Analytical studies of the cloud droplet spectral dispersion influence on the first indirect aerosol effect   总被引：1，自引：0，他引：1  

解小宁  刘晓东 《大气科学进展》2013,30(5):1313-1319

  相似文献   

Cross-equatorial structures of equatorially trapped nonlinear Rossby waves     

《Dynamics of Atmospheres and Oceans》2013

Analysis of the Sea Surface Height (SSH) from satellite altimeters has shown that equatorially trapped Rossby waves exhibit asymmetric cross-equatorial structures; their northern extrema are much larger in magnitude than their southern counterparts. Such asymmetry is inconsistent with the classical theory for the first baroclinic, first meridional equatorially trapped Rossby mode, which predicts that SSH and zonal velocity are symmetric in latitude and the meridional velocity is latitudinally antisymmetric (Matsuno, 1966). Chelton et al. (2003) attributed the observed asymmetry to the mean-shear-induced modifications of first meridional mode Rossby waves. The present paper examines nonlinear rectification of cross-equatorial wave structures in the presence of different zonal mean currents. Nonlinear traveling Rossby waves embedded in shears are calculated numerically in a 1.5-layer model. Nonlinearity is shown to increase the cross-equatorial asymmetry substantially making the northern extrema even more pronounced. However, nonlinearity only slightly increases the magnitude of the westward phase speed.  相似文献   

Domestic actions contributing to the mitigation of GHG emissions from power generation in Brazil     

《Climate Policy》2013,13(2-3):247-254

Abstract

Continued growth and the privatisation of Brazil's electricity system, which is largely based upon hydropower, is projected to lead to big expansion mainly of natural gas but also coal power stations with a resulting huge growth in greenhouse gases (GHG) emissions unless steps are taken to avoid this. The Brazilian National Program of Power Conservation and Efficient Use of Electrical Energy in terms of avoided GHG emissions (PROCEL), originally created in 1985, is a multi-stakeholder program coordinated by Eletrobrás aimed to reduce the waste of electrical power on both supply and demand side. Initially crippled by lack of funds, a new finance structure introduced in 1994 has greatly increased PROCEL's impact. Here we develop scenarios that suggest that continued expansion of PROCEL's programme, including resources that might be drawn through clean development mechanism (CDM) projects, to meet projected PROCEL targets over the next two decades could avoid approximately one-third of the GHG emissions from the Brazilian power sector. This contribution demonstrates the significant global environmental benefits of PROCEL in addition to national benefits of this innovative programme.  相似文献   

EC-thin降水预报与极端天气预报指数在浙江暴雨预报中的检验与释用          下载免费PDF全文

傅良  娄小芬  张玉静 《气象与减灾研究》2020,43(4):275-283

利用ECMWF模式降水和极端天气指数资料,以及浙江省68个气象站降水观测资料,评估了ECMWF细网格模式(EC-thin)和降水极端天气指数(EFI)对浙江2018—2020年梅汛期暴雨预报效果。研究表明：对于同一预报时效,随着阈值的增加,EC-thin和降水EFI的暴雨预报评分都呈现“先增加、后减小”的趋势,对于不同预报时效都存在某一阈值使得暴雨预报评分达到最大。从24 h时效到72 h时效,EC-thin的降水预报阈值从45 mm逐渐下降到25 mm,而降水EFI的暴雨预报阈值从07下降到06。EC-thin和降水EFI对暴雨预报的空报率随着阈值的增大而减小,漏报率随着阈值的增大而增大。对于不同预报时效,通过合理组合EC-thin降水阈值和降水EFI阈值,可以得到更好的暴雨预报效果,其评分高于单独使用降水EFI阈值或EC-thin降水阈值得到的评分。  相似文献   

Light-Time Effect in the Eclipsing Binaries GO Cyg, GW Cep, AR Aur and V505 Sgr     

D. Chochol  T. Pribulla  M. Vaňko  P. Mayer  M. Wolf  P. G. Niarchos  K. D. Gazeas  V. N. Manimanis  L. Brát  M. Zejda 《Astrophysics and Space Science》2006,304(1-4):93-96

Orbital period changes of the eclipsing binaries GO Cyg and GW Cep are explained by the light-time effect for the first time. New minima of the eclipsing binary AR Aur improve the predicted light-time orbit. The light-time orbit with the quadratic ephemeris of the binary matches the new observations of V505 Sgr better than the linear one. As the light-time effect fits in corresponding O − C diagrams of all four systems have been reaching extreme values, the observations of minima times in forthcoming years are highly desirable.  相似文献   

Observing Magnetic Fields in Star-Forming Regions     

Jim Cohen 《Astrophysics and Space Science》2005,295(1-2):27-36

Magnetic field strengths and directions can be estimated using many different observational techniques that span a wide range of wavelengths. Each observational method favours different regimes of scale size, density and other physical conditions. The available techniques and their ranges of applicability are briefly described and the current status of observations is reviewed, with particular emphasis on high-resolution observations of star-forming regions.  相似文献   

Delayed plastic model for time‐dependent behaviour of materials     

Tsutomu Namikawa 《国际地质力学数值与分析法杂志》2001,25(6):605-627

A delayed plastic model, based on the theory of plasticity, is proposed to represent the time‐dependent behaviour of materials. It is assumed in this model that the stress can lie outside the yield surface and the conjugate stress called static stress is defined on the yield surface. The stress–strain relation is calculated based on the plastic theory embedding the static stress. Thus, the stress–strain relation of the model practically corresponds to that of the inviscid elastoplastic model under fairly low rate deformation. The delayed plastic model is coupled with the Cam‐clay model for normally consolidated clays. The performance of the model is then examined by comparing the model predictions with reported time‐dependent behaviour of clays under undrained triaxial conditions. It is shown that the model is capable of predicting the effect of strain rate during undrained shear and the undrained creep behaviour including creep rupture. Copyright © 2001 John Wiley & Sons, Ltd.  相似文献   

The iron Kα lines as a tool for magnetic field estimations in non-flat accretion flows     

A.F. Zakharov  Z. Ma  Y. Bao 《New Astronomy》2004,9(8):663-677

Observations of AGNs and microquasars by ASCA, RXTE, Chandra and XMM-Newton indicate the existence of broad X-ray emission lines of ionized heavy elements in their spectra. Such spectral lines were discovered also in X-ray spectra of neutron stars and X-ray afterglows of GRBs. Recently, Zakharov et al. [MNRAS 342 (2003) 1325] described a procedure to estimate an upper limit of the magnetic fields in regions from which X-ray photons are emitted. The authors simulated typical profiles of the iron Kα line in the presence of magnetic field and compared them with observational data in the framework of the widely accepted accretion disk model. Here we further consider typical Zeeman splitting in the framework of a model of non-flat accretion flows, which is a generalization of previous consideration into non-equatorial plane motion of particles emitting X-ray photons. Using perspective facilities of space borne instruments (e.g., Constellation-X mission) a better resolution of the blue peak structure of iron Kα line will allow to evaluate the magnetic fields with higher accuracy.  相似文献   

影响鸢乌贼手钓上钩率的因子探讨     

吴国峰  陈新军 《广东海洋大学学报》2006,26(6):35-38

根据印度洋西北部鸢乌贼(Symplectoteuthis oualaniensis)作业渔场的现场调查数据,分析了作业水深、作业时段、摄食等级和月相等因子对手钓上钩率的影响。统计表明,晚上、午夜和凌晨3个不同时段和不同作业水深对手钓上钩率均有显著性影响。3个时段中,其摄食等级呈先低后高再低的现象。午夜和凌晨,上钩率的变化趋势与摄食等级的变化趋势呈显著的负相关。在月相的影响下,离朔日三四天之前,手钓产量呈上升趋势;离望日五六天之前,手钓产量呈明显的下降趋势。  相似文献   

滕州泉上煤矿碳酸盐岩富水性及对煤层开采的影响          下载免费PDF全文

朱昌元  燕伟  李文东 《山东国土资源》2006,22(5):42-45

通过滕县煤田(南部)泉上煤矿井下实际揭露及钻孔资料,分析研究了十下灰岩、奥灰富水性特征及石炭二叠纪月门沟群对太原组16,17煤层开采的影响,认为在开采16煤层时,必须遵循“深部疏水降压,浅部采煤”的方针;在开采17煤层时,正常情况下不会受到奥灰水的威协;在井巷开拓过程中必须慎重对待十二灰,应先查明十二灰与奥灰的关系,防止奥灰底鼓水危害。  相似文献