Assessment of wind-forcing impact on a global wind-wave model using the TOPEX altimeter     

Hui Feng  Doug Vandemark  Yves Quilfen  Bertrand Chapron  Brian Beckley 《Ocean Engineering》2006,33(11-12):1431-1461

The study presents assessment of an operational wave model (Wavewatch III), focusing upon the model sensitivity to wind-forcing products. Four wind fields are used to drive the model, including the NCEP/NCAR reanalysis and three other products that assimilate various satellite wind measurements having high spatial resolution, including the QuikSCAT scatterometer. Three wave field statistics: significant wave height, mean zero-crossing wave period, and mean square slope are compared with collocated TOPEX altimeter derivatives to gauge the relative skill of differing wind-forced model runs, as well as to demonstrate an extended use of the altimeter beyond simply supplying wave height for wave model validation and assimilation. Results suggest that model output is critically sensitive to choice of the wind field product. Higher spatial resolution in the wind fields does lead to improved agreement for the higher-order wave statistics.  相似文献   

Atmospheric forcing, larval drift, and recruitment of capelin (Mallotus villosus)     

Dalley  Edgar L.; Anderson  John T.; deYoung  Brad 《ICES Journal of Marine Science》2002,59(5):929-941

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热带三大洋海表温度和云水关系的初探     

刘秦玉  秦婷 《中国海洋大学学报(自然科学版)》2007,37(3):345-350

热带太平洋、大西洋和热带印度洋是全球海洋-大气相互作用最显著的海域。为了探讨热带三大洋局地海洋-大气相互作用中的某些特征,利用新的卫星遥感资料对热带三大洋的云水和海表温度(SST)异常变化进行了统计相关分析。研究发现:在赤道太平洋和赤道大西洋云水和SST二者在超前或滞后5周内都呈现明显的正相关关系,表明3个赤道海域云水和SST之间具有明显的相互作用正反馈机制;在热带西印度洋SST异常超前CLW异常一周时,正相关系数最大,SST的变化导致云水的变化;而在以较冷海水为下垫面的赤道外东北太平洋,东南太平洋以及赤道外的南大西洋海域,二者呈明显的负相关关系,云水的变化会引起SST的变化。位于菲律宾以东的热带西北太平洋区,云水量的变化引起SST的变化;而赤道东印度洋暖池区即存在云水量的增加(减少)引起SST降低(升高)的现象,也存在SST降低(升高)引起云水量的减少(增加)的现象。以上结果将为进一步理解海洋-大气相互作用,在数值模式中正确设计海洋-大气边界层参数化方案提供参考。  相似文献   

Sea surface temperature observation by Global Imager (GLI)/ADEOS-II: Algorithm and accuracy of the product   总被引：1，自引：0，他引：1  

Futoki Sakaida  Kohtaro Hosoda  Masao Moriyama  Hiroshi Murakami  Akira Mukaida  Hiroshi Kawamura 《Journal of Oceanography》2006,62(3):311-319

A sea surface temperature (SST) retrieval algorithm for Global Imager (GLI) aboard the ADEOS-II satellite has been developed. The algorithm is used to produce the standard SST product in the Japan Aerospace Exploration Agency (JAXA). The algorithm for cloud screening is formed by combinations of various types of tests to detect cloud-contaminated pixels. The combination is changed according to the solar zenith angle, which enables us to detect clouds even in the sun glitter region in daytime. The parameters in the cloud-detection tests have been tuned using the GLI global observations. SST is calculated by the Multi-Channel SST (MCSST) technique from the detected clear pixels. Using drifting buoy measurements, match-up data are produced to derive the coefficients of the MCSST equations and to examine their performance. The bias and RMSE of the GLI SST are 0.03 K and 0.66 K for daytime and, −0.01 K and 0.70 K for nighttime, respectively.  相似文献   

快速移动的0510号热带风暴"珊瑚"路径及对深圳降水影响的分析     

曹春燕  江崟 《台湾海峡》2006,25(4):559-565

从天气形势、雷达回波和卫星云图特征对2005年第10号热带风暴“珊瑚”的移动路径和对深圳降水的影响进行了详细的分析．结果表明：副热带高压的演变，对热带气旋的移动路径尤其是路径的转向影响很大，副高的增强、减弱是热带气旋发生转向的重要条件；螺旋云带的变化通常能表明热带气旋未来的移动及其强度变化，眉状云带是热带气旋北上的重要特征云系；“珊瑚”在登陆前后西侧云系迅速减弱，以及登陆后加速北上，深圳没有转吹南风，是导致深圳没有出现暴雨的主要原因．  相似文献   

WEST: A northern California study of the role of wind-driven transport in the productivity of coastal plankton communities   总被引：1，自引：0，他引：1  

J.L. Largier  C.A. Lawrence  M. Roughan  D.M. Kaplan  E.P. Dever  C.E. Dorman  R.M. Kudela  S.M. Bollens  F.P. Wilkerson  R.C. Dugdale  L.W. Botsford  N. Garfield  B. Kuebel Cervantes  D. Kora in 《Deep Sea Research Part II: Topical Studies in Oceanography》2006,53(25-26):2833

The “Wind Events and Shelf Transport” (WEST) program was an interdisciplinary study of coastal upwelling off northern California in 2000–03. WEST was comprised of modeling and field observations. The primary goal of WEST was to better describe and understand the competing influences of wind forcing on planktonic productivity in coastal waters. While increased upwelling-favorable winds lead to increased nutrient supply, they also result in reduced light exposure due to deeper surface mixed layers and increased advective loss of plankton from coastal waters. The key to understanding high levels of productivity, amidst these competing responses to wind forcing, is the temporal and spatial structure of upwelling. Temporal fluctuations and spatial patterns allow strong upwelling that favors nutrient delivery to be juxtaposed with less energetic conditions that favor stratification and plankton blooms. Observations of winds, ocean circulation, nutrients, phytoplankton and zooplankton off Bodega Bay and Point Reyes (38°N) were combined with model studies of winds, circulation and productivity. This overview of the WEST program provides an introduction to the WEST special issue of Deep-Sea Research, including the motivation for WEST, a summary of study components, an integrative synthesis of major research results to-date, and background on conditions during field studies in May–June 2001 (the upwelling period on which this special issue is focused).  相似文献   

Periodicity in the crater formation rate and implications for astronomical modeling     

S. Yabushita 《Celestial Mechanics and Dynamical Astronomy》1992,54(1-3):161-178

Claim for periodicity in the crater formation rate is reinvestigated using a criterion proposed by Broadbent, and data sets of Rampino and Stothers and of Grieve are shown to satisfy the periodicity criterion (P 30 Myr).On the other hand, currently observed impactors are mainly asteroids, while long and short periodic comets whose fluxes may vary by external disturbances occupy only a small fraction. Using a Monte Carlo simulation, constraints are obtained for the dispersion Q(Myr) from an exact periodicity and for the periodic components (F _tp) in the signals for their periodicity to be detected. It is found that for = 5, 6 and 7 Myr, F _tp, would have to be 40% or greater, 60% or greater and 80% or greater, respectively. These constraints are used to discuss whether the giant molecular cloud perturbations can give rise to the periodicity in the impact events. The amplitude of the solar Z-motion need to be some 100pc for = 6 Myr, which requires the periodic component (SP and LP comets, if the former originate from the latter) to be 60%, while for = 7 Myr, the periodic component need to be 80%. The GMC perturbation model consistent with the periodicity appears to be the one where the amplitude is 100pc and the periodic component - 60% of the impactors. If SP comets mainly originate from a source such as the hypothetical Kuiper belt, the GMC perturbation would not be consistent with the periodicity.  相似文献   

Near-parabolic cometary flux in the outer solar system     

T. Tsujii 《Celestial Mechanics and Dynamical Astronomy》1992,54(1-3):271-274

The flux of near-parabolic comets in the outer-planetary region is estimated on the presumption that the major planets and the galactic tide control the dynamics of comets. It is found that the flux of the Oort cloud comets (semi-major axis > 20000 AU) is similar to the case of a strong comet shower derived on the presumption that the galactic tidal force were not operative. On the other hand, the flux of comets with semi-major axes <- 20000 AU is found to be an increasing function of q (perihelion distance) until q reaches 20 AU, while for a 45000 AU it is a rapidly increasing function for q 12 AU. In other words, for comets of the inner extension of the Oort cloud the planetary perturbation acts as a strong barrier for them to penetrate into the inner planetary region.  相似文献   

A model of the galactic tidal interaction with the oort comet cloud     

John J. Matese  Patrick G. Whitman 《Celestial Mechanics and Dynamical Astronomy》1992,54(1-3):13-35

We consider a model of the in situ Oort cloud which is isotropic with a random distrihution of perihelia directions and angular momenta. The energy distribution adopted has a continuous range of values appropriate for long-period (>200 yr) comets. Only the tidal torque of the Galaxy is included as a perturbation of comet orbits and it is approximated to be that due to a quasi-steady state distribution of matter with disk-like symmetry. The time evolution of all orbital elements can be analytically obtained for this case. In particular, the change in the perihelion distance per orbit and its dependence on other orbital elements is readily found. We further make the assumption that a comet whose perihelion distance was beyond 15 AU during its last passage through the Solar System would have orbit parameters that are essentially unchanged by planetary perturbations. Conversely, if the prior passage was inside 15 AU we assume that planetary perturbations would have removed the comet from the in situ energy distribution accessible by the galactic tide. Comets which had their perihelia changed from beyond 15 AU to within 5 AU in a single orbit are taken to be observable. We are able to track the evolution of 10⁶ comets as they are made observable by the galactic tidal touque. Detailed results are obtained for the predicted distribution of new (0 < 1/ < 10^–4 AU^–1) comets. Further, correlations between orbital elements can be studied. We present predictions of observed distributions and compare them with the random in situ results as well as with the actual observed distributions of class I comets. The predictions are in reasonable agreement with actual observations and, in many cases, are significantly different from random when perihelia directions are separated into galactic northern and southern hemispheres. However the well-known asymmetry in the north-south populations of perihelia remains to be explained. Such an asymmetry is consistent with the dominance of tidal torques today if a major stochastic event produced it in the past since tidal torques are unable to cause the migration of perihelia across the latitude barriers ±26°.6 in the disk model.  相似文献   

国土资源大数据上云高效运行体系及关键技术研究——以山东省为例          下载免费PDF全文

安国强  仲阳  吴建廷  孔维剑  秦晓敏  许霄霄  陈龙飞 《山东国土资源》2020,36(7):74-80

基于山东省国土资源大数据上云系统建设和应用实践,在仿真实验的基础上,研究提高山东省国土资源大数据上云效率的运行体系和关键技术,为全省政务云建设提供参考。研究结果表明,通过高效运行体系构建和关键技术的应用,山东省国土资源上云系统快速显示、裁切、瓦片、数据挖掘等效率都得到不同程度的提高,其中上云系统并发性能耗时平均提速99.5%以上,矢量数据裁图效率同比提升17倍。研究结论:从功能设计、数据组织、硬件环境和拓扑结构四个方面统筹设计国土资源大数据上云系统高效运行体系,从数据处理、异构数据集成、分布式数据存储及挖掘、海量图库管理、灵活的搭建式开发等关键技术创新,可以大幅提高国土资源大数据上云运行效率。  相似文献