Long-term Field Observations on Seasonality in Chlorophyll-<Emphasis Type="Italic">a</Emphasis> Concentrations in a Shallow Coastal Marine Ecosystem,the Wadden Sea     

Catharina Johanna Maria Philippart  Jolanda Martine van Iperen  Gerhard Cornelis Cadée  Alain François Zuur 《Estuaries and Coasts》2010,33(2):286-294

Analyses of long-term field observations (1974–2007) on chlorophyll-a concentrations in the western Wadden Sea showed no long-term trends in the timing of the wax and wane of phytoplankton spring blooms. There is weak evidence, however, that the height of the autumn bloom has decreased since the early 1990s. This fading of the autumn bloom may have had consequences for the carbon transfer to higher trophic levels, currently hampering primary consumer species that mostly rely on food supply during late summer. Current and other findings suggest a shortening of the growing season due to the fading of the autumn bloom in the Wadden Sea and a lengthening of the growing season due to an advancement of the spring bloom in the North Sea. These regionally different changes in seasonality may have contributed to the coinciding decrease in bivalve filtering capacity in the western Wadden Sea and the large-scale offshore shift of juvenile plaice from the Wadden Sea to the adjacent North Sea.  相似文献   

A pore-throat model based on grain-size distribution to quantify gravity-dominated DNAPL instabilities in a water-saturated homogeneous porous medium     

Khalifa Nsir  Gerhard Schfer 《Comptes Rendus Geoscience》2010,342(12):881-891

A pore-scale network model based on spherical pore bodies and cylindrical pore throats was developed to describe the displacement of water by DNAPL. The pore body size and the pore throat size were given by statistical distributions with user-specified values for the minimum, mean and maximum sizes. The numerical model was applied to a laboratory experiment conducted on a sand-filled glass column. The parameters relative to pore body size and pore throat size that were used in the construction of the equivalent network were derived from the discrete grain-size distribution of the real porous medium. The calculated arrival times of the DNAPL front were compared with those measured using optic fibre sensors placed at different points on the control section of the experimental device. Furthermore, the model simulated DNAPL pressure measured at the entrance section of the system. In general, the numerical results obtained with the model were in good agreement with the actual measurements.  相似文献   

贵州省空气污染过程的大气环流特征及分型研究     

李浪  白慧  方荻  宋丹 《中低纬山地气象》2021,45(5):34-41

该文通过分析2015—2017年贵州省9次空气污染过程的平均大气环流特征及500 hPa大气环流EOF分型结果,综合探讨了贵州省发生空气污染过程时的高空环流、低空水平输送、垂直结构和逆温等特征以及热力和动力因子的贡献情况。结果表明,贵州省发生空气污染过程时,常伴有低空逆温出现,500 hPa高度距平场分型结果主要呈纬向环流型和两槽一脊型环流形势。对EOF第1模态中持续时间较长、污染较重的2次典型污染过程的低空逆温、风切变和垂直速度等进行深入分析发现,2次典型空气污染过程中,在水平方向上地面风场处于风速辐合区,大气层结较稳定,不利于污染物的水平扩散;在垂直方向上低层风垂直切变较弱,对流上升运动也较弱,不利于污染物的垂直扩散。从热力条件和动力条件上来看,在第1次空气污染过程中动力条件的正贡献占主导作用,而第2次空气污染过程中热力条件和动力条件均是正贡献。  相似文献   

尘埃消光对伽玛射线暴余辉的影响     

吕谷靖  邵琅  金志平  韦大明 《天文学报》2011,52(3):190-198

为了研究尘埃消光对伽玛射线暴余辉的影响,基于严格的Mie理论和最新的星际尘埃光学性质,进行了高精度的数值计算,并分析具有不同物理参数的尘埃所产生的消光曲线.结果表明,介质密度和金属丰度是决定消光总量的主要物理参数,而尘埃颗粒大小的分布则是产生不同消光曲线轮廓的重要物理参数.如果尘埃颗粒相互聚集形成导致尺度增大,将产生较平或者较灰的消光曲线,同时绝对总量将减少;相反,如果尘埃颗粒由于某种原因发生离解导致尺度变小,将产生较陡的消光曲线,同时消光总量将增加.这些结果将对理解光学暗暴的形成机制提供重要的启示.  相似文献   

Effect of Dust Extinction on Gamma-ray Burst Afterglows     

Gu-Jing L?  Lang Shao  Zhi-Ping Jin  Da-Ming Wei 《Chinese Astronomy and Astrophysics》2011,35(4):372

In order to study the effect of dust extinction on the afterglow of gamma-ray bursts (GRBs), we carry out numerical calculations with high precision based on the rigorous Mie theory and the latest optical properties of interstellar dust grains, and analyze the different extinction curves produced by dust grains with different physical parameters. Our results indicate that the absolute extinction quantity is substantially determined by the medium density and metallicity. However, the shape of the extinction curve is mainly determined by the size distribution of the dust grains. If the dust grains aggregate to form larger ones, they will cause a flatter or grayer extinction curve with lower extinction quantity. On the contrary, if the dust grains are disassociated to smaller ones due to some uncertain processes, they will cause a steeper extinction curve with larger amount of extinction. These results might provide an important insight into understanding the origin of the optically dark GRBs.  相似文献   

陕西省气象科学共享数据集的制作及处理          下载免费PDF全文

王小宁  阴秀菊  汤浪 《陕西气象》2009,(4):34-36

陕西省气象科学数据共享系统是中国气象科学数据共享服务网的区域级和省级物理节点之一,按照中国气象局“气象资料共享管理办法”要求和数据共享策略,通过网络在线和离线方式对社会开展数据共享服务。  相似文献   

3种再分析资料基本统计量比较   总被引：2，自引：0，他引：2  

何浪  吴洪宝  赵晓川 《南京气象学院学报》2009,32(1):54-63

为了评估中国气象部门整理的资料的特色和应用价值,使用统计方法检验了中国资料和NCEP/NCAR、ECMWF再分析资料7月100 hPa、500 hPa位势高度场和1月海平面气压场的气候均值和年际方差的差异显著性,并比较了1月和7月北半球主要大气活动中心面积、强度指数的年际变化差异和相关程度。结果表明：1）ECMWF再分析资料7月100 hPa、500 hPa位势高度场的气候均值都显著小于中国资料,且其历年值分别小于1 660、588 dagpm,与中国资料相比不适合用于研究南亚高压、副热带高压;2）中国资料是由单层等压面图上直接读数得到的,更接近实际观测值,更适宜于诊断单个等压面上的气压系统;3）3种资料冬季蒙古高压、阿留申低压的年际变化一致性要好于夏季南亚高压、副热带高压。  相似文献   

Trace element partitioning between orthopyroxene and anhydrous silicate melt on the lherzolite solidus from 1.1 to 3.2 GPa and 1,230 to 1,535°C in the model system Na<Subscript>2</Subscript>O–CaO–MgO–Al<Subscript>2</Subscript>O<Subscript>3</Subscript>–SiO<Subscript>2</Subscript>     

Dirk Frei  Axel Liebscher  Gerhard Franz  Bernd Wunder  Stephan Klemme  Jon Blundy 《Contributions to Mineralogy and Petrology》2009,157(4):473-490

We determined experimentally the Nernst distribution coefficient between orthopyroxene and anhydrous silicate melt for trace elements i in the system Na₂O–CaO–MgO–Al₂O₃–SiO₂ (NCMAS) along the dry model lherzolite solidus from 1.1 GPa/1,230°C up to 3.2 GPa/1,535°C in a piston cylinder apparatus. Major and trace element composition of melt and orthopyroxene were determined with a combination of electron microprobe and ion probe analyses. We provide partitioning data for trace elements Li, Be, B, K, Sc, Ti, V, Cr, Co, Ni, Rb, Sr, Y, Zr, Nb, Cs, Ba, La, Ce, Sm, Nd, Yb, Lu, Hf, Ta, Pb, U, and Th. The melts were chosen to be boninitic at 1.1 and 2.0 GPa, picritic at 2.3 GPa and komatiitic at 2.7 and 3.2 GPa. Orthopyroxene is Tschermakitic with 8 mol% Mg-Tschermaks MgAl[AlSiO₆] at 1.1 GPa while at higher pressure it has 18–20 mol%. The rare earth elements show a continuous, significant increase in compatibility with decreasing ionic radius from D _La^opx−melt ∼ 0.0008 to D _Lu^opx−melt ∼ 0.15. For the high-field-strength elements compatibility increases from D _Th^opx−melt ∼ 0.001 through D _Nb^opx−melt ∼ 0.0015, D _U^opx−melt ∼ 0.002, D _Ta^opx−melt ∼ 0.005, D _Zr^opx−melt ∼ 0.02 and D _Hf^opx−melt ∼ 0.04 to D _Ti^opx−melt ∼ 0.14. From mathematical and graphical fits we determined best-fit values for D ₀^M1, D ₀^M2, r ₀^M1, r ₀^M2, E ₀^M1, and E ₀^M2 for the two different M sites in orthopyroxene according to the lattice strain model and calculated the intracrystalline distribution between M1 and M2. Our data indicate extreme intracrystalline fractionation for most elements in orthopyroxene; for the divalent cations D _i ^M2−M1 varies by three orders of magnitude between D _Co^M2−M1 = 0.00098–0.00919 and D _Ba^M2−M1 = 2.3–28. Trivalent cations Al and Cr almost exclusively substitute on M1 while the other trivalent cations substitute on M2; D _La^M2−M1 reaches extreme values between 6.5 × 10⁷ and 1.4 × 10¹⁶. Tetravalent cations Ti, Hf, and Zr almost exclusively substitute on M1 while U and Th exclusively substitute on M2. Our new comprehensive data set can be used for polybaric-polythermal melting models along the Earth’s mantle solidus. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献   

List of major natural disasters, 1960–1987     

Berz  Gerhard 《Natural Hazards》1988,1(1):97-99

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HIDEEP – an extragalactic blind survey for very low column-density neutral hydrogen     

R. F. Minchin  M. J. Disney  P. J. Boyce  W. J. G. de Blok  Q. A. Parker  G. D. Banks †  K. C. Freeman  D. A. Garcia  B. K. Gibson  M. Grossi  R. F. Haynes  P. M. Knezek  R. H. Lang  D. F. Malin  R. M. Price  I. M. Stewart  A. E. Wright 《Monthly notices of the Royal Astronomical Society》2003,346(3):787-802

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