流层低层出现西风异常,在西北太平洋地区形成一个异常的气旋性环流,并且匹配有较大的正涡度异常;对流层高层出现赤道东风异常和一个与低层气旋性环流相匹配的反气旋性环流,有利于对流活动的发展,从而有利于热带气旋的生成和发展。在增加了PMM的海温强迫的试验中,热带气旋中心的海平面最低气压降低,850 hPa中心附近最大切向风速增加,气旋中高层的暖心强度增强。热带气旋强度总体增加。数值模拟结果与资料分析相互映证,揭示了太平洋经向模态对西北太平洋热带气旋有重要影响。 相似文献
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西北太平洋热带气旋频数的年际、年代际变化及预测 总被引：4，自引：0，他引：4
利用1950-2009年60 a的热带气旋资料、NOAA海温、NCEP再分析资料及74项环流指数等资料,研究了西北太平洋热带气旋频数的年际、年代际变化特征,结果表明,西北太平洋热带气旋生成频数既有显著的年际变化,同时也存在明显的年代际变化。自1950年以来,西北太平洋热带气旋频数经历了一个先增加再减少的过程,其中转折点在20世纪70年代中后期,与之相对应,热带气旋路径频数也呈现明显年代际变化。在此基础上,通过分析前期春季海温场、大气环流异常及环流指数与夏季(6-10月)热带气旋生成频数的相关关系,选取了影响夏季西北太平洋热带气旋活动频数的预测因子,建立了一个夏季西北太平洋热带气旋生成频数的多元回归预测模型。检验结果表明,该模型能较好地拟合1951-2003年夏季西北太平洋热带气旋生成频数的年际变化,拟合率为0.6。对2004-2009年夏季热带气旋生成频数的独立样本预测试验表明,该模型对夏季西北太平洋热带气旋活动频数具有较好的预测能力,可以为热带气旋业务预报提供一定参考。 相似文献
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该文提出一种西北太平洋热带气旋年生成活动的客观预测模型。研究大尺度环境因子对西北太平洋热带气旋年生成频次的作用,使用最小角回归算法对初始14个预测因子进行选择和降维,将资料集分为训练集（1979—2015年）和验证集（2016—2020年）,建立随机森林回归模型预测热带气旋年生成频次。分析环境因子对西北太平洋热带气旋生成位置的作用,使用逐步回归算法筛选影响显著的预测因子,建立局部泊松回归模型预测热带气旋生成空间位置的概率。结果表明:随机森林回归模型可以预测西北热带气旋频次的主要变化和趋势,揭示环境因子对西北太平洋热带气旋年生成频次的影响。局部泊松回归模型对于气旋生成位置概率有一定预测能力。利用随机森林回归模型和局部泊松回归模型模拟1979—2020年西北太平洋热带气旋生成,结果与观测基本一致,可见模型可为热带气旋危险性分析提供参考。 相似文献
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西北太平洋热带气旋移动路径的年际变化及其机理研究 总被引：19，自引：3，他引：19
利用JTWC的热带气旋资料、NCEP/NCAR再分析的风场资料以及Scripps海洋研究所的海温资料分析了西北太平洋热带气旋(TC)移动路径的年际变化及其机理。结果表明,西北太平洋TC移动路径有明显的年际变化并与西太平洋暖池热状态有很密切的关系。当西太平洋暖池处于暖状态,西北太平洋上空TC移动路径偏西,影响中国的台风个数偏多;相反,当西太平洋暖池处于冷状态,西北太平洋的TC移动路径偏东,影响日本的台风个数偏多,而影响中国的台风个数可能偏少。本研究以西太平洋暖池处于冷状态的2004年与西太平洋暖池处于暖状态的2006年的西北太平洋TC移动路径的差别进一步论证了这一分析结果并从动力理论方面分析了在西太平洋暖池不同热状态下,季风槽对赤道西传天气尺度的Rossby重力混合波转变成热带低压型波动(TD型波动)的影响,以此揭示西太平洋暖池的热状态对西北太平洋TC生成位置与移动路径年际变化的影响机理。分析结果表明,当西北太平洋暖池处于暖状态时,季风槽偏西,使得热带太平洋上空对流层低层Rossby重力混合波转变成TD型波动的位置也偏西,从而造成TC生成平均位置偏西,并易于出现西行路径;相反,当西太平洋暖池处于冷状态时,季风槽偏东,这造成了对流层低层Rossby重力混合波转变成TD型波动的区域,以及TC生成的平均位置都偏东,从而导致TC移动路径以东北转向为主。 相似文献
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热带大气季节内振荡对西北太平洋地区热带气旋路径的影响 总被引：3，自引：1，他引：2
利用NOAA的逐日OLR场资料、ECMWF逐日风场(850 hPa)资料、以及美国联合台风预报中心(JTWC)的热带气旋(TC)数据,参考Wheeler和Hendon提出的MJO指数,通过Combined-EOF方法定义热带20～90 d振荡(ISO)的指数,对西北太平洋(WNP)区域进行ISO不同相位的划分,深入研究西北太平洋地区ISO对于热带气旋(TC)路径变化的影响。研究结果表明,在ISO东风位相中,在ISO反气旋性环流东北侧气流影响下,西太副高南侧偏东气流较弱,生成在副高中的TC在140 °E以东转折的比率较大;而在西风位相,副高南侧偏东气流受ISO气旋性环流影响加强,生成在该区域的TC在偏东气流引导下首先向西,当西北移动至近海区域后,在西南季风气流以及副高西侧偏东南气流的共同作用下,容易发生顺时针的北折,因而在140 °E以西转折类的TC比率较高。还分析了台风个例中的ISO流场形势,发现当ISO气旋(反气旋)性环流中心与热带气旋中心重合时,热带气旋路径会发生突然的右折。 相似文献
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The second Madden–Julian Oscillation (MJO) event during the field campaign of the Dynamics of the MJO/Cooperative Indian Ocean Experiment on Intraseasonal Variability in the Year 2011 (DYNAMO/CINDY2011) exhibi ted an unusual double rainband structure. Using a wavenumber-frequency spectral filtering method, we unveil that this double rainband structure arises primarily from the Kelvin wave component. The zonal phase speed of the double rainbands is about 7.9 degree per day in the equatorial Indian Ocean, being in the range of convectively coupled Kelvin wave phase speeds. The convection and circulation anomalies associated with the Kelvin wave component are characterized by two anomalous convective cells, with low-level westerly (easterly) and high (low) pressure anomalies to the west (east) of the convective centers, and opposite wind and pressure anomalies in the upper troposphere. Such a zonal wind–pressure phase relationship is consistent with the equatorial free-wave dynamics. While the free-atmospheric circulation was dominated by the first baroclinic mode vertical structure, moisture and vertical motion in the boundary layer led the convection.The convection and circulation structures derived based on the conventional MJO filter show a different characteristic. For example, the phase speed is slower (about 5.9 degree per day), and there were no double convective branches. This suggests that MJO generally involves multi-scales and it is incomplete to extract its signals by using the conventional filtering technique. 相似文献
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The summer monsoon rainfall over India exhibits strong intraseasonal variability. Earlier studies have identified Madden Julian Oscillation (MJO) as one of the most influencing factors of the intraseasonal variability of the monsoon rainfall. In this study, using India Meteorological Department (IMD) high resolution daily gridded rainfall data and Wheeler?CHendon MJO indices, the intra-seasonal variation of daily rainfall distribution over India associated with various Phases of eastward propagating MJO life cycle was examined to understand the mechanism linking the MJO to the intraseasonal variability. During MJO Phases of 1 and 2, formation of MJO associated positive convective anomaly over the equatorial Indian Ocean activated the oceanic tropical convergence zone (OTCZ) and the resultant changes in the monsoon circulation caused break monsoon type rainfall distribution. Associated with this, negative convective anomalies over monsoon trough zone region extended eastwards to date line indicating weaker than normal northern hemisphere inter tropical convergence zone (ITCZ). The positive convective anomalies over OTCZ and negative convective anomalies over ITCZ formed a dipole like pattern. Subsequently, as the MJO propagated eastwards to west equatorial Pacific through the maritime continent, a gradual northward shift of the OTCZ was observed and negative convective anomalies started appearing over equatorial Indian Ocean. During Phase 4, while the eastwards propagating MJO linked positive convective anomalies activated the eastern part of the ITCZ, the northward propagating OTCZ merged with monsoon trough (western part of the ITCZ) and induced positive convective anomalies over the region. During Phases 5 and 6, the dipole pattern in convective anomalies was reversed compared to that during Phases 1 and 2. This resulted active monsoon type rainfall distribution over India. During the subsequent Phases (7 and 8), the convective and lower tropospheric anomaly patterns were very similar to that during Phase 1 and 2 except for above normal convective anomalies over equatorial Indian Ocean. A general decrease in the rainfall was also observed over most parts of the country. The associated dry conditions extended up to northwest Pacific. Thus the impact of the MJO on the monsoon was not limited to the Indian region. The impact was rather felt over larger spatial scale extending up to Pacific. This study also revealed that the onset of break and active events over India and the duration of these events are strongly related to the Phase and strength of the MJO. The break events were relatively better associated with the strong MJO Phases than the active events. About 83% of the break events were found to be set in during the Phases 7, 8, 1 and 2 of MJO with maximum during Phase 1 (40%). On the other hand, about 70% of the active events were set in during the MJO Phases of 3 to 6 with maximum during Phase 4 (21%). The results of this study indicate an opportunity for using the real time information and skillful prediction of MJO Phases for the prediction of break and active conditions which are very crucial for agriculture decisions. 相似文献
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Boreal summer intraseasonal (30–50 day) variability (BSISV) over the Asian monsoon region is more complex than its boreal winter counterpart, the Madden–Julian oscillation (MJO), since it also exhibits northward and northwestward propagating convective components near India and over the west Pacific. Here we analyze the BSISV in the CMIP3 and two CMIP2+ coupled ocean–atmosphere models. Though most models exhibit eastward propagation of convective anomalies over the Indian Ocean, difficulty remains in simulating the life cycle of the BSISV, as few represent its eastward extension into the western/central Pacific. As such, few models produce statistically significant anomalies that comprise the northwest to southeast tilted convection, which results from the forced Rossby waves that are excited by the near-equatorial convective anomalies. Our results indicate that it is a necessary, but not sufficient condition, that the locations the time-mean monsoon heat sources and the easterly wind shear be simulated correctly in order for the life cycle of the BSISV to be represented realistically. Extreme caution is needed when using metrics, such as the pattern correlation, for assessing the fidelity of model performance, as models with the most physically realistic BSISV do not necessarily exhibit the highest pattern correlations with observations. Furthermore, diagnostic latitude-time plots to evaluate the northward propagation of convection from the equator to India and the Bay of Bengal also need to be used with caution. Here, incorrectly representing extratropical–tropical interactions can give rise to “apparent” northward propagation when none exists in association with the eastward propagating equatorial convection. Despite these cautions, the use of multiple cross-checking diagnostics enables the fidelity of the simulation of the BSISV to be meaningfully assessed. 相似文献
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New diagnostics of the Madden–Julian oscillation (MJO) cycle in ocean temperature and, for the first time, salinity are presented. The MJO composites are based on 4 years of gridded Argo float data from 2003 to 2006, and extend from the surface to 1,400 m depth in the tropical Indian and Pacific Oceans. The MJO surface salinity anomalies are consistent with precipitation minus evaporation fluxes in the Indian Ocean, and with anomalous zonal advection in the Pacific. The Argo sea surface temperature and thermocline depth anomalies are consistent with previous studies using other data sets. The near-surface density changes due to salinity are comparable to, and partially offset, those due to temperature, emphasising the importance of including salinity as well as temperature changes in mixed-layer modelling of tropical intraseasonal processes. The MJO-forced equatorial Kelvin wave that propagates along the thermocline in the Pacific extends down into the deep ocean, to at least 1,400 m. Coherent, statistically significant, MJO temperature and salinity anomalies are also present in the deep Indian Ocean. 相似文献
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The Madden–Julian oscillation (MJO) is observed to interact with moist Kelvin waves. To understand the role of this interaction, a simple scale-interaction model is built, which describes the MJO modulation of moist Kelvin waves and the feedback from moist Kelvin waves through upscale eddy heat and momentum transfer. The backward-tilted moist Kelvin waves produce eddy momentum transfer (EMT) characterized by the lower-tropospheric westerly winds and eddy heat transfer (EHT) that warms the mid-troposphere. The EHT tends to induce the lower-tropospheric easterly winds and low pressure, which is located in front of the “westerly wind burst” induced by the EMT. Adding the eddy forcing to a neutral MJO skeleton model, we show that the EHT provides an instability source for the MJO by warming up the mid-troposphere, and the EMT offers an additional instability source by enhancing the lower-tropospheric westerly winds. The eddy forcing selects eastward propagation for the unstable mode, because it generates positive/negative eddy available potential energy for the eastward/westward modes by changing their thermal and dynamical structures. The present results show that moist Kelvin waves can provide a positive feedback to the MJO only when they are located within (or near) the convective complex (center) of the MJO. The EHT and EMT feedback works positively in the front and rear part of the MJO, respectively. These theoretical results suggest the potential importance of moist Kelvin waves in sustaining the MJO and encourage further observations to document the relationship between moist Kelvin waves and the MJO. 相似文献
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MJO活动对云南5月降水的影响 总被引：5，自引：3，他引：2
本文分析了1979～2008年5月MJO(Madden and Julian Oscillation)不同位相上大尺度环流对流和水汽输送的异常情况及其对云南5月降水的影响。按MJO活动中心位置从西向东分为8个位相, 在不同位相上, 云南5月降水呈现出明显的差异:第4～6位相(MJO对流中心位于赤道印度洋中部至西太平洋)降水偏多, 而第7～8位相(赤道太平洋中部以东)和第1～3位相(赤道印度洋中西部)降水偏少, 其中以第6位相的降水正异常和第2位相的负异常最为显著。在MJO 1～8位相中, 对流主体从热带印度洋东移。在第1～3位相, 孟加拉湾还未形成西南向水汽输送, 而云南又处于水汽辐散区, 降水较少;第4位相时对流主体到达90°N附近, 部分对流云系向孟加拉湾北传, 并在孟加拉湾生成气旋性环流, 向云南输送水汽, 云南降水增多;第5位相时对流主体传到南海, 部分对流云系在南海北传, 同时在南海形成北传的气旋性环流;第6位相时赤道MJO对流主体虽然东移出孟加拉湾, 但孟加拉湾和南海的两个气旋性环流依然继续北传, 孟加拉湾气旋东部的西南风和南海气旋西部的东北风在云南交汇, 云南被强烈的水汽辐合区控制, 降水最充沛。第7～8位相时, 对流主体减弱, 东移到南海和西太平洋一带, 孟加拉湾转向为偏北风, 停止向云南输送水汽, 且云南处于水汽辐散区控制, 降水偏少。因此, MJO主体在东传过程中, 激发了热带对流在孟加拉湾和南海两条通道上的北传, 强盛的水汽输送和两个海区气旋环流的有利配置是造成云南5月降水的重要原因。 相似文献
17.
Increased evidence has shown the important role of Atlantic sea surface temperature (SST) in modulating the El Niño–Southern Oscillation (ENSO). Persistent anomalies of summer Madden–Julian Oscillation (MJO) act to link the Atlantic SST anomalies (SSTAs) to ENSO. The Atlantic SSTAs are strongly correlated with the persistent anomalies of summer MJO, and possibly affect MJO in two major ways. One is that an anomalous cyclonic (anticyclonic) circulation appears over the tropical Atlantic Ocean associated with positive (negative) SSTA in spring, and it intensifies (weakens) the Walker circulation. Equatorial updraft anomaly then appears over the Indian Ocean and the eastern Pacific Ocean, intensifying MJO activity over these regions. The other involves a high pressure (low pressure) anomaly associated with the North Atlantic SSTA tripole pattern that is transmitted to the mid- and low-latitudes by a circumglobal teleconnection pattern, leading to strong (weak) convective activity of MJO over the Indian Ocean. The above results offer new viewpoints about the process from springtime Atlantic SSTA signals to summertime atmospheric oscillation, and then to the MJO of tropical atmosphere affecting wintertime Pacific ENSO events, which connects different oceans. 相似文献
18.
Jian Ling Chongyin Li Wen Zhou Xiaolong Jia 《Theoretical and Applied Climatology》2014,115(1-2):231-241
Mechanisms for convective initiation of the Madden–Julian oscillation (MJO) remain poorly understood. During recent years, <50 % of large-scale convectively active episodes over the tropical Indian Ocean have led to MJO initiation. This study explores the structure and evolution of precipitation, diabatic heating, and potential vorticity (PV) that might be used to tell whether an MJO event will be initiated once such a convection episode occurs. Three different cases are studied. As convection becomes active in a large area over the tropical Indian Ocean, early signs favorable for MJO initiation are apparent: a persistent basin-scale coverage in the zonal direction by positive anomalies in precipitation and diabatic heating (in a swallowtail pattern), a persistent vertical dipole of PV generation with cyclonic (anticyclonic) PV generation in the lower (upper) troposphere covering a zonally extended area, and a cyclonic PV anomaly in the midtroposphere with a cyclonic PV pair straddling the equator immediately west of the diabatic heating center. All these signs are robust in the MJO composite but rarely occur all together in a given MJO case. The likelihood of an MJO event following a convective episode over the tropical Indian Ocean depends on how many of these signs occur and how persistent they are. While a preexisting MJO signal is neither a necessary nor a sufficient sign for MJO initiation, an active convective episode over the tropical Indian Ocean is necessary but insufficient for MJO initiation. MJO initiation depends on detailed convective behaviors over the tropical Indian Ocean. 相似文献
19.
Sensitivity of the Simulated Tropical Intraseasonal Oscillation to Cumulus Parameterizations 
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下载免费PDF全文 The sensitivity of the simulated tropical intraseasonal oscillation or MJO (Madden and Julian oscilla tion)to different cumulus parameterizations is studied by using an atmospheric general circulation model (GCM)-SAMIL(Spectral Atmospheric Model of IAP LASG).Results show that performance of the model in simulating the MJO alters widely when using two different cumulus parameterization schemes-the moist convective adjustment scheme(MCA)and the Zhang-McFarlane(ZM)scheme.MJO simulated by the MCA scheme was found to be more realistic than that simulated by the ZM scheme.MJO produced by the ZM scheme is too weak and shows little propagation characteristics.Weak moisture convergence at low levels simulated by the ZM scheme is not enough to maintain the structure and the eastward propagation of the oscillation.These two cumulus schemes produced different vertical structures of the heating profile.The heating profile produced by the ZM scheme is nearly uniform with height and the heating is too weak compared to that produced by the MCA,which maybe contributes greatly to the failure of simulating a reasonable MJO.Comparing the simulated MJO by these two schemes indicate that the MJO simulated by the GCM is highly sensitive to cumulus parameterizations implanted in.The diabatic heating profile plays an important role in the performance of the GCM.Three sensitivity experiments with different heating profiles are designed in which modified heating profiles peak respectively in the upper troposphere(UH), middle troposphere(MH),and lower troposphere(LH).Both the LH run and the MH run produce eastward propagating signals on the intraseasonal timescale,while it is interesting that the intraseasonal timescale signals produced by the UH run propagate westward.It indicates that a realistic intraseasonal oscillation is more prone to be excited when the maximum heating concentrates in the middle-low levels,especially in the middle levels,while westward propagating disturbances axe more prone to be produced when the maximum heating appears very high. 相似文献
20.
Convection activity over the Guinean coast and Central Africa during northern spring from synoptic to intra-seasonal timescales 总被引：1，自引：1，他引：0
This study proposes an overview of the main synoptic, medium-range and intraseasonal modes of convection and precipitation in northern spring (March–June 1979–2010) over West and Central Africa, and to understand their atmospheric dynamics. It is based on daily National Oceanic and Atmospheric Administration outgoing longwave radiation and Cloud Archive User Service Tb convection data, daily TRMM and Global Precipitation Climatology Project rainfall products and daily ERA-Interim reanalysis atmospheric fields. It is first shown that mesoscale convective systems can be modulated in terms of occurrences number and intensity at such time scales. Based on empirical orthogonal function analyses on the 2–90-day filtered data it is shown that the main mode of convective and rainfall variability is located along the Guinean coast with a moderate to weak extension over Central Africa. Corresponding regressed deseasonalised atmospheric fields highlight an eastward propagation of patterns consistent with convectively coupled equatorial Kelvin wave dynamics. Then a singular spectrum analysis combined with a Hierarchical Ascendant Classification enable to define objectively the main spectral bands of variability within the 2–90-day band, and highlight three main bands, 2–8-, 8–22- and 20–90-day. Within these three bands, space–time spectral decomposition is used to identify the relative impacts of convectively coupled equatorial Kelvin, Rossby and inertia–gravity waves, as well as Madden–Julian Oscillation (MJO) signal. It confirms that eastward propagating signals (convectively coupled equatorial Kelvin wave and MJO) are highly dominant in these convection and precipitation variability modes over the Guinean coast during northern spring. So, while rain-producing individual systems are moving westward, their activity are highly modulated by sub-regional and regional scales envelops moving to the east. This is a burning issue for operational forecasting centers to be able to monitor and predict such eastward propagating envelops of convective activity. 相似文献