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991.
超强台风"桑美"在浙江省温州市苍南县登陆,登陆时中心附近最大风力达17级,中心气压920hPa,是近50年来登陆我国大陆最强的台风。为了认识超强台风"桑美"强度突然增强的机制机理,气象工作者做了许多有意义的工作,如"桑美"的观测分析、数值模拟、强度突增原因探究等。文章对以往研究成果进行了简述,指出了目前在此方面研究存在的问题,如数值模拟台风强度突增的量值偏小,强度突增的机理没有新的明显突破,以及气候变暖对台风强度突增如何影响涉及较少等。 相似文献
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Xidan Feng Zhi Dang Weilin Huang Longyi Shao Weijun Li 《Journal of Atmospheric Chemistry》2009,64(1):37-51
Samples of airborne PM2.5 particles in Guangzhou urban area were collected during the autumn of 2006 and the spring of 2007. The morphologies and elemental
compositions of individual particles were determined by Scanning Electron Microscopy coupled with Energy Dispersive X-ray
Spectrometer (SEM-EDX). The obtained images were further analyzed for size distribution by an image analysis system. Based
on the morphology, particles in PM2.5 were classified into four groups: soot aggregates, minerals, fly ash and others. The amount of soot aggregates and minerals
were higher than that of fly ashes. The distributions of particles by number and size in two seasons were bimodal with 90%
less than 1.0 μm in diameter. The primary peak from the autumn samples was in the size range of 0.4 ~ 0.5 μm, and 0.3 ~ 0.4 μm
for the spring samples. More soot aggregates (36.1%) and minerals (61.5%) were found than fly ash (2.4%) in autumn, but soot
aggregates (89.9%) was the dominant particle type in spring. The size distribution of particles according to the volume was
generally opposite to that according to the number. Particles less than 1.0 μm were as high as 89.5% in number but contributed
only 18.9% in volume, indicating that fine particles contributed relatively little in volume although existing in large numbers. 相似文献
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针对中国科学院上海技术物理研究所研制的1500元红外线列焦平面探测器的输出特性,提出了以低噪声运放为核心的信息获取电路和以FPGA(Field Programmable Gate Array)为核心的数据预处理的设计方案,实现了驱动电路和探测器的良好匹配,较好地发挥了探测器高灵敏度的特性.测试结果表明,该方案不仅对系统获得优于50 mK噪声等效温差的高灵敏度成像起到了重要作用,足够宽的量化设计还保证了系统的动态范围和图像的丰富层次.该设计方案已成功应用在一些其他类型的红外焦平面探测器中. 相似文献
999.
De-Fu Bu Feng Yuan Fu-Guo Xie 《Monthly notices of the Royal Astronomical Society》2009,392(1):325-331
Observations and numerical magnetohydrodynamic (MHD) simulations indicate the existence of outflows and ordered large-scale magnetic fields in the inner region of hot accretion flows. In this paper, we present the self-similar solutions for advection-dominated accretion flows (ADAFs) with outflows and ordered magnetic fields. Stimulated by numerical simulations, we assume that the magnetic field has a strong toroidal component and a vertical component in addition to a stochastic component. We obtain the self-similar solutions to the equations describing the magnetized ADAFs, taking into account the dynamical effects of the outflow. We compare the results with the canonical ADAFs and find that the dynamical properties of ADAFs such as radial velocity, angular velocity and temperature can be significantly changed in the presence of ordered magnetic fields and outflows. The stronger the magnetic field is, the lower the temperature of the accretion flow will be and the faster the flow rotates. The relevance to observations is briefly discussed. 相似文献
1000.
Lei Chen Shengmiao Wu Feng Yuan 《Monthly notices of the Royal Astronomical Society》2009,398(4):1900-1904
We consider a thin accretion disc warped due to the Bardeen–Petterson effect, presenting both analytical and numerical solutions for the situation in which the two viscosity coefficients vary with radius as a power law, with the two power-law indices not necessarily equal. The analytical solutions are compared with numerical ones, showing that our new analytical solution is more accurate than the previous one, which overestimated the inclination change in the outer disc. Our new analytical solution is appropriate for moderately warped discs, while for extremely misaligned discs only a numerical solution is appropriate. 相似文献