加密重力测量数据管理程序的实现

在测绘生产中,测绘成果的管理和原始数据的预处理是非常重要的工作。本文介绍了以VS2008为平台开发一个加密重力测量数据管理程序的过程,详述了如何运用VC++结合ADO技术创建ACCESS数据库,实现对测量数据的录入、修改、删除、重力段差和重力值的计算、计算结果的显示输出。     

2008年河南持续低温、冻雨和暴雪成因

应用常规气象观测和1°×1°NCEP资料,分析了2008年1月中下旬河南持续低温、冻雨、暴雪的成因,结果表明:1月中下旬500 hPa极涡较历史同期明显偏东偏南,咸里海和孟加拉湾地区的高度明显偏低;冻雨出现时大气的温度垂直分布呈现中暖下冷的特征,存在明显的逆温层和＞0 ℃的暖层;暴雪产生时底层东北风明显加大.极涡位置偏东,有利于极地冷空气不断沿贝加尔湖脊前西北气流南下,中纬环流东高西低,有利于孟加拉湾水汽持续向东北方向输送,两者是导致河南出现持续低温雨雪天气的主因.冻雨发生时上空需存在厚度超过500 m的暖层(t＞0 ℃),暖层下有近2 000 m的t＜0 ℃的冷层,且950-750 hPa大气相对湿度＞90%.近地面东北急流的出现或东北风的加强,促进了低层的辐合或抬升,有助于垂直风切变加强和上升运动发展,对降水的加强有指示意义.     

2008年山东小麦秋冬连旱成因分析

对山东省2008年小麦播种至2009年1月的气候资料进行统计分析,结果表明：2008年11月份以后,降水持续偏少,是小麦受旱的主要原因,冬前没有适时浇灌越冬水等其他管理因素是小麦受旱的重要原因。     

一次α中尺度低涡暴雨的数值模拟

用WRF模式对2007年4月21—22日的一次中α低涡暴雨过程进行了高分辨率模拟,结果表明:(1)该低涡的产生与湖北西部的地形条件有一定的联系,低压倒槽系统为其提供了必要的环流背景,反演自FY-2 C卫星的TBB资料较好地反映了该中α低涡的整个活动过程。(2)对低涡发展最强阶段的动力和热力结构分析表明,低涡右侧为较强的上升运动,而其左侧则为下沉运动,在中低层冷空气上部有南侧暖湿空气上爬造成的次级上升运动;低涡左侧存在较明显的湿斜压锋区,后部则有明显的干冷气切入;南风风量对总体水汽输送的贡献要大于西风风量。(3)WRF模式中NOAH和热扩散陆面方案的对比分析表明,NOAH方案更加有利于低涡中心的发展,因此能够产生较热扩散方案更强的中心区降水,但是这种增强作用主要分布在低涡区附近,其他地区差别不大。     

气象探空数据动态比对中误差计算方法研究

在高空动态数据比对中,需要同时考虑系统误差与随机误差。采用多个探空仪同球比对施放的方法,从相对系统误差、标准偏差等方面,对被试探空仪进行比对评估,同时采取误差分离方法,计算被试探空仪的随机误差。考虑高空温度在对流层与平流层的不同变化趋势,采取细化分层方式进行计算,以反映大气特性。     

Comparative Studies of Different Mesoscale Convection Parameterization Schemes in the Simulation of Mei-Yu Front Heavy Rain

The mei-yu front heavy rainstorms occurred over Nanjing on 3 5 and 8 9 July 2003 and were simulated in this paper using the Weather Research and Forecasting Model (WRFv3.1) with various mesoscale convection parameterization schemes (MCPSs). The simulations show that the temporal and spatial evolution and distribution of rainstorms can be modeled; however, there was incongruity between the comparative simulations of four different MCPSs and the observed data. These disparities were exhibited in the simulations of both the 24-hour surface rainfall total and the hourly precipitation rate. Further analysis revealed that the discrepancies of vertical velocity and the convective vorticity vector (CVV) between the four simulations were attributed to the deviation of rainfall values. In addition, the simulations show that the mid-scale convection, particularly the mesoscale convection system (MCS) formation, can be well simulated with the proper mesoscale convection parameterization schemes and may be a crucial factor of the mei-yu front heavy rainstorm. These results suggest that, in an effort to enhance simulation and prediction of heavy rainfall and rainstorms, subsequent studies should focus on the development and improvement of MCPS.     

连云港沿海地区及近海风能资源评估

通过对连云港市30多年气象整编资料及沿海高密度自动气象站、6座测风塔、4座海岛气象站等加密观测资料研究,在充分考虑当地特殊地形特点的基础上,探讨了该地区沿海及近海风能资源的时空分布规律及特点,并重点对风湍流强度的特征及强湍流对风电的影响进行了剖析;研究表明,近海地区风能资源储量相对丰富,风速变化稳定,且风垂直切变较小,具有更为广阔的开发利用前景.     

翁田台地电场观测受干扰的因素分析

海南省文昌翁田台地电场数据质量自2019年3月开始下降,地电场数据质量下降主要表现为日相关系数偏低、北南向长极距与短极距数据曲线呈反向变化、绝缘度趋向于零等情况.2019年3月—2020年10月,我们分别对观测室装置系统、室外外线路、连接口等逐一进行详细的排查工作和电极、电缆的对比实验工作,最终确定影响因素为电极故障和...     

The influence of magnetic fields on neutrino-dominated accretion disc

We consider the influence of magnetic fields on the model of neutrino-dominated accretion flows (NDAFs) for gamma-ray bursts (GRBs) via the assumption that the accretion rate of the disc is totally caused by the torque of the Lorentz force, i.e. the magnetic braking of large-scale magnetic fields and magnetic viscosity of small-scale magnetic fields. We calculate the structure, composition, luminosity of neutrino emission and the Poynting flux, and the rate of mass loss driven by neutrino heating or launched centrifugally by large-scale magnetic fields, based on the physical condition of the magnetized NDAFs. It is shown that the magnetized disc is favourable to interpret the diverse prompt emissions as well as the X-ray flares observed in the early afterglow of GRBs.     

Old stellar population synthesis： new age and mass estimates for Mayall Ⅱ = G1

Mayall Ⅱ = G1 is one of the most luminous globular clusters （GCs） in M31. Here, we determine its age and mass by comparing multicolor photometry with theoretical stellar population synthesis models. Based on far- and near-ultraviolet GALEX photometry, broad-band UBVRI, and infrared JHKs 2MASS data, we construct the most extensive spectral energy distribution of G 1 to date, spanning the wavelength range from 1538 to 20 000A. A quantitative comparison with a variety of simple stellar population （SSP） models yields a mean age which is consistent with G1 being among the oldest building blocks of M31 and having formed within ～1.7 Gyr after the Big Bang. Irrespective of the SSP model or stellar initial mass function adopted, the resulting mass estimates （of order 10^7M⊙） indicate that GI is one of the most massive GCs in the Local Group. However, we speculate that the cluster＇s exceptionally high mass suggests that it may not be a genuine GC. Our results also suggest that G1 may contain, on average, （1.65±0.63） × 10^2L⊙ far-ultraviolet-bright, hot, extreme horizontal-branch stars, depending on the adopted SSP model. In addition, we demonstrate that extensive multi-passband photometry coupled with SSP analysis enables one to obtain age estimates for old SSPs that have similar accuracies as those from integrated spectroscopy or resolved stellar photometry, provided that some of the free parameters can be constrained independently.