Probing the nuclear activity with supermassive black holes

We report three new or updated techniques for probing the parameters of active galaxies based on the masses of their central black holes M_BH). First, we derived a near-IR analog of the bulge luminosity versus M_BH relationship. The low scatter makes it a promising new tool to study the black hole demographics. Next, we present relations between M_BH and the10 μm and 2-10 keV nuclear luminosity. They may help to study the M_BH evolution over wide redshift ranges. Finally, we measured M_BH in quasars from z ∼ 3.4 to z ∼ 0.3 to search directly for M_BH growth. Surprisingly, we found no evidence for growth implying that the majority of quasar host galaxies have undergone their last major merger at z ≥ 3. This revised version was published online in August 2006 with corrections to the Cover Date.     

A simple model for lensing by black holes in galactic nuclei

The lensing properties of the Plummer model with a central point mass and external shear are derived, including the image multiplicities, critical curves and caustics. This provides a simple model for a flattened galaxy with a central supermassive black hole. For the Plummer model with black hole, the maximum number of images is four, provided the black hole mass is less than an upper bound which is calculated analytically. This introduces a method to constrain black hole masses by counting images, thus applicable at cosmological distance. With shear, the maximum number of images is six and we illustrate the occurrence of an astroid caustic and two metamorphoses.     

A THREE-DIMENSIONAL ELASTIC NESTED-GRID MESO-(β-γ)SCALE ATMOSPHERIC MODEL——PARTI:MODEL DESCRIPTION

A three-dimensional elastic nonhydrostatic mesoscale(β-γ)model with nested-grid is presented.It uses a set of fullequations in terrain-following coordinates as its basic dynamic frame,which is solved with a time-splitting algorithmfor acoustic and gravity waves.The model physical parameterization includes a K-theory subgrid eddy mixing for cloudand free atmosphere,a bulk planetary boundary layer parameterization,and three types of sofisticated cloudmicrophysics schemes with double-parameters for hail-bearing clouds,warm clouds and snowing clouds respectively.The model is designed to be used flexibly for simulations of a variety of meso-and small-scale atmospheric processes,and can be improved as a regional and local operational NWP system in future.     

云南省红河地区2004年第一场透雨过程分析

利用2004年5月15～21日第一场透雨过程的高空资料,对产生强降雨天气的主要物理量进行分析,总结主要物理量的变化特征,揭示这次强降雨产生发展变化规律,对今后在预报过程中对主要物理量的变化引起重视,具有一定的参考意义。     

High-Altitude CUSP: The Extremely Dynamic Region in Geospace

The high-altitude dayside cusps (both northern and southern) are extremely dynamic regions in geospace. Large diamagnetic cavities with significant fluctuations of the local magnetic field strength have been observed there. These cusp diamagnetic cavities are always there day after day and are as large as 6 R_E Associated with these cavities are charged particles with energies from 20 keV up to 10 MeV. The intensities of the cusp energetic ions have been observed to increase by as much as four orders of the magnitude when compared with regions adjacent to the cusp which includes the magnetosheath. Their seed populations are a mixture of ionospheric and solar wind particles. The measured energetic ion fluxes in the high-altitude cusp are higher than that in both the regions upstream and downstream from the bow shock. Turbulent electric fields with an amplitude of about 10 mV/m are also present in the cusp, and a cusp resonant acceleration mechanism is suggested. The observations indicate that the dayside high-altitude cusp is a key region for transferring the solar wind mass, momentum, and energy into the Earth’s magnetosphere.     

不同对流参数化方案和初值场组合对四川两次暴雨影响的数值模拟

针对2004年9月2~6日四川盆地东北部一次持续性暴雨过程和2004年6月30日成都地区暴雨过程,利用MM5中尺度数值模式,进行了Grell、Kuo、KF及BM四种积云对流参数化方案与T213模式分析值及NCEP再分析值两种初始值组合的数值试验,分析了不同积云方案和初值组合的模拟性能。比较结果表明,MM5模式较好地再现了这两次强降水过程。在同一模式中,不同对流参数化方案和不同初值组合在降水落区和强度模拟上存在一定程度的差异。初步模拟表明NCEP资料模拟的降水强度较T213资料模拟的降水强度偏弱,但降水落区较T213资料模拟的更接近实况,T213资料模拟的降水空报现象较严重。以T213资料模拟得到的高度、温度场都较NCEP资料更有利于影响系统的加强,模拟的湿度场、散度场和垂直运动场都较NCEP资料更有利于强降水的发生。相对而言,NCEP资料模拟结果更接近实况,Kuo和Grell方案对初值表现出更为敏感。     

多积云参数化方案热带气旋路径集合预报试验

利用MM5模式采用5种积云参数化方案选项研究了2004～2006年共8个热带气旋路径的集合预报。结果表明,热带气旋路径预报对积云参数化方案的选取是敏感的,积云参数化方案之间优劣互补,而选择无积云参数化方案选项对热带气旋路径的预报有积极的贡献。采用3种路径集合预报方案研究的结果表明,集合方法对热带气旋路径预报有明显的改善,其中无积云参数化Grell、Betts—Miller和Kain—Fritsch4种积云参数化方案选项组合的集合预报效果最好,平均路径误差最小。     

Comparative Planetary Space Physics

It has been 60 years since the space physics as new branch of geophysics started to grow in 1957 when the space age was opened by a small satellite called sputnik. The knowledge of Earth and planetary space has been significantly extended and deepened, but the questions we are facing today are more challenging. A consensus reached is that we have to regard the Earth (planet) as an integrated system including all spheres from the inner core to the magnetosphere, and we should try to investigate some questions standing on the ground of interdisciplinary study, especially those questions related to Earth’s (planetary) evolution. Space environment as the outer part of a planetary system, commonly exists in all planets but also exhibits strong diversity. Here, we introduce the short history of basic ideas and methods of comparative study, the advantages on understanding of some issues of global scale, and the prospect from comparative perspective.     

西北地区春季云系的垂直结构特征飞机观测统计分析

根据2001年5—6月8架次的飞机探测资料,配合地面观测和卫星资料综合分析得出了西北地区春季云系的垂直结构宏微观特征,包括云厚、云底高度、云粒子浓度、含水量、有效半径、粒子谱分布函数等。降水性层状云厚平均约2000 m,低云含水量垂直方向上平均为0.07 g·m~(-3),中云含水量垂直方向上平均为0.03 g·m~(-3)。对比分析降水云和非降水云系的微物理特征量,两者存在显著的差异,降水性层状云有效半径要达到10～16μm。     

玻色-爱因斯坦凝聚和重力测量——2001年诺贝尔物理学奖评介

介绍了2001年诺贝尔物理学奖获得者康奈尔，韦曼，克特勒的科学研究成果，实验玻色－爱因斯坦凝聚（BEC）及其在理论上的意义和应用前景，讨论了BEC在研制高精度重力仪方面的应用问题，为此回顾了重力测量现状，朱棣文等研制的原子干涉重力仪和ClauserJ提出的物质波干涉重力仪，分析表明，如果利用BEC，则重力仪的测量精度在朱棣文等工作基础上将会有很大的提高。