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81.
1991年梅雨期中冷空气活动的个例分析 总被引:4,自引:1,他引:4
通过对1991年7月4—6日江淮地区大暴雨过程中冷空气的轨迹分析表明,来自西北方向的冷空气造成了冷暖空气在长江流域的对峙和高原东侧50hPa槽的发展,后者又进而促使了梅雨锋上的气旋发展。 相似文献
82.
83.
TRAJECTORY DIAGNOSIS OF AIR PARCELS IN HIGH-AND LOW-LEVEL JETS FOR A HEAVY RAINFALL CASE DURING MEIYU SEASON OF 1991 下载免费PDF全文
Trajectory diagnostic methods were used to analyze air parcels of high-and low-level jets during the heavy rainfall of 4-6 July 1991.It is found that air parcels above rainfall area travelled from the entrance of the high-level jet,passing through the jet center and reached the exit region.Upper tropospheric divergence over rainfall area resulted from decelerative motion of the jet flow.Warm and moist southwest flow converged and ascended ahead of the low-level jet.The decreasing of low-level pressure as a result of high-level divergence that caused the low-level jet became unexpectedly strong. 相似文献
84.
Ü. Rannik T. Markkanen J. Raittila P. Hari T. Vesala 《Boundary-Layer Meteorology》2003,109(2):163-189
Observations of wind statistics within and above a Scots pine forest are comparedwith those predicted from an analytical second-order closure model. The roughnesssublayer (RSL) effects, and the influence of stability on similarity functions, arestudied using observations. The commonly accepted forms of similarity functionsdescribe the influence of diabatic effects above the RSL well. According to earlierstudies they are expected also to apply within the RSL. As an exception, the averagewind speed normalised with friction velocity was found to be invariant with stabilityclose to the canopy top under unstable conditions. Lagrangian stochastic trajectorysimulations were used to evaluate the influence of canopy turbulence profiles onfootprint prediction. The main uncertainty was found to arise from parameterisationof the random forcing term in the Lagrangian velocity equation. The influence ofdiabatic conditions was studied, and it was found that thermal stability affectssignificantly the footprint function above the forest canopy, but significantuncertainty exists because of uncertainties in the formulation of stability functions. 相似文献
85.
在使用2.5维混合模拟方法研究了Petschek模型稳态驱动磁场 重联演化的基础上, 本文考察了计算域内各典型区域中粒子分布函数的变化,描绘了重联区不同位置几种类型的 非Maxwell分布函数. 结果表明,磁场重联会将重联区少部分粒子加速到很高的能量,不同 加速程度的粒子将形成球壳状的速度分布. 粒子的轨道特征表明,在重联区中出流的粒子, 有一部分被磁镜捕获,其回旋半径大于重联区宽度,并构成整个流体速度的低速部分. 另外 ,在X中性点附近进入重联区的粒子沿磁力线向出流区以三种形式漂移,分别为:沿磁力线 逃逸、捕获在磁镜中随流体运动、横越磁力线漂移,其比例分别约为70%,20%和10%。 相似文献
86.
Abstract Physical stratigraphy within shoreface‐shelf parasequences contains a detailed, but virtually unstudied, record of shallow‐marine processes over a range of historical and geological timescales. Using high‐quality outcrop data sets, it is possible to reconstruct ancient shoreface‐shelf morphology from clinoform surfaces, and to track the evolving morphology of the ancient shoreface‐shelf. Our results suggest that shoreface‐shelf morphology varied considerably in response to processes that operate over a range of timescales. (1) Individual clinoform surfaces form as a result of enhanced wave scour and/or sediment starvation, which may be driven by minor fluctuations in relative sea level, sediment supply and/or wave climate over short timescales (101?103 years). These external controls cannot be distinguished in vertical facies successions, but may potentially be differentiated by the resulting clinoform geometries. (2) Clinoform geometry and distribution changes systematically within a single parasequence, reflecting the cycle in sea level and/or sediment supply that produced the parasequence (102?105 years). These changes record steepening of the shoreface‐shelf profile during early progradation and maintenance of a relatively uniform profile during late progradation. Modern shorefaces are not representative of this stratigraphic variability. (3) Clinoform geometries vary greatly between different parasequences as a result of variations in parasequence stacking pattern and relict shelf morphology during shoreface progradation (105?108 years). These controls determine the external dimensions of the parasequence. 相似文献
87.
LI Xiang LIN Hui 《地球空间信息科学学报》2006,9(1):65-70
Introduction Withthedramaticdevelopmentofpositioning andtelecommunicationtechnologies,lotsoftraj ectorydataofmovingvehiclescanbecalculated,collected,andtransferred.Inthemeanwhile,thisdevelopmentandtheavailabilityoftrajectory datahavealsomotivatedresearche… 相似文献
88.
LI Xiang LIN Hui 《地球空间信息科学学报》2006,9(2):112-117
IntroductionIf let roadway entities be denoted by arcs and in-tersections be denoted by nodes, then a road net-work can be represented with node-arc model. Be-cause the designation of nodes can be determinedby arcs according to the definition of node-arc mod-el, howto designate arcs becomes the key of repre-senting a road network. As described in the firstpaper of the series, all four kinds of roadway enti-ties (i.e., streets, road segments, carriageways,and lanes) can be represented by arcs. … 相似文献
89.
An approximate analytical solution for the deposition of heavy particles released from an elevated line source 总被引:1,自引:1,他引:1
This work re-examines and further develops an analytical solution for the deposition swath of heavy particles released in
the atmosphere from an elevated source over uniform terrain, correcting the particle diffusivity for the crossing trajectory
effect. The revised (approximate) analytical solution proves to be accurate within 20% over a wide range of micrometeorological
conditions and particle size, despite its neglect of the turbulence component of the deposition flux. It compares very satisfactorily
with experimental data and with the simulations of a Lagrangian stochastic model, provided the variable U(H)/w
g
≤7 (ratio of the mean horizontal wind speed at source height to the particle settling velocity). In this domain of validity,
simple formulae relating the statistics of the deposition swath to U(H)/w
g
are derived. 相似文献
90.
Pavel Spurný 《Earth, Moon, and Planets》1995,68(1-3):529-537
Many Perseid meteors were photographed in the Czech part of the European Fireball Network during the activity of the new strong and sharp maximum on August 12, 1993. Basic data on many of them were evaluated and radiants, atmospheric trajectories and some orbital elements are presented here and compared with atmospheric and orbital data of regular Perseids, which were photographed outside the new activity in 1993 and preceding years. No substantial difference between these two groups of Perseid meteors was found. 相似文献