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101.
本文选取2012年4月27-28日影响北京的一次沙尘天气过程进行分析,发现在本次过程中,沙源地区的沙尘暴主要发生在地面冷锋和500 hPa槽后,在近地层强烈的感热加热与中低层冷平流的共同作用下,形成了不稳定层结及深厚的混合层,最高可达600 hPa,是沙尘天气能够影响下游地区的重要条件。本文还通过分析等熵混合层厚度变化及其平流过程来追踪沙尘天气的输送路径和定位沉降地,发现本次过程有两种传输路径,一种是沿辽宁北部向东而后转向东北方向,主要沿等熵混合层平流向下游移动,之后随着等熵混合层的接地沉降到近地层,该路径影响高度较高;另一种是沿辽宁南部向东南方向移动,混合层平流较清楚,但沉降时与东北路径明显不同,在辽东半岛东部地面辐散气流及下沉运动的作用下发生沉降,并随冷锋后冷高压南侧的东风回流向西输送影响北京地区。另外,由于混合层之上的稳定层明显下压,使沙尘输送高度偏低。运用HYSPLIT模式模拟的前、后向轨迹证实了上述两种输送路径,表明北京的扬沙天气是由东风回流造成的。 相似文献
102.
雷达回波外推预报的误差分析 总被引:4,自引:0,他引:4
基于天气雷达资料的外推预报是灾害天气临近预报的基础,选取4次强降水过程分析了外推预报的误差.主要分析方法包括3个步骤:(1)采用多尺度回波跟踪方法确定雷达回波的运动场;(2)采用半拉格朗日平流方案对雷达回波进行外推;(3)预报结果和观测结果进行对比.利用去相关时间方法分析了雷达回波的可预报性,利用预报技巧评分和相对绝对误差对外推预报的误差进行了定量分析.此外,还分析了外推预报的误差与尺度之间的关系,以及外推预报中的不确定因素 回波强度变化和回波运动场变化在预报误差中的相对重要性.这4次强降水过程的误差分析表明,预报误差随预报时效的变化基本上是以指数规律递减的,大尺度的降水系统对应较长的持续性,对于发展演变较快、尺度较小的风暴,其持续性较短. 相似文献
103.
利用常规气象观测资料和Micaps提供的相关资料,对2009年9月19—20日在河套地区发生的寒潮天气的环流形势及物理量进行分析。分析表明:在寒潮爆发前期,500hPa系统,蒙古西部的冷中心强度≥-32℃,且温度场滞后于高度场,为冷空气爆发南下提供了最基本条件;700hPa河套地区及上游≥16m.s-1的西北风急流基本形成,等温线与等高线交角≥45°且10个纬距内有4条及以上等温线的密集区;850hPa河套地区有≥16℃的暖中心,高空槽前后的西北风速≥18 m.s-1,温度线与高度线的夹角>45°;地面蒙古气旋的暖性性质为寒潮爆发的前期提供了有利的热力条件,地面冷锋后部冷高压轴线接近南北向,且冷高压中心强度≥1040hPa,3h变压≥3hPa。 相似文献
104.
赤道东北太平洋表层沉积物间隙水中营养盐的剖面分布及其海底扩散通量 总被引:3,自引:0,他引:3
对赤道东北太平洋海域表层沉积物间隙水中硅酸盐、磷酸盐和硝酸盐等营养盐的剖面分布三个航次的研究表明,研究区在采样深度内沉积物中有机质的分解以硝化作用为主.在水-沉积物界面附近硅酸盐、磷酸盐和硝酸盐都存在着极陡的浓度梯度, Fick扩散定理的计算结果表明,研究区内硅酸盐、磷酸盐和硝酸盐的海底扩散通量分别为- 886.45~ 42.62 μ mol/(m2· d)、- 3.04~ 5.83 μ mol/(m2· d)和- 189.43~ 21.05 μ mol/(m2· d),且硅酸盐和硝酸盐主要是从沉积物向底层水体扩散,是底层水体营养盐的来源之一;研究区内硅酸盐、磷酸盐和硝酸盐的海底扩散通量存在着一定的时间和空间变化, 这可能与因全球气候变化而导致的沉积环境的改变有关. 相似文献
105.
V. Urpin 《Astronomische Nachrichten》2015,336(3):266-270
The stars of the middle main sequence often have spot‐like chemical structures at their surfaces. We consider the diffusion process caused by electric currents that can lead to the formation of such chemical spots. Diffusion is considered using the partial momentum equations derived by the Chapman‐Enskog method. We argue that diffusion caused by electric currents can substantially change the surface chemistry of stars and form spotted chemical structures even in a relatively weak magnetic field. The considered mechanism can be responsible for a formation of element spots in Hg‐Mn and Ap‐stars. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
106.
Cooling rates based on the retrograde diffusion of Fe2+ and Mg between garnet and biotite inclusions commonly show two contrasting scenarios: a) narrow closure temperature range with apparent absence of retrograde diffusion; or b) high result dispersion due to compositional variations in garnet and biotite. Cooling rates from migmatites, felsic and mafic granulites from Ribeira Fold Belt (SE Brazil) also show these two scenarios. Although the former can be explained by very fast cooling, the latter is often the result of open-system behaviour caused by deformation. Retrogressive cooling during the exhumation of granulite-facies rocks is often processed by thrusting and shearing which may cause plastic deformation, fractures and cracks in the garnet megablasts, allowing chemical diffusion outside the garnet megablast – biotite inclusion system.However, a careful use of garnets and biotites with large Fe/Mg variation and software that reduces result dispersion provides a good correlation between closure temperatures and the size of biotite inclusions which are mostly due to diffusion and compositional readjustment to thermal evolution during retrogression.Results show that felsic and mafic granulites have low cooling rates (1–2 °C/Ma) at higher temperatures and high cooling rates (∼100 °C/Ma) at lower temperatures, suggesting a two-step cooling/exhumation process, whereas migmatites show a small decrease in cooling rates during cooling (from 2.0 to 0.5 °C/Ma). These results agree with previously obtained thermochronological data, which indicates that this method is a valid tool to obtain meaningful petrological cooling rates in complex high-grade orogenic belts, such as the Ribeira Fold Belt. 相似文献
107.
Huaiwei Ni 《中国地球化学学报》2014,33(2):125-130
Oxygen isotope fractionation between coexisting minerals in slowly cooled rocks conveys information about their cooling history. By using the fast grain boundary (FGB) model to simulate closed-system diffusive ex- change of oxygen isotopes between coexisting minerals, I show that the apparent equilibrium temperatures (Tae) by the mineral pair with the largest isotopic fractionation (PLIF) always lies between the closure temperatures (To) of those two minerals. Therefore, when the rate of oxygen diffusion and hence Tc for the PLIF chance to be comparable (such as in the case of quartz and magnetite), Tae will serve as a good approximation of To regardless of variation in mineral proportions. The specialty of the PLIF in constraining Tac within their Tc range can be generalized to other stable isotope systems and element partitioning. By approximating Tc with Tac and inverting Dodson's equation, the cooling rate of plutonic or metamorphic rocks can be inferred. 相似文献
108.
W. K. Hocking 《Earth, Moon, and Planets》2004,95(1-4):671-679
At altitudes above 93 km in the atmosphere, magnetic and electric fields can affect the modes and rates of non-turbulent diffusion
of ionized meteor trails. Anisotropic diffusion is expected. Most theories of anisotropic diffusion, and indeed most experimental
studies, have concentrated on the effects of the magnetic field in producing this anisotropy, and different rates of expansion
are expected in directions parallel to and perpendicular to the magnetic field lines. In this study, we use interferometric
meteor radars to investigate the dependence of the ambipolar diffusion coefficient on viewing direction relative to the magnetic
field, and show that the dependence is at best weak when daily averages are used. We then demonstrate that the reason for
this effect is that the positions of maximum and minimum diffusion rates varies as a function of time of day, and that daily
averaging masks the anisotropy. One possibility to account for the observations is that this strong diurnal variation is a
consequence of the electric fields in the upper atmosphere, which are often tidally driven. An alternative possibility is
a diurnal cycle in mean meteor entrance speeds. We lean towards the first hypothesis, but both possibilities are discussed.
We demonstrate our results with data from several sites, but particularly using the Clovar radar near London, Ontario, Canada. 相似文献
109.
Abstract An analytical electron microscope study of almandine garnet from a metamorphosed Al–Fe‐rich rock revealed detailed composition profiles and defect microstructures of resorption zoning along fluid‐infiltrated veins and even into the garnet/ilmenite (inclusion) interface. This indicates a limited volume diffusion for the cations in substitution (mainly Ca and Fe) and an interface‐controlled partition for the extension of a composition‐invariant margin. A corrugated interface between the Ca‐rich margin/zone and the almandine garnet core is characterized by dislocation arrays and recovery texture further suggesting a resorption process facilitated by diffusion‐induced recrystallization, diffusion‐induced dislocation migration and diffusion–induced grain boundary migration. Integrated microstructural and chemical studies are essential for understanding the underlying mechanisms of processes such as garnet zoning and its modification. Without this understanding, it will not be possible to reliably use garnet compositions for thermobarometry and other applications that rely on garnet chemical information. 相似文献
110.
Claude Froeschlé Massimiliano Guzzo Elena Lega 《Celestial Mechanics and Dynamical Astronomy》2005,92(1-3):243-255
We detect and measure diffusion along resonances in a quasi-integrable symplectic map for different values of the perturbation parameter. As in a previously studied Hamiltonian case (Lega et al., 2003) results agree with the prediction of the Nekhoroshev theorem. Moreover, for values of the perturbation parameter slightly below the critical value of the transition between Nekhoroshev and Chirikov regime we have also found a diffusion of some orbits along macroscopic portions of the phase space. Such a diffusion follows in a spectacular way the peculiar structure of resonant lines. 相似文献