The magnetic field and wind confinement of β Cephei: new clues for interpreting the Be phenomenon?     

J.-F. Donati  G.A. Wade  J. Babel  H_f. Henrichs  J.A. de Jong  T.J. Harries 《Monthly notices of the Royal Astronomical Society》2001,326(4):1265-1278

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Denudation rates of crystalline rock in the Huangling anticline of the Three Gorges of the Yangtze River in China since the Eocene     

张丽萍  杨达源  朱大奎 《中国科学D辑(英文版)》2003,46(9):928-940

The processes and rates of the weathering denudation of the bare crystalline rock are important problems in the field of geosciences[1—6]. Essentially, the weathering denudation process is the process of rock destruction and transportation. In different …  相似文献   

北淮阳及其邻接区地壳稳定性研究   总被引：1，自引：1，他引：0  

李细光  曾佐勋  彭晓文  曾克峰  张志 《大地构造与成矿学》2003,27(3):287-294

运用多学科、多技术相结合的研究方法,从现今构造应力场特征、现代地壳形变特征、主干断裂构造以及区域断裂活动性分析、新构造运动、地震活动、数值模拟等方面入手,对北淮阳及其邻接区地壳稳定性进行了全面而系统的研究,指出本区地震活动受走滑活动断裂控制,中、强地震集中于区内东南部和西北部NW向与NE向断裂交汇处;第四纪无大规模差异升降运动;数值模拟等综合分析表明,信阳地区的区域构造稳定性高,现代地壳形变量小,应力平缓,地震活动少且弱。  相似文献   

The heating of the solar corona     

R.?W.?WalshEmail author  J.?Ireland 《Astronomy and Astrophysics Review》2003,12(1):1-41

The heating of the solar corona has been a fundamental astrophysical issue for over sixty years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO and TRACE) have revealed the complex and often subtle magnetic-field and plasma interactions throughout the solar atmosphere in unprecedented detail. It is now established that any energy release mechanism is magnetic in origin - the challenge posed is to determine what specific heat input is dominating in a given coronal feature throughout the solar cycle. This review outlines a range of possible magnetohydrodynamic (MHD) coronal heating theories, including MHD wave dissipation and MHD reconnection as well as the accumulating observational evidence for quasi-periodic oscillations and small-scale energy bursts occurring in the corona. Also, we describe current attempts to interpret plasma temperature, density and velocity diagnostics in the light of specific localised energy release. The progress in these investigations expected from future solar missions (Solar-B, STEREO, SDO and Solar Orbiter) is also assessed.Received: 6 February 2003, Published online: 14 November 2003 Correspondence to: R. W. Walsh  相似文献   

Some Comments on the Magnetic Braking of CP Stars     

Yu. V. Glagolevskij 《Astrophysics》2003,46(3):319-328

The low rotation velocities of magnetic CP stars are discussed. Arguments against the involvement of the magnetic field in the loss of angular momentum are given: (1) the fields are not strong enough in young stars in the stage of evolution prior to the main sequence; (2) there is no significant statistical correlation between the magnetic field strength and the rotation period of CP stars; (3) stars with short periods have the highest fields; (4) a substantial number of stars with very low magnetic fields (B _e < 500 G) have rotation speeds that are typical of other CP stars; (5) simulations of the magnetic fields by Leroy and the author show that the orientation of dipoles inside rotating stars, both slow and fast, is consistent with an arbitrary orientation of the dipoles; and, (6) slow rotators with P>25 days, which form 12% of the total, probably lie at the edge of the velocity distribution for low mass stars. All of these properties conflict with the hypothesis of magnetic braking of CP stars.  相似文献   

长庆中部气田奥陶纪马家沟组储层成岩模式与孔隙系统   总被引：1，自引：2，他引：1  

吴亚生何顺利  卢涛达世攀  李跃刚戴永定 《岩石学报》2006,22(8):2171-2181

长庆中部气田奥陶纪马家沟组马五～马五储层的主要成岩作用包括:(Ⅰ)准同生白云石化作用;(Ⅱ)白云石对小球状硬石膏结核(简称"膏球")和板状硬石膏晶体的交代;(Ⅲ)石膏的溶解;(Ⅳ)自生石英、自生粘土矿物在白云石晶间生长;(Ⅴ)早期方解石的充填作用;(Ⅵ)晚期方解石的充填作用;(Ⅶ)钾石盐的充填作用;(Ⅷ)去白云石化作用。其中造成孔隙的是(Ⅰ)、(Ⅱ)、(Ⅲ),破坏孔隙的主要是(Ⅴ)、(Ⅵ)、(Ⅶ)、(Ⅷ)。最重要的成岩作用是(Ⅰ)、(Ⅱ)、(Ⅲ)。主要的成岩模式有:云化-溶蚀型、云化-溶蚀-充填型、云化-溶解型、云化-交代-溶解型、云化-交代-溶解-早充填型、云化-交代-溶解-早充填-晚充填型、云化-交代-溶解-早充填-晚充填-钾石盐充填型。其中云化-溶解型、云化-交代-溶解型以及云化-溶蚀型是形成孔隙的主要成岩方式。主要的孔隙系统类型有5种:密球型、"球 胀裂缝型"、"球 晶间溶孔型"、晶模孔型、晶间溶孔型。其中,密球型、"球 胀裂缝型"、"球 晶间溶孔型"是最主要的孔隙系统类型。长庆中部气田马五段储层的发育首先受沉积微相控制,即膏球的发育;在此基础上还受成岩方式控制。膏球发育于马五、马五、马五、马五,尤其是马五。白云石对硬石膏球的交代作用和石膏的溶解作用广泛发育于马五、马五、马五、马五、马五、马五、马五、马五地层中。早期方解石、晚期方解石和钾石盐的充填作用主要发育在马五、马五、马五和马五地层中,而在马五、马五地层中不发育。膏球在马五、马五、马五不发育。所以,马五、马五、马五是最好的储集层段马五、马五是其次的储集层段。马五、马五、马五是最差的储集层段。  相似文献   

南海热带气旋路径集合预报试验   总被引：6，自引：14，他引：6  

袁金南  万齐林  黄燕燕  丁伟钰 《热带气象学报》2006,22(2):105-112

利用3种不同模式的初始资料，通过它们生成得到16个不同的初始场，分别对2004年南海及其周边地区9个热带气旋个例进行集合预报试验，最后筛选得到了7个南海热带气旋初值集合成员，由此初步探讨了南海热带气旋初值集合成员的生成方法。结果表明，采用不同模式的初始资料生成得到初值集合成员的方法用于集合预报，对南海热带气旋路径预报有一些明显的改进。  相似文献   

Study on the Variational Assimilation Technique for the Retrieval of Wind Fields from Doppler Radar Data   总被引：2，自引：0，他引：2       下载免费PDF全文

WAN Qilin  XUE Jishan  ZHUANG Shiyu 《Acta Meteorologica Sinica》2006,20(1):1-19

This paper introduces a variational assimilation technique for the retrieval of wind fields from Doppler radar data. The assimilated information included both the radial velocity (RV) and the movement of radar echo. In this assimilation technique, the key is transforming the movement of radar echo to a new radar measuring variable- "apparent velocity" (AV). Thus, the information of wind is added, and the indeterminacy of recovering two-dimensional wind only by AV was overcome effectively by combining RV with AV. By means of CMA GRAPES-3Dvar and CINRAD data, some experiments were performed. The results show that the method of retrieval of wind fields is useful in obtaining the construction of the weather system.  相似文献   

多普勒天气雷达资料对中尺度模式短时预报的影响   总被引：22，自引：8，他引：22  

盛春岩  浦一芬  高守亭 《大气科学》2006,30(1):93-107

利用中尺度模式ARPS(The Advanced Regional Prediction System)及其资料分析系统ADAS(ARPS Data Analysis System),将国内新一代多普勒雷达(CINRAD)反射率及径向风资料直接用于中尺度数值模拟,通过一次华北地区暴雨过程的模拟对比试验,分析了雷达资料对初始场的改进效果及其对模拟结果的影响,结果表明:(1)利用雷达径向风资料对初始风场进行调整后,自近地面到对流层顶的u,v,w都发生了变化,调整后的初始风场在对流层中层变化最大.(2)利用雷达反射率进行微物理调整和云分析能调整初始场中的云水信息,使得雷达回波附近3 km以下的水汽混合比(qv)增加,4 km以下的雨水混合比(qr)增加,对流层(约10 km以下)的云水混合比(qc)增加,4～9 km的对流层上部云冰混合比(qi)和雪混合比(qs)增加.ADAS通过非绝热初始化调整温度场,从而得到了一个动力和热力上平衡的初始场.(3)模拟的1 h雨量与实况的对比表明,同时利用雷达反射率和径向风改进过的初始场能明显增强3 h内的降水强度和落区预报,改善中尺度数值模式短时定量降水预报.模拟的1 h流场对比分析表明,经雷达径向风调整后,能够在初始场中增加气旋性涡旋等中小尺度风信息,明显减少模式的spin-up时间.(4)通过对雷达径向风和反射率对模式初始场和模拟结果影响的对比分析发现,雷达径向风主要是改进初始风场,而雷达反射率主要是改进初始场中的湿度参数,增加初始场中云水等的含量,调整温度场.通过模拟的6 h降水对比发现,利用雷达径向风调整初始场后,对降水模拟有一定的改进,但效果不甚明显,而雷达反射率资料对定量降水预报改进效果明显,同时使用雷达径向风和反射率资料改进初始场后对降水的模拟效果最明显.  相似文献   

一类退缩反应扩散方程组初边值问题解的存在性和唯一性     

邹赢  李刚  徐金花 《南京气象学院学报》2006,29(2):242-248

利用紧性理论，证明了扩散现象中出现的一类退缩抛物型方程组初边值问题解的存在性和唯一性。  相似文献