A long-term record of photosynthetically available radiation (PAR) and total solar energy at 38.6°N, 78.2°W

Photosynthetically available radiation (PAR; 400–700 nm, E m⁻² d⁻¹) is the fraction of the total solar energy (Mjoules m⁻² d⁻¹) that is used by organisms for photosynthesis and vision. We present a statistical summary of a 17-yr time series of PAR data (1982–1998) collected near Chesapeake Bay as well as a second set of data on PAR and total solar energy gathered over a shorter time span (1997–1998). The time series data (5,126 daily totals) varied between 1–67 E m⁻² d⁻¹ and were used to estimate the minimum and maximum values of PAR as a function of day of the year. In monthly frequency distributions of the PAR data, three modes were observed corresponding to sunny, partly cloudy, and overcast days. The second set of PAR and total solar energy data were used to examine the ratio of PAR to total solar energy, which was 2.04 E Mjoule⁻¹ for PAR between 10 and 70 E m⁻² d⁻¹. On overcast days, the ratio increased to as high as 3 E Mjoule⁻¹ as PAR increased in importance as a fraction of the total solar energy. These values were consistent with others in the literature, and the relationships reported here can be used to predict the climatology of PAR and total solar energy within the Chesapeake region. The PAR data were also combined with reported minimum values of PAR for net primary production in the surface mixed layer of the water column of aquatic systems to estimate the combinations of mixed layer depth and diffuse attenuation coefficient (number of optical depths) under which light limitation of phytoplankton primary production is expected to occur.     

Ice ages and the thermal equilibrium of the earth,II

The energy required to sustain midlatitude continental glaciations comes from solar radiation absorbed by the oceans. It is made available through changes in relative amounts of energy lost from the sea surface as net outgoing infrared radiation, sensible heat loss, and latent heat loss. Ice sheets form in response to the initial occurrence of a large perennial snowfield in the subarctic. When such a snowfield forms, it undergoes a drastic reduction in absorbed solar energy because of its high albedo. When the absorbed solar energy cannot supply local infrared radiation losses, the snowfield cools, thus increasing the energy gradient between itself and external, warmer areas that can act as energy sources. Cooling of the snowfield progresses until the energy gradients between the snowfield and external heat sources are sufficient to bring in enough (latent plus sensible) energy to balance the energy budget over the snowfield. Much of the energy is imported as latent heat. The snow that falls and nourishes the ice sheet is a by-product of the process used to satisfy the energy balance requirements of the snowfield. The oceans are the primary energy source for the ice sheet because only the ocean can supply large amounts of latent heat. At first, some of the energy extracted by the ice sheet from the ocean is stored heat, so the ocean cools. As it cools, less energy is lost as net outgoing infrared radiation, and the energy thus saved is then available to augment evaporation. The ratio between sensible and latent heat lost by the ocean is the Bowen ratio; it depends in part on the sea surface temperature. As the sea surface temperature falls during a glaciation, the Bowen ratio increases, until most of the available energy leaves the oceans as sensible, rather than latent heat. The ice sheet starves, and an interglacial period begins. The oscillations between stadial and interstadial intervals within a glaciation are caused by the effects of varying amounts of glacial meltwater entering the oceans as a surface layer that acts to reduce the amount of energy available for glacial nourishment. This causes the ice sheet to melt back, which continues the supply of meltwater until the ice sheet diminishes to a size consistent with the reduced rate of nourishment. The meltwater supply then decreases, the rate of nourishment increases, and a new stadial begins.     

青藏高原林芝与四川盆地温江地区晴天辐射和能量平衡特征

分析了2008年青藏高原林芝地区与四川盆地温江地区无降水条件下地表辐射、 湍流通量和地表反照率的日变化及月际变化特征, 并探讨了季风过程对其产生的影响.结果表明: 林芝与温江地区地表辐射和湍流通量都具有明显的日变化和月际变化周期, 季风期受云的影响, 日循环规律变得不是非常规则.季风对林芝地区地表能量分配影响极大, 季风前感热通量占主导地位, 季风期和季风后(夏、 秋节)潜热通量是净辐射的主要消耗项; 温江地区全年潜热在净辐射的分布中占主导地位, 感热通量的作用和土壤热通量相当. 林芝地区年平均地表反照率为0.21, 温江地区年平均仅为0.14; 季风前(3-5月)、 季风中(6-7月)和季风后(8-9月), 林芝地区的地表反照率分别为0.20、 0.19和0.20, 温江地区的地表反照率分别为0.13、 0.11和0.14.     

南海海-气通量交换研究进展

1998年的"南海季风试验(SCSMEX)"已经过去10年了,SCSMEX启动的南海海-气通量试验研究也有10个年头.在SCSMEX和国家自然科学基金面上项目"南海季风爆发期近海面层通量观测和湍流结构的观测研究"支持下,10年来在西沙实施了3次(1998年、2000年、2002年)海-气通量观测试验,开展了试验资料分析研究,重点是西南季风爆发前后海-气通量交换过程研究,辐射通量、感热通量、潜热通量、动量通量随天气条件的变化研究,海-气通量日变化,通量交换系数以及通量变化对低层大气、上层海洋的影响研究.对10年来南海通量研究作一回顾,对未来的通量观测研究计划特别是2008"亚洲季风年"西沙通量观测提出一些建议.     

黄河源鄂陵湖地区辐射收支和地表能量平衡特征研究

利用2010年6-7月鄂陵湖野外试验的近地层观测数据,分析了在不同天气条件下黄河源鄂陵湖地区辐射分量、地表能量分量、土壤温度和反照率的变化特征. 结果表明：不同天气条件下,辐射和地表能量各分量日变化差异较大,晴天、阴天和雨天的地表反照率依次递减,平均反照率约为0.21;观测期内,平均辐射贡献从大到小依次为向上长波、向下长波、向下短波、向上短波,日积分值分别为31.4 MJ·m^-2、25.6 MJ·m^-2、22.4 MJ·m^-2、4.2 MJ·m^-2,净辐射(12.5 MJ·m^-2)占向下短波辐射的55.7%;平均地表能量和土壤温度的变化幅度较晴天小,感热、潜热、0 cm土壤热通量的平均日积分值分别占净辐射的21.2%、43.1%、8.2%;平均土壤温度变化幅度随深度增加逐渐减小,浅层土壤温度峰值较晴天低2 ℃,深层土壤温度相差不大. 云和降水的扰动削弱了向下短波辐射,导致平均感热通量和0 cm土壤热通量的峰值比晴天小,而平均潜热通量的峰值大于晴天. 由于湖泊水体巨大的热容量和水分供应,鄂陵湖地区的气温日较差较小,地表温度变化幅度变小,附近地表温度升高缓慢. 鄂陵湖区的地表能量平衡中,潜热通量占主导,感热和地表土壤热通量次之. 研究结果有助于理解气候变化背景下黄河源区湖泊的能量水分循环过程,为促进该地区光热资源的合理利用和畜牧业的可持续发展提供数据支持.     

Chlorophyll modulation of mixed layer thermodynamics in a mixed-layer isopycnal General Circulation Model — An example from Arabian Sea and equatorial Pacific

Western tropical Indian Ocean, Arabian Sea, and the equatorial Pacific are known as regions of intense bio-chemical-physical interactions: the Arabian Sea has the largest phytoplankton bloom with seasonal signal, while the equatorial Pacific bloom is perennial with quasi-permanent upwelling. Here, we studied three dimensional ocean thermodynamics comparing recent ocean observation with ocean general circulation model (OPYC) experiment combined with remotely sensed chlorophyll pigment concentrations from the Coastal Zone Color Scanner (CZCS). Using solar radiation parameterization representing observations that a higher abundance of chlorophyll increases absorption of solar irradiance and heating rate in the upper ocean, we showed that the mixed layer thickness decreases more than they would be under clear water conditions. These changes in the model mixed layer were consistent with Joint Global Ocean Flux Study (JGOFS) observations during the 1994-1995 Arabian Sea experiment and epi-fluorescence microscopy (EFM) on samples collected during Equatorial Pacific Ocean Climate Study (EPOCS) in November, 1988. In the Arabian Sea, as the chlorophyll concentrations peak in October (3 mg/m³) after the summer plankton bloom induced by coastal upwelling, the chlorophyll induced biological heating enhanced the sea surface temperature (SST) by as much as 0.6‡C and sub-layer temperature decreases and sub-layer thickness increases. In the equatorial Pacific, modest concentrations of chlorophyll less than 0.3 mg/m³ is enough to introduce a meridional differential heating, which results in reducing the equatorial mixed layer thickness to more than 20 m. The anomalous meridional tilting of the mixed layer bottom enhances off equatorial westward geostrophic currents. Consequently, the equatorial undercurrent transports more water from west to east. We proposed that these numerical model experiments with use of satellite andin situ ocean observations are consistent under three dimensional ocean circulation theory combined with solar radiation transfer process.     

Advances in Studying the Sea-Air Dimethysulphide Exchange Process in the Southern Ocean

Dimethylsulphide (DMS) is an important marine biogenic gas and can be released into atmosphere through sea air gas exchange. The oxidants of DMS in atmosphere are the main compounds of pristine marine sulphate aerosols and would affect the global climate change finally. Almost all the atmospheric DMS, about 90%, comes from the ocean. The southern ocean, which consists about 20% of the whole ocean area, is one of the largest atmospheric DMS sources. In contrast with the other oceans, the Southern Ocean appears great spatial and temporal variability of surface seawater DMS. In addition, there are the complex hydrography system, variable sea ice condition and various biologic activities in the Southern Ocean as to make survey and understand DMS as well as its controlling factors most difficult. Moreover, it is significant to integrate the DMS sea ice exchange processes and its controlling factors studies. In order to develop survey and research on the sea air DMS exchange and biogeochemistry processes, estimate methods of the sea air DMS fluxes will be reviewed, characteristics of the spatial and temporal distribution of surface seawater DMS will be discussed and the sea air DMS flux in the Southern Ocean will be assessed. Finally, major controlling factors of DMS sea air DMS processes will also be analyzed.     

北极沿岸地区水体中氢氧稳定同位素组成及水分转化过程研究

2010年7月参加第三届北京中学生北极科学考察活动,收集了北极沿岸地区的挪威斯瓦尔巴德群岛(Svalbard)、冰岛、格陵兰沿岸地区的海水、沿岸海水、海冰表面冰样、地表径流等水体样品,对样品进行了氢氧稳定同位素成分测定,分析了北极沿岸地区水体的水循环过程.结果表明,该地区不同水体中的稳定同位素具有不同特征.沿岸海水中δ...     

Mercury concentrations in environmental media at a hazardous solid waste landfill site and mercury emissions from the site

Mercury (Hg) concentrations in air, effluent water, landfill gas, leachate, groundwater, and soil at a hazardous solid waste landfill site in Korea were measured along with air–soil surface Hg exchange fluxes at the site. The concentrations and fluxes were considerably higher than have been found elsewhere in Korea. Gaseous Hg concentrations in the air peaked during the day, coinciding with Hg being released from the landfill surface. This suggests that air–soil exchange increased the Hg concentrations in the atmosphere. The air–soil exchange flux increased abruptly when solar radiation reached the soil surface. The Hg flux peaked about 3 h before the solar radiation peaked, possibly because reducible Hg was abundant at the soil surface. The Hg emission flux activation energy (E _a) was low, indicating that the Hg species present and Hg–soil binding were probably not as important (because of the high Hg content of the soil) as in previous studies. The methylmercury to total Hg ratios in the discharged effluent, groundwater, and leachate was clearly higher than typically found in coastal water and freshwater, suggesting bacteria caused active methylation to occur under the reducing conditions in the anaerobic landfill. The results suggested that considerable amounts of Hg are probably transported from the landfill to nearby environmental media and that this will continue if waste with a high Hg content continues to be added to the landfill without being pretreated.     

青藏铁路沿线地表和路基表面热力学模式(Ⅲ):参数化方案

以物理过程分析为基础,根据野外实测资料设计了青藏铁路沿线地表和路基表面热力学模式中的大气辐射参数化方案,对直接太阳辐射、大气散射辐射、大气向下长波辐射参数进行处理,得到了较好的结果.在无云大气条件下,对直接太阳辐射透过率和大气散射辐射以太阳天顶角进行参数化;对大气向下长波辐射以大气等效辐射率及气温进行参数化;在云天条件下,基于晴阴比的云量参数化和基于气候资料的云天系数参数化都各有较好的效果.对土壤热通量的参数化方法和拖曳系数的取值问题进行了讨论,更完善的方法还有待于与实验测量工作相结合.     

Dynamics of sea-ice biogeochemistry in the coastal Antarctica during transition from summer to winter

The seasonality of carbon dioxide partial pressure(pCO_2).air-sea CO_2 fluxes and associated environmental parameters were investigated in the Antarctic coastal waters.The in-situ survey was carried out from the austral summer till the onset of winter[January 2012,February 2010 and March 2009) in the Enderby Basin.Rapid decrease in pCO_2 was evident under the sea-ice cover in January,when both water column and sea-ice algal activity resulted in the removal of nutrients and dissolved inorganic carbon(DIC) and increase in pH.The major highlight of this study is the shift in the dominant biogeochemical factors from summer to early winter.Nutrient limitation(low Si/N),sea-ice cover,low photosynthetically active radiation(PAR),deep mixed layer and high upwelling velocity contributed towards higher pCO_2during March(early winter).CO_2 fluxes suggest that the Enderby Basin acts as a strong CO_2 sink during January(-81 mmol m~2 d~(-1)),however it acts as a weak sink of CO_2 with-2.4 and-1.7 mmol m~(-2) d~(-1)during February and March,respectively.The present work,concludes that sea ice plays a dual role towards climate change,by decreasing sea surface PCO_2 in summer and enhancing in early winter.Our observations emphasize the need to address seasonal sea-ice driven CO_2 flux dynamics in assessing Antarctic contributions to the global oceanic CO_2 budget.     

北极地区地面辐射量和云辐射强迫特征

In this paper the characteristics of surface radiative fluxes and cloud-radiative forcing are reviewed with a focus on the Arctic. Three aspects are addressed, including (i) changes in radiation flux over the global surface; (ii) characteristics of surface fluxes in the Arctic; and (iii) characteristics of cloud-radiative forcing in the Arctic. The clouds not only significantly reduce the peak summer radiative heating of the surface but also reduce the wintertime radiative cooling at the surface in　higher latitudes. The downward longwave fluxes dominates the incident radiative fluxes in the Arctic during most of the year. Incoming shortwave fluxes are negligible during late fall, winter and early spring, and even during the midsummer the incoming shortwave fluxes are only slightly greater than the downward longwave fluxes. The total net surface radiative flux is negative for most of the year and only positive during midsummer in the Arctic. The global net cloud-radiative forcing is negative, but the cloud-radiative forcing is positive in the Arctic, showing a warming effect, except for a short period in mid-summer. Positive cloud-radiative forcing in the Arctic is attributed　to the presence of snow and ice with high albedo and the absence of solar radiation during the polar night.     

西太平洋暖池冰期旋回中的类ENSO式演化及其驱动机制

作为全球接受太阳辐射最多、表层海水温度最高的区域,西太平洋暖池区通过厄尔尼诺-南方涛动(El Niño-Southern Oscillation,ENSO)和季风等过程影响着全球气候的变化。越来越多的沉积记录证明,在地质历史时期西太平洋暖池也存在类似于现代ENSO过程的“类ENSO式”变化。而目前类ENSO式变化与冰期—间冰期旋回之间的响应关系和驱动机制及其与东亚季风的关联仍存在争议。本文利用位于暖池核心区的B10岩心浮游有孔虫氧同位素、Mg/Ca(质量分数比)和黏土矿物参数重建了暖池区氧同位素8期以来的古气候记录,并结合已有的热带海表温度记录、中国石笋氧同位素和南大洋地区海表温度记录,研究了西太平洋暖池冰期旋回中类ENSO状态的演化规律及其与东亚季风的关系,并探讨了暖池区类ENSO演化的驱动机制。结果发现:冰期时,西太平洋暖池区温跃层变浅,赤道东、西太平洋温差减小,同时,东亚夏季风减弱,暖池区降水量相对减少,与现代El Niño时期气候态类似;间冰期时,西太平洋暖池区温跃层加深,赤道东、西太平洋温差增大,东亚冬夏季风增强,暖池区降水量相对增加,与现代La Niña时期气候态类似。频谱分析结果表明,西太平洋暖池区海表温度的变化具有偏心率周期(96 ka)。冰消期时,低纬度太阳辐射量的增加,增大了纬向上的SST梯度,并使得次表层海水储存了更多的热量,积累的热量会通过调节次表层环流向暖池区的热传输,最终调控赤道太平洋地区Walker环流强度和ENSO活动的长期变化。而冰期时,南大洋地区降温所引起的东南信风和大洋环流异常可能对类ENSO式起到调控的作用。     

Mineral ballast and particle settling rates in the coastal upwelling system off NW Africa and the South Atlantic

The ocean off NW Africa is the second most important coastal upwelling system with a total annual primary production of 0.33 Gt of carbon per year (Carr in Deep Sea Res II 49:59–80, 2002). Deep ocean organic carbon fluxes measured by sediment traps are also fairly high despite low biogenic opal fluxes. Due to a low supply of dissolved silicate from subsurface waters, the ocean off NW Africa is characterized by predominantly carbonate-secreting primary producers, i.e. coccolithophorids. These algae which are key primary producers since millions of years are found in organic- and chlorophyll-rich zooplankton fecal pellets, which sink rapidly through the water column within a few days. Particle flux studies in the Mauretanian upwelling area (Cape Blanc) confirm the hypothesis of Armstrong et al. (Deep Sea Res II 49:219–236, 2002) who proposed that ballast availability, e.g. of carbonate particles, is essential to predict deep ocean organic carbon fluxes. The role of dust as ballast mineral for organic carbon, however, must be also taken into consideration in the coastal settings off NW Africa. There, high settling rates of larger particles approach 400 m day⁻¹, which may be due to a particular composition of mineral ballast. An assessment of particle settling rates from opal-production systems in the Southern Ocean of the Atlantic Sector, in contrast, provides lower values, consistent with the assumptions of Francois et al. (Global Biogeochem Cycles 16(4):1087, 2002). Satellite chlorophyll distributions, particle distributions and fluxes in the water column off NW Africa as well as modelling studies suggest a significant lateral flux component and export of particles from coastal shelf waters into the open ocean. These transport processes have implications for paleo-reconstructions from sediment cores retrieved at continental margin settings.     

Predicting solar radiation fluxes for solar energy system applications

The mean daily global solar radiation flux is influenced by astronomical, climatological, geographical, geometrical, meteorological, and physical parameters. This paper deals with the study of the effects of influencing parameters on the mean daily global solar radiation flux, and also with the computation of the solar radiation flux at the surface of the earth in locations without solar radiation measurements. The reference–real data were borrowed from the Iranian Meteorological Organization. The analysis of data showed that the mean daily solar radiation flux on a horizontal surface is related to parameters such as: mean daily extraterrestrial solar radiation, average daily ratio of sunshine duration, mean daily relative humidity, mean daily maximum air temperature, mean daily maximum dew point temperature, mean daily atmospheric pressure, and sine of the solar declination angle. Multiple regression and correlation analysis were applied to predict the mean daily global solar radiation flux on a horizontal surface. The models were validated when compared with the reference–measured data of global solar radiation flux. The results showed that the models estimate the global solar radiation flux within a narrow relative error band. The values of mean bias errors and root mean square errors were within acceptable margins. The predicted values of global solar radiation flux by this approach can be used for the design and performance estimation in solar applications. The model can be used in areas where meteorological stations do not exist and information on solar radiation flux cannot be obtained experimentally.     

Comparative energy balance study for arctic tundra, sea surface glaciers and boreal forests

Seasonal change in the energy balance on the arctic tundra is presented. The thermal stability of a dry snow cover is investigated in detail. In addition to high reflection by the snow cover, a significant absorption of solar radiation on the very surface of the snow cover was found responsible for the thermal stability. The efficient absorption of solar radiation by the surface rather than the interior of the snow cover and the almost immediate removal of the absorbed energy through radiative emission and turbulent heat fluxes keep the temperature of the snow cover low.The energy balances for the melt and postmelt period for various arctic surfaces are compared. The most important difference of the energy balance between the tundra and tther low attitude arctic surface, such as the sea and ablation areas of glaciers, is not the net radiation but the latent heat of fusion. Extremely small heat cosuumption through the melt on the tundra is the basis for higher temperature, characteristics to the tundra climate in the Arctic.     

Comparative energy balance study for arctic tundra,sea surface glaciers and boreal forests

Seasonal change in the energy balance on the arctic tundra is presented. The thermal stability of a dry snow cover is investigated in detail. In addition to high reflection by the snow cover, a significant absorption of solar radiation on the very surface of the snow cover was found responsible for the thermal stability. The efficient absorption of solar radiation by the surface rather than the interior of the snow cover and the almost immediate removal of the absorbed energy through radiative emission and turbulent heat fluxes keep the temperature of the snow cover low. The energy balances for the melt and postmelt period for various arctic surfaces are compared. The most important difference of the energy balance between the tundra and tther low attitude arctic surface, such as the sea and ablation areas of glaciers, is not the net radiation but the latent heat of fusion. Extremely small heat cosuumption through the melt on the tundra is the basis for higher temperature, characteristics to the tundra climate in the Arctic.     

基于热力学过程的渤海海冰生消模型

为了对渤海海冰生消问题进行模拟,基于三维自由水面垂向分层动网格的Euler-Lagrangian模式,采用VC（Vertex-Centered）方式的非结构化有限体积方法离散三维浅水方程组,模拟渤海的水流运动过程。以此水动力场为背景,引入热力学过程的影响,对渤海海域的冬季结冰过程进行模拟,建立了海冰生消模型。其中热力学参数主要包括大气温度、相对湿度、风场特征、太阳辐射、感热通量系数以及潜热通量系数。以渤海2011/2012年常冰年的结冰过程为例,将各个热力学参数对冰情影响的敏感性进行分析,对模型进行了验证。结果表明,感热与潜热系数是对冰情影响最敏感的一项,即当感热和潜热通量系数仅减小了0.000 2后,其海冰的最大厚度就减小了15 cm。最后,通过连续实测的水动力数据与2009/2010年冬季的典型海冰灾害过程再一次对模型进行了验证,充分说明了模型具有较高的精确性、稳定性与实用性。     

A reevaluation of the oceanic uranium budget for the Holocene

We present a new assessment of the pre-anthropogenic U budget for the Holocene ocean. We find that the gross input of U to the ocean lies in the range 53±17 Mmol/year, where the dominant source is river runoff (42.0±14.5 Mmol/year) and the direct discharge of groundwater could represent a significant additional input (9.3±8.7 Mmol/year). The soluble U flux associated with the aeolian input of crustal dust is minor (1.8±1.1 Mmol/year), falling well within the errors associated with the riverine flux. Removal of U to the organic rich sediments of salt marshes and mangrove swamps during river–sea mixing may significantly modify the riverine flux, such that the net U input is reduced to 42±18 Mmol/year. Evaluation of the U isotope budget demonstrates that the limits we have established on the U input flux are reasonable and suggests that direct groundwater discharge may play a significant role in maintaining the oceanic excess of ²³⁴U. The total sink of U from the ocean lies in the range 48±14 Mmol/year. We find that three major processes control the magnitude of this flux: (1) removal to oxygen-depleted sediments (26.9±12.2 Mmol/year); (2) incorporation into biogenic carbonate (13.3±5.6 Mmol/year); and (3) crustal sequestration during hydrothermal alteration and seafloor weathering (5.7±3.3 Mmol/year). The removal of U to opaline silica (0.6±0.3 Mmol/year) and hydrogenous phases (1.4±0.8 Mmol/year) is minimal, falling well within the errors associated with the other sinks. That the input and output fluxes balance within the calculated errors implies that U may be in steady state in the Holocene ocean. In this case, the input and output fluxes lie in the range 34–60 Mmol/year, giving an oceanic U residence time of 3.2–5.6×10⁵ years. However, given the large uncertainties, a significant imbalance between the Holocene input and output fluxes cannot be ruled out. The constancy of the ancient seawater U concentration implies that the U budget is in steady state over the time period of a glacial–interglacial climate cycle (10⁵ year). A Holocene flux imbalance must, therefore, be offset by an opposing flux imbalance during glacial periods or at the interglacial–glacial transition. We suggest that the storage of U in the coastal zone and shallow water carbonates during interglacial periods and the release of that U at or following the interglacial–glacial transition could be sufficient to affect the short-term stability of the U budget. Providing tighter constraints on U fluxes in the Holocene ocean is a prerequisite to understanding the U budget on the time scale of a glacial–interglacial climate cycle and using this element as a valuable palaeoceanographic proxy.     

河流活性物质入海通量:初步成果

河流是陆地与海洋相互作用的重要纽带,查明陆地河流活性物质入海通量是当前生态地球化学评价的一项重要任务。文中选择了中国东部入海河流中主要的35条河流,分丰、枯水期系统采集了悬浮物、过滤水、底泥等样品,利用河流径流量参数,计算得到了各河流主要重金属及营养元素的年入海通量及陆地河流年入海总通量,确定了各元素水溶态及悬浮物态迁移入海量的比例,为陆海相互作用研究、浅海生态地球化学评价提供了重要依据。