南京地区闪电定位资料与探空资料的应用分析

利用江苏省闪电定位系统的观测资料,结合南京探空资料,分析了以南京探空站为中心的1°×1°的经纬度范围内,在两次探空放球时间段内所发生的闪电情况.分析表明,沙氏指数、700 hPa与1000 hPa假相当位温θse差、500 hPa与700 hPa假相当位温θse差、1000 hPa温度、500 hPa温度对南京地区闪电活动的实时预警有比较明显的作用,并定义了闪电概率指数,可用于预报0～30 min内闪电的发生概率.本研究对南京地区雷电实时监测与预警有参考价值.     

一次持续空气污染过程的气象条件分析

2004年12月24-30日,淄博地区出现一次持续一周的强空气污染过程.本文分析了这次过程的主要污染物浓度变化特征和造成强污染的天气形势特点以及主要的气象变量分布特征.结果表明:高空维持稳定纬向环流、逆温层结持续存在、混合层厚度增加、低空风速小,导致污染物不能及时随大气扩散,污染物浓度增大.     

在非匀质波动中应用拉格朗日函数平均法应注意的问题

本文主要讨论了变分原理在解决有关非均质波动中存在的问题,并分析了使用普通变分原理、限制性变分原理、多重尺度法对惯性重力内波方程进行研究的结果,发现使用变分原理,限制性变分原理都是有条件的,即它们仅对某些类型的方程才有效,而对于有些方程用不同的方法,可得到不同的结果.这些对以后正确使用变分原理有一定的参考价值.     

1880-2006年中国夏季雨带类型的年代际变化特征

 利用1880-2006年中国东部地区夏季降水量及1951-2006年中国160个站夏季降水量和北半球大气环流资料,在夏季降水分型的基础上,研究了夏季雨型的年代际变化规律,分析了夏季各类雨型所对应的北半球500 hPa环流场的主要特征。结果表明：东部季风区和西部区存在着20～40 a左右的年代际振荡趋势,东北区则表现为明显的15 a左右的年代际变化特点;东部季风区四类雨型东亚大气环流差异显著,西部区二类雨型和东北区二类雨型欧亚大气环流的配置基本都相反。     

快速冷却电子的精确同步辐射谱与GRB辐射

普遍认为内激波中电子的同步辐射是γ射线暴快速光变辐射的主要辐射机制,但理论预言与观测结果始终符合不好.确认在内激波中电子因辐射损失而快速冷却,分析指出以往研究中求得的快速冷却电子同步辐射谱只是一个粗略的结果,由数值计算求得单电子快速冷却时的精确同步辐射谱,从而用一个统一模型合理解释观测到的长γ暴低能谱指数α的分布,拟合α与vFv谱的峰值能量Ep之间的相关.     

Cosmic‐ray rejection for single spectroscopic CCD images by means of template matching

This article describes a novel algorithm for cosmic‐ray rejection in single spectroscopic CCD images. This algorithm is based on a variation of template matching. It focuses on identifying those pixels belong to spectra, while other conventional algorithms tried to locate the cosmic‐ray hits directly. The main principle is applying template matching to find suspicious blocks, which is followed by surface patching to locate the legitimate pixels accurately. Therefore, the rest pixels are the ones corrupted by cosmic‐ray hits. Meanwhile, almost all the parameters are automatically extracted from the images. Examples of its performance are given for both simulated and observed images. It shows an advantage of significantly low false alarm rate with relatively high detection rate (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

An alternative symbiotic channel to Type Ia supernovae

By assuming an aspherical stellar wind with an equatorial disc from a red giant, we investigate the production of Type Ia supernovae (SNe Ia) via a symbiotic channel. We estimate that the Galactic birthrate of SNe Ia via the symbiotic channel is between  1.03 × 10⁻³  and  2.27 × 10⁻⁵ yr⁻¹  , while the delay time of SNe Ia has a wide range from ∼0.07 to 5 Gyr. The results are greatly affected by the outflow velocity and mass-loss rate of the equatorial disc. Using our model, we discuss the progenitors of SN 2002ic and SN 2006X.     

A Study on the Light Curves of GRBs

It is generally believed that the complexity and variability of the light curves of gamma-ray bursts (GRBs) are caused by the internal shocks, which would occur when a rapid shell catches up a slower one and collides with it. The electrons in the shock layer are heated by the shocks and radiate via the mechanisms of synchrotron radiation and inverse Compton scattering. Based on relativistic kinematics, a relation between the photon number of the emission from the rapidly moving shock layer and the number of the photons received by an observer is derived. Then, employing the angular spreading of the internal shock emission, the curve equation and profile of a single pulse are obtained, and the shape is typically in the shape of a fast rise and exponential decline. Furthermore, by using the model of the successive collisions of multiple shells under the condition of reasonable parameters, the observed light curves are fitted with a rather good effect. Therefore, by this means, more different types of light curves of GRBs can be explained.