天津港水域围垦条件下的水动力变化分析     

陈丹茜  兰庭飞  裴艳东  杜家笔  汪亚平  高建华 《海洋科学》2019,43(10):113-125

本研究旨在讨论天津滨海新区的围垦对其附近水域水动力和悬沙输运所造成的影响,并进行定量评估。在天津港南部、北部海域分别选取4个站位进行了全潮水文观测,获取了流速剖面、悬沙浓度剖面数据,并据此计算了底切应力、潮不对称性以及余流。结果表明,底部悬沙浓度与流速、底切应力存在相位一致性,绝大部分站位的沉积物都呈现向岸净输运的趋势,悬沙通量分解显示潮汐捕捉项是该区域悬沙输运的主要贡献项;围垦愈增的2009～2015年,天津港北部潮不对称性增强,向陆的单宽悬沙输运率由20.15 g/(m·s)变至24.92 g/(m·s),而南部海域潮不对称性减弱,向陆的单宽悬沙输运率从37.75 g/(m·s)减小至6.37 g/(m·s)。综上,持续地围垦可能导致天津港附近海域的水动力条件改变,推测北部潮滩淤涨可能加快,而南部淤涨速率减小。  相似文献   

Assessing the relative contributions of the flood tide and the ebb tide to tidal channel network dynamics     

Liang Geng  Zheng Gong  Zeng Zhou  Stefano Lanzoni  Andrea D'Alpaos 《地球表面变化过程与地形》2020,45(1):237-250

Flood and ebb currents provide different contributions to the initiation and evolution of tidal channel networks, generating diverse network structures and channel cross-sections. In order to separate the effects of these contributions, a physical model of a sloping tidal-flat basin was set up in the laboratory. Depending on the degree of tidal asymmetry imposed offshore, either flood or ebb currents can be enhanced. The experimental results show that the ebb current has a higher capability to initiate and shape tidal networks than the flood current. Headward erosion is mainly induced by the ebb flow. The slightly inclined flat surface tends to reduce the energy of the flood current and to enhance the ebb current, thus prolonging the duration of morphodynamic activity as well as sediment motion. Overall, flood-dominated tides favour the formation of small-scale channel branches in the upper basin zone, while long lasting ebb-dominated tides result in more complex, wider and deeper tidal networks. © 2019 John Wiley & Sons, Ltd.  相似文献   

热带东印度洋SST对气候变暖和变冷的响应     

徐杉  罗义勇 《海洋学报(英文版)》2019,38(5):76-85

The response of the eastern tropical Indian Ocean(ETIO) to heat fluxes of equal amplitude but opposite sign is investigated using the Community Earth System Model(CESM). A significant positive asymmetry in sea surface temperature(SST) is found over the ETIO—the warming responses to the positive forcing exceeds the cooling to the negative forcing. A mixed layer heat budget analysis is carried out to identify the mechanisms responsible for the SST asymmetry. Results show that it is mainly ascribed to the ocean dynamical processes, including vertical advections and diffusion. The net surface heat flux, on the contrary, works to reduce the asymmetry through its shortwave radiation and latent heat flux components. The former is due to the nonlinear relationship between SST and cloud, while the latter is resulted mainly from Newtonian damping and air-sea stability effects. Changes in the SST skewness are also evaluated, with more enhanced negative SST skewness over the ETIO found for the cooling than heating scenarios due to the asymmetric thermocline-SST feedback.  相似文献   

The Asymmetry of Subsurface Temperature Anomalies Associated with ENSO in the Equatorial Western Pacific          下载免费PDF全文

HUA Li-Juan  YU Yong-Qiang 《大气和海洋科学快报》2015,8(1):23-28

The phenomenon of ENSO asymmetry has been recognized for many years, but most studies have focused on the asymmetry of surface temperature anomalies in the equatorial eastern Pacific. Here, the authors investigate the temperature asymmetry associated with ENSO in the subsurface of the western Pacific through analysis of observations and numerical experiments with an ocean GCM. Both the observation and simulation exhibit significant ENSO asymmetry, characterized by negative temperature skewness in the equatorial western Pacific and positive skewness in the eastern Pacific. Heat budget analysis reveals that nonlinear dynamical heating results in the positive temperature asymmetry in the equatorial eastern Pacific, but tends to weaken the negative temperature asymmetry in the equatorial western Pacific. The climatological meridional current transports the temperature anomalies and corresponding negative asymmetry from the off-equator region to the equator in the subsurface of the western Pacific. Through a sensitivity experiment with reversed wind stress forcing, the authors suggest that the skewness of the wind stress anomalies does not contribute to the negative temperature asymmetry in the western Pacific in the first-order approximation, while the internal nonlinear dynamics does play a key role. The study suggests that, as a result of nonlinear processes, the oceanic responses to anomalous wind stress are nonlinear and asymmetric in the tropical Pacific.  相似文献   

Optimal Perturbations Triggering Weather Regime Transitions: Onset of Blocking and Strong Zonal Flow   总被引：1，自引：0，他引：1  

JIANG Zhin  MU Mu  WANG Donghai 《大气科学进展》2011,28(1):59-68

In this paper, the approach proposed by Mu and Jiang (2008) to obtain the optimal perturbations for triggering blocking (BL) onset is generalized to seek the optimal perturbations triggering onset of the strong zonal flow (SZF) regime. The BL and SZF regimes are characterized by the same dipole-like anomaly pattern superposed on the climatological flow, but with opposite sign. The results show that this method is also superior at finding the initial optimal perturbations triggering onset of the SZF regime, especially in the medium range. Furthermore, by comparing the two kinds of conditional nonlinear optimal perturbations (CNOPs) trig-gering onset of BL and SZF regimes, we find that in the linear approximation, there is symmetry in the sensitivities for BL and SZF onset, and the perturbations that optimally trigger onset of BL and SZF regimes at times when linear approximation is valid are also characterized by the same spatial pattern but with opposite sign. Whereas when the optimization time is extended to 6 days, the two kinds of CNOPs lose their out-of-phase behavior. The nonlinearity results in an asymmetry between the sensitivity for BL and SZF onset. Additionally, we find that the optimal perturbations have one common property, which is that the second baroclinic mode contributes more to the initial perturbations while the barotropic mode dominates the final structures.  相似文献   

河口往复流中潮流不对称与推移质输沙的关系   总被引：2，自引：0，他引：2  

李谊纯  董德信  陈波 《海洋科学》2015,39(6):99-103

潮流不对称现象是近岸潮波运动的基本特征之一,为了研究潮流不对称对推移质泥沙长期净输运的作用机制,首先在往复流情况下对Bagnold推移质输沙率公式(1966)由于不包含起动流速所可能导致的误差进行理论分析,进而由统计学中的"偏度"的概念出发,推导了河口潮流不对称与推移质输沙之间的定量关系。研究认为,虽然Bagnold推移质输沙率公式不包含泥沙起动流速,但是只要泥沙起动流速和最大流速的比值在一定范围内,则在理论上公式的计算误差是可以接受的。由偏度结合Bagnold公式导出了潮流不对称与推移质输沙之间的关系,表明推移质泥沙的长期净输运不仅与余流有关,而且与不同分潮组合之间、余流与分潮之间的相互作用紧密相关。该关系还给出了一个由潮流调和常数估算河口推移质输沙的简便方法。经对比,从潮流不对称出发估算推移质输沙与直接采用推移质输沙率公式结果一致。  相似文献   

中近磁尾等离子体片统计特性研究   总被引：1，自引：0，他引：1       下载免费PDF全文

张帅  田安民  史全岐  孙为杰  尧中华  傅绥燕  宗秋刚  濮祖荫 《地球物理学报》2016,59(2):411-418

本文使用Cluster-C1卫星的CIS仪器和FGM仪器测量得到的质子通量数据和计算的β数据,判断Cluster卫星在地球磁尾不同位置位于等离子体片内的概率.使用2001—2004年7—11月的Cluster-C1数据,分别在行星际磁场南向和北向时,得出X-10RE区域内卫星位于等离子体片的概率在Y-Dz平面的分布图(Dz是卫星到中性片的距离).通过对比行星际磁场南向和北向时的卫星位于等离子体片的概率的分布图,我们发现等离子体片在行星际磁场南向时比在行星际磁场北向时要薄,并且这个效应在磁尾晨昏两侧比在午夜附近明显,同时我们还发现等离子体片在晨侧比在昏侧厚.  相似文献   

Asymmetry in oceanic crustal structure of the South China Sea basin and its implications on mantle geodynamics     

Fan Zhang  Xubo Zhang  Weiwei Ding  Tingting Wang  Jian Zhu 《International Geology Review》2020,62(7-8):840-858

ABSTRACT

We investigated the oceanic crustal structure and lithospheric dynamics of the South China Sea (SCS) basin through a comprehensive analysis of residual gravity anomaly and bathymetry combined with seismic constraints and interpretation from geodynamic modelling. We first calculated the residual mantle Bouguer anomaly (RMBA) of the oceanic crustal regions of the SCS by removing from free-air gravity anomaly the predicted gravitational attractions of water-sediment, sediment-crust, and crust-mantle interfaces, as well as the effects of lithospheric plate cooling, using the latest crustal age constraints including IODP Expedition 349 and recent deep-tow magnetic surveys. We then calculated models of the gravity-derived crustal thickness and calibrated them using the available seismic refraction profiles of the SCS. The gravity-derived crustal thickness models correlate positively with seismically determined crustal thickness values. Our analysis revealed that the isochron-averaged RMBA are consistently more negative over the northern flank of the SCS basin than the southern conjugate for magnetic anomaly chrons C8n (~25.18 Ma) to C5Dn (~17.38 Ma), implying warmer mantle and/or thicker crust over much of the northern flank. Computational geodynamic modelling yielded the following interpretations: (1) Models of asymmetric and variable spreading rates based on the relatively high-resolution deep-tow magnetic analysis would predict alternating thicker and thinner crust at the northern flank than the southern conjugate, which is inconsistent with the observed systematically thicker crust on the northern flank. (2) Models of episodic southward ridge jumps could reproduce the observed N-S asymmetry, but only for crustal age of 23.6–20 Ma. (3) Southward migration of the SCS ridge axis would predict slightly thinner crust at the northern flank, which is inconsistent with the observations. (4) Models of higher mantle temperatures of up to 25–50°C or >2% less depleted mantle sources on the northern flank could produce large enough anomalies to explain the observed N-S asymmetries.  相似文献   

Observations of asymmetry in contrasting wave‐ and tidally‐dominated environments within a mesotidal basin: implications for estuarine morphological evolution          下载免费PDF全文

Stephen Hunt  Karin R. Bryan  Julia C. Mullarney  Mark Pritchard 《地球表面变化过程与地形》2016,41(15):2207-2222

Tides are often considered to be the dominant hydrodynamic process within mesotidal estuaries although waves can also have a large influence on intertidal erosion rates. Here, we use a combination of hydrodynamic measurements and sediment deposition records to determine the conditions under which observed waves are ‘morphologically significant’, in which case they influence tidal and suspended sediment flux asymmetry and subsequently infilling over geomorphological timescales. Morphological significant conditions were evaluated using data from contrasting arms in a dendritic mesotidal estuary, in which the orientation of the arms relative to the prevailing wind results in a marked difference in wave conditions, deposition rates and morphology. By defining the morphological significance of waves as a product of the magnitude of bed shear stress and frequency of occurrence, even small (but frequently occurring) winds are shown to be capable of generating waves that are morphologically significant given sufficient fetch. In the arm in which fetch length is restricted, only stronger but rare storm events can influence sediment flux and therefore tides are more morphologically significant over longer timescales. Water depth within this mesotidal estuary is shown to be a critical parameter in controlling morphological significance; the rapid attenuation of short period waves with depth results in contrasting patterns of erosion occurring during neaps and accretion during springs. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

Hemispheric asymmetry of sunspot area in solar cycle 23 and rising phase of solar cycle 24: Comparison of three data sets     

《New Astronomy》2015

Analysis of long-term solar data from different observatories is required to compare and confirm the various level of solar activity in depth. In this paper, we study the north–south asymmetry of monthly mean sunspot area distribution during the cycle-23 and rising phase of cycle-24 using the data from Kodaikanal Observatory (KO), Michelson Doppler Imager (MDI) and Solar Optical Observing Network (SOON). Our analysis confirmed the double peak behavior of solar cycle-23 and the dominance of southern hemisphere in all the sunspot area data obtained from three different resources. The analysis also showed that there is a 5–6 months time delay in the activity levels of two hemispheres. Furthermore, the wavelet analysis carried on the same data sets showed several known periodicities (e.g., 170–180 days, 2.1 year) in the north–south difference of sunspot area data. The temporal occurrence of these periods is also the same in all the three data sets. These results could help in understanding the underlying mechanism of north–south asymmetry of solar activity.  相似文献