Atmospheric input of trace elements to the western Pacific Ocean and the Kuroshio ocean area

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ESTIMATES OF SEA SURFACE FLUXES DURING TOGA-COARE IOP

With the marine ship observation data set obtained by three cruise-phases of Chinese Xi-angyanghong 5 from November 5,1992 to February 19,1993 in the TOGA-COARE IOP at 2°S,156°E.the sea surface fluxes at this point are estimated by three different bulk schemes.Firstly.aquasi-linear relation is found between the neutral drag coefficients and wind speed.Then,the sta-bility-dependent drag and heat transfer coefficients are solved in the iterative method.Based onthus-derived transfer coefficients,the momentum,sensible and latent heat fluxes are calculated.In the warm pool region,the fluxes corresponding to the westeily winds are much greater thanthose of the easterly trade winds.The magnitude of sea surface fluxes depends upon the atmo-spheric stability as well,in particular in the case of weak wind condition.The estimated sea sur-face net heat budget shows that considerable amount of heat transport from ocean to atmosphere ismainly produced by the effective longwave radiation,latent and sensible heat fluxes.Among themthe value of latent heat flux is the largest and the sensible heat flux is the smallest.Finally,an ac-curacy analysis is made by direct measurements with the eddy-correlation method on the JapaneseR/V Hakuho board at the same time.It is shown that the bulk-derived fluxes are acceptable withmuch confidence.The estimated effective longwave radiation is used to compare with those by di-rect observations on Xiangyanghong 5.This research is compared with TOGA investigation in thetropical western Pacific.     

A study of a fair weather boundary layer in TOGA-COARE: Parameterization of surface fluxes in large scale and regional models for light wind conditions

The study focuses on a way to parameterize the effect of subgrid scale convective motions on surface fluxes in large scale and regional models for the case of light surface winds. As previously proposed, these subgrid effects are assumed to scale with the convection intensity through the relationship: where is the mean velocity of the wind, U₀ the velocity of the mean wind, w_* the free convection velocity, and an empirical coefficient to be determined. Both observations and numerical simulation are presently used to determine the free convection coefficient .Large eddy simulation of a fair weather convective boundary layer case observed during TOGA-COARE is performed. Comparisons between observations and the simulation of surface properties and vertical profiles in the planetary boundary layer are presented. The simulated vertical turbulent fluxes of heat, moisture and buoyancy range well within estimates from aircraft measurements.The most important result is that the true free convection coefficient , directly estimated from simulation, leads to a value of 0.65, smaller than the ones estimated from temporal and spatial variances. Using observations and simulation, estimates of from temporal and spatial variances are obtained with similar values 0.8. From both theoretical derivations and numerical computations, it is shown that estimates of the true from variances are possible but only after applying a correction factor equal to 0.8. If this correction is not used, is overestimated by about 25%. The time and space sampling problem is also addressed in using numerical simulations.     

Short-term variabilities of upper ocean current in the warm pool region during TOGA/COARE IOP

Oceanic current data in the warm pool region of the western equatorial Pacific measured by upward-looking moored Acoustic Doppler Current Profilers at two equatorial sites (147°E and 154°E) and two off-equatorial sites (2°N and 2°S, 156°E) during TOGA/COARE Intensive Observing Period (IOP) from November 1992 to February 1993 are used to examine short-term variabilities in the upper layer above 160–240 m. In time series of the zonal and meridional currents in many layers, spectral peaks are found at periods around 2 days and 4 days in addition to high energies in a period range longer than 10 days. The signal with the period of about 2 days has significantly high energies at all sites, and its magnitude is higher for the meridional current than for the zonal one. This signal is especially active in the first half of IOP from November to December in 1992. In this period, the quasi-2-day signal in the current field is coherent between northern (2°N) and southern (2°S) stations, but it has no evident relationship with that in the surface wind field around the stations. The quasi-4-day signal with the period of about 4 days has highest energies in layers above 160 m at the southern station, and is coherent between northern and southern stations. Besides, the signal at the station of 2°S has a significantly high coherence with that in the wind at the southern station, suggesting that it is a local phenomenon.     

Variability of thermohaline structure at 4°S, 156°E during TOGA COARE IOP

The thermohaline structure at 4°S, 156°E was analyzed based on CTD data acquired during the TOGA COARE Intensive Observing Period (IOP) from November, 1992 to February, 1993. The ocean responses during two Madden-Julian Oscillation (MJO) events were preliminarily studied based on meteorological field observation. The main water masses at the observation point were Tropical Surface Water, Southern Subtropical Lower Water and Southern Intermediate Water from surface downward. There was good correlation of sea surface temperature with the wind field, and of the surface salinity with wind speed and rainfalls. Both of the two surface variables were also modulated by upwelling caused by westerly winds at the observation point. The isohaline layer was not always shallower than the isothemal layer in this observation and could be considered as the lower limit of the diurnal variation of the isothernal layers in most cases. The existence of large variations of the maximum salinity core is suggested to be related to the meridional motion in that depth. Contribution No. 2264 from the Institute of Oceanology, Chinese Academy of Sciences. This project was supported by NSFC (No. 49176255).     

印度洋通道及其对中国地缘环境影响

印度洋通道是中国获取能源和其他资源、出口工业产品并同南亚、西亚、非洲和欧洲国家交流合作的生命线。随着中美关系和中国周边地缘态势的深刻变化,中国需要积极谋划逐渐降低对传统的南海—马六甲海峡通道的依赖,建设新的印度洋通道,从而降低自身的地缘环境风险,并由此优化国内经济发展布局,推动西南沿边地区进一步开发与开放,并提升中国同印度洋沿岸国家和地区的交流与合作水平。本研究从通道的定义和特征出发,梳理了现有及潜在的印度洋通道,比较分析了各条通道的战略意义、前景及地缘环境影响,从而为中国的印度洋战略构建和“一带一路”倡议推进提供新的视角和见解。     

TOGA－COARE强化期（IOP）西太平洋海域的辐射特征

该文利用ＴＯＧＡ－ＣＯＡＲＥ强化观测期（ＩＯＰ）所获得的辐射观测资料（１９９２年１１月１０日—１９９３年２月１８日），对考察点（２°１５′Ｓ，１５８°００′Ｅ）的辐射分量进行了分析，其中包括总辐射、直接辐射、散射辐射、海表长波辐射、大气逆辐射、海表反射辐射及其反照率、净辐射及有效辐射。结果表明：和其它地区（如高原）比较，观测点的总辐射、直接辐射均很强；反射率小，晴天平均为０．０４—０．０５，阴天为０．０６—０．０８；海表长波辐射大而日变化小，大气逆辐射强而日变化大；有效辐射小而净辐射大。     

资源02C卫星P／MS相机内方位几何标定方法研究

为解决国产资源02C卫星影像相机内方位几何标定问题,提出了一种利用公众地理信息数据进行高精度相机内方位在轨几何标定的方法。该方法利用资源02C卫星影像与公众地理信息数据自动配准获取的海量地面控制点并进行附加自检校参数的最小二乘平差,实现了资源一号02C卫星P／Ms相机的内方位标定,精度可以达到子像素级。     

TOGA-COARE IOP期间赤道西太平洋海表壁垒层的研究

根据“向阳红五号”调查船于１９９２－１９９３年ＴＯＧＡ－ＣＯＡＱＲＥ（Ｔｒｏｐｉｃａｌ Ｏｃｅａｎ ａｎｄ Ｇｌｏｂａｌ Ａｔｍｏｓｐｈｅｒｅ－Ｃｏｕｐｌｅｄ Ｏｃｅａｎ Ａｔｍｏｓｐｈｅｒｅ Ｒｅｓｐｏｎｓｅ Ｅｘｐｅｒｉｍｅｎｔ）强化观测期（ＩＯＰ）期间,在赤道西太平洋观测到的ＣＴＤ,海面气象等资料,计算了海表ｂａｒｒｉｅｒ ｌａｙｅｒ（壁垒层）厚度。并对该海区壁垒层厚度的变化特征及机制作初步     

TOGA-COARE IOP部分观测资料初步分析

初步分析中国科学院南海海洋研究所《实验3号》科学考察船在TOGA—COARE IOP连续三个航次中部分CTD和ADCP原始观测资料指出:90-210m间大于35的盐度极值除存在准日周期变化外,在量值上还存在约73d的周期变化。但受资料长度的限制,目前尚无法确定上述周期是否属于稳定周期。在上述深度范围内亦存在较低盐度和温度水体侵入现象,其强度存在10—15d的周期变化。等温线和等密度线常出现振幅达10m以上,周期约3d的振荡,而且有时表现出次中尺度涡(submesoscale eddy)及涡旋链特征。比较风、SST、混合层深度间的关系时发现,风强度和大风维持时间对SST和混合层深度的影响很大,如西风暴发过程可使平均SST降低0.5℃左右,使平均混合层深度加深8m以上。分析西风暴发过程及西风暴发后洋流铅垂变化和洋流随时间变化发现,西风暴发过程导致79m以浅深度上的东向射流,且19m深处流动随时间顺时针改向,79m深处流动随时间逆时针方向改向。