天气学和天气预报的研究进展

全面回顾了75年来中国科学院大气物理研究所科研人员在气团、锋面、梅雨、寒潮、阻高、副高、暴雨、高低空急流、亚澳季风区内涡旋和对流等现象的天气学研究进展及其在不同时期所取得的研究成果,总结了在短中期天气预报及短期气候预测领域在模式发展和改进以及在数值模拟等方面所取得的成就和进展.同时指出模式发展和预测在中国数值天气预报及短期气候预测方面所做出的贡献.     

基于改进LM-GN算法的磁性目标定位方法研究

利用三轴磁传感器阵列对水下磁性目标进行定位是典型的非线性最小二乘优化问题,传统高斯– 牛顿（GN）法和列文伯格–马夸尔特（LM）算法在求解该问题时具有初值敏感性问题。通过引入信赖域搜索技术,对 LM 算法进行改进,并基于改进的 LM 算法实现磁性目标定位,又通过设置判断阈值来评估迭代点与最优解的距离,提出一种结合改进 LM 算法和高斯–牛顿法特点的改进 LM-GN 算法,既降低了算法对初始值的依赖性,又提高了运行效率。仿真实验结果表明：该方法可以克服现有方法中受初始值影响较大的问题,对目标特征参数的估计更精确,且收敛速度快,具有一定的实际应用价值。     

Reduction of surface subsidence risk by fly ash exploitation as filling material in deep mining areas

The possibility of filling empty underground spaces, which exist owing to the extraction of mineral raw materials, with fly ash and cement fly ash mixes has been studied for the purpose of reducing the impact of deep mining on the surface. The method of physical modelling was used to study the behaviour of fly ash mixes deposited in extracted mine spaces. The models were constructed for two different geometries of underground extracted mine spaces: into cavities of the type of large slits created in the course of mining in steeply lode deposits without subsequently filling the empty space and in vertical shafts of rectangular or circular cross-section with horizontal side headings that have partly caved in due to mine shocks or other seismic events.     

IRAS 20231+3440区外流激发源的性质研究

给出红外点源IRAS 20231 3440附近恒星形成区近红外．JHK’和H2成像观测结果，以及与该IRAS点源成协的近红外点源IRS1的K波段分光观测结果．．JHK’观测显示该区域存在嵌埋的年轻星天体，H2窄波段观测揭示了若干个氢分子发射结点，其中有几个结点排列成线形，暗示分子氢喷流的存在．喷流的北部与已知观测的分子外流成协，表明二者之间存在联系．喷流的走向提示IRS1可能是其激发源，对IRS1的K波段分光观测给出了进一步的证据．从近红外、MSX及IRAS资料估计出IRS1的能谱分布，表明它是一个处于ClassI状态的中等质量的年轻星天体．     

VIDEO AND PHOTOGRAPHIC SPECTROSCOPY OF 1998 AND 2001 LEONID PERSISTENT TRAINS FROM 300 TO 930 nm

Spectra of persistent meteor trains were observed at wavelength between 300 and 930 nm. Two obtained train spectra during the 1998 and 2001 Leonid meteor showers are reported here. During the 1998 Leonids, one train was detected by a photographic camera with a spectrograph covering 370–640 nm region. On the other hand, during the 2001 Leonids, video observations were carried out using image intensified cameras in ultraviolet (UV), visible and near infrared (near-IR) wavelengths. Temperatures in persistent trains have been measured by atmospheric O₂ A(0,1) band at the wavelength near 864.5 nm. From a video spectrum obtained just 7 s after parent fireball’s flare, a rotational temperature of 250 K at altitude of 88.0±0.5 km was estimated. We can say that the cooling time scale of train strongly depends on the initial mass of its fireball at least for Leonids. Based on cooling constant calculated from our results, we estimated a temperature of ∼ ∼130 K as a final exothermic temperature at early stage of persistent trains.     

Enhanced Star Formation in Seyfert 2 Galaxies

In this paper, we report our preliminary results on enhanced star formation activity in Seyfert 2 galaxies. By re-analysing the Tully-Fisher relation for Whittle's (1992) sample and for a Seyfert 2s' sample selecting from Veron-Cetty and Veron (1996), we find that (1) almost all Seyfert 2 galaxies with circumnuclear star formation have a ratio of far infrared (FIR) to blue luminosities (L_FIR/L_B) to be larger than 1/3; (2) for Seyfert 2 galaxies with L_FIR/L_B > 1/3, the Tuly-Fisher relation is similar to that of the normal spiral galaxies; while for those with L_FIR/L_B ≥ 1/3, they are significantly different from the normal ones, which confirms Whittle's suggestion of enhanced star formation activities in the circumnuclear regions of these Seyfert 2 galaxies. This revised version was published online in July 2006 with corrections to the Cover Date.     

在97.8GHz处测量地球大气的不透明度

用研制的全自动辐射计在97．8GHz上测量南京市内大气的不透明度以及这种不透明度随时间的变化．辐射计记录大气在不同天顶高度的辐射温度,由此测出天顶方向的大气不透明度。在56小时的测量时间内,取得了1400多组数据,拟合得到了在观测时段内天顶方向的大气不透明度在0．2至0．7之间,典型值为0．4,表明测试地点的大气条件允许进行3mm波段的射电天文观测．由于在工作频段内大气不透明度的主要来源是对流层水汽的吸收,测量的不透明度可用来直接反映大气内水汽的含量,并实时校准大气吸收．     

Experimental study of extreme shear stress for shallow flow under simulated rainfall

The raindrop impact and overland flow are two major factors causing soil detachment and particle transportation. In this study, the turbulent characteristics of the shallow rain‐impacted water flow were investigated using a 2‐D fibre‐optic laser Doppler velocimetry (FLDV) and an artificial rainfall simulator. The fluctuating turbulent shear stress was computed using digital data processing techniques. The experimental data showed that the Reynolds shear stress follows a probability distribution with heavy tails. The tail probability increases with an increase of rainfall intensity or raindrop diameter, and it decreases with an increase of Reynolds number. A modified empirical equation was derived using both the raindrop diameter and rainfall intensity as independent variables to provide a better prediction of the Darcy‐Weisbach friction coefficient f under rainfall conditions. Copyright © 2009 John Wiley & Sons, Ltd.     

手机短信在无人值守地震监测点防盗报警中的应用

随着无人地震监测点的不断增加,其防盗问题便摆在我们面前.文章介绍了在无人地震监测点安置防盗装置,在检测到有人非法入侵盗窃的信号时,其报警消息通过手机 Modem 板以手机短信的方式通知相关工作人员进行处理.文中对防盗装置、手机 Modem 板、单片机的硬件组成进行了描述,对单片机的控制程序作了介绍.以这种传递报警信号的工作方式对于无人值守地震台是比较可行的,对减少地震台站损失,提高运转连续率和工作质量,具有一定实用价值.     

甘肃桦树沟铁铜矿床地球化学及成因

甘肃桦树为铁铜矿床地质、同位素地球化学、包裹体地球化学、同位素年代学研究表明，该矿床形成于震旦纪裂陷海盆环境，矿床成因属典型的热水沉积成矿。