基于MICAPS系统的气象图形Web显示

利用MICAPS系统后台运行程序,通过修改相关参数和编写程序,将天气实况、城市预报和数值预报产品等气象数据,在Web服务器上实时自动生成预报员熟悉的MICAPS图形,并在叠加底图后保存为标准图像文件.再通过Web语言设计,实现在Web网络上提供实时的、全面的、专业的气象图形,从而提高了气象网站的专业性和服务功能.     

双流冬草莓低温冻害天气特征及防冻措施探讨

双流县作为我国最大的冬草莓生产基地,低温冻害是冬季生产关键期的主要气象灾害。本文对2005年初低温冻害进行了分析,归纳出了双流县冬草莓低温冻害的发生规律及冻害临界温度指标,并提出了具体的防冻措施。     

Scaling of oblique impacts in frictional targets: Implications for crater size and formation mechanisms

Almost every meteorite impact occurs at an oblique angle of incidence, yet the effect of impact angle on crater size or formation mechanism is only poorly understood. This is, in large part, due to the difficulty of inferring impactor properties, such as size, velocity and trajectory, from observations of natural craters, and the expense and complexity of simulating oblique impacts using numerical models. Laboratory oblique impact experiments and previous numerical models have shown that the portion of the projectile’s kinetic energy that is involved in crater excavation decreases significantly with impact angle. However, a thorough quantification of planetary-scale oblique impact cratering does not exist and the effect of impact angle on crater size is not considered by current scaling laws. To address this gap in understanding, we developed iSALE-3D, a three-dimensional multi-rheology hydrocode, which is efficient enough to perform a large number of well-resolved oblique impact simulations within a reasonable time. Here we present the results of a comprehensive numerical study containing more than 200 three-dimensional hydrocode-simulations covering a broad range of projectile sizes, impact angles and friction coefficients. We show that existing scaling laws in principle describe oblique planetary-scale impact events at angles greater than 30° measured from horizontal. The displaced mass of a crater decreases with impact angle in a sinusoidal manner. However, our results indicate that the assumption that crater size scales with the vertical component of the impact velocity does not hold for materials with a friction coefficient significantly lower than 0.7 (sand). We found that increasing coefficients of friction result in smaller craters and a formation process more controlled by impactor momentum than by energy.     

Adaptive Optics Image Restoration Based on Frame Selection and Multi-frame Blind Deconvolution

Restricted by the observational condition and the hardware, adaptive optics can only make a partial correction of the optical images blurred by atmospheric turbulence. A postprocessing method based on frame selection and multi-frame blind deconvolution is proposed for the restoration of high-resolution adaptive optics images. By frame selection we mean we first make a selection of the degraded (blurred) images for participation in the iterative blind deconvolution calculation, with no need of any a priori knowledge, and with only a positivity constraint. This method has been applied to the restoration of some stellar images observed by the 61-element adaptive optics system installed on the Yunnan Observatory 1.2m telescope. The experimental results indicate that this method can effectively compensate for the residual errors of the adaptive optics system on the image, and the restored image can reach the diffraction-limited quality.     

年轻星天体的质量

质量是恒星最基本、最重要的物理量之一,它在恒星形成和演化过程中起着至关重要的作用.年轻星天体的形成机制以及早期演化过程是彻底解决恒星形成问题的关键所在,而年轻星天体形成过程中的物质下落、质量吸积以及外流等物理过程都与年轻星天体的质量密切相关.该文介绍了确定年轻星天体质量的一些常用方法,包括利用开普勒定律的动力学方法、赫罗图方法、年轻星天体脉动方法和磁层吸积方法等.并对这些方法的适用范围及测量精度进行了评述,还综述了各种方法的研究进展及未来可能的发展.     

Maturation related changes in the distribution of ester bound fatty acids and alcohols in a coal series from the New Zealand Coal Band covering diagenetic to catagenetic coalification levels

A rank series of lignites and coals of low to moderate maturation levels (vitrinite reflectance (R₀): 0.27–0.8%) from the New Zealand Coal Band were investigated using alkaline ester cleavage experiments to reveal compositional changes of ester bound components (fatty acids and alcohols) during increasing maturation. Ester bound alcohols are found to be present in highest amounts in the very immature lignite samples (R₀: 0.27–0.29%), but show a rapid decrease during early diagenesis. Ester bound fatty acids also show an initial exponential decrease during diagenesis, but reveal an intermittent increase during early catagenesis before decreasing again during main catagenesis. This intermittent increase was related to the short chain fatty acids. To obtain a maturity related signal and to eliminate facies related scattering in the amounts of fatty acids in the coal samples, the carbon preference index of fatty acids (CPI_FA) parameter is introduced here. For the long chain fatty acids (C₂₀–C₃₂) originating from terrigenous plant debris, the CPI_FA decreases with increasing maturity, showing a strong maturation related signal. During diagenesis, the same trend can be observed for the short chain fatty acids, but the intermittent increase in the amounts of short chain fatty acids is also accompanied by high CPI_FA values. This indicates less altered organic biomass at this advanced maturation level and is in contrast to the mature CPI_FA signal of the long chain fatty acids of the same samples. One possible reason for this discrepancy could be extremely different amounts of short and long chain fatty acids in the original source organic matter of these samples. However, another intriguing explanation could be the incorporation of immature bacterial biomass from deep microbial communities containing C₁₆ and C₁₈ fatty acids as main cell membrane components. Deep microbial life might be stimulated at this interval by the increasing release of thermally generated potential substrates from the organic matrix during early catagenesis. In contrast to the fatty acids, the high amounts of alcohols in the immature lignite samples are also visible in the alkene distribution from the open system pyrolysis experiments of the organic matrix before and after saponification.     

A novel procedure to detect low molecular weight compounds released by alkaline ester cleavage from low maturity coals to assess its feedstock potential for deep microbial life

In recent years the widespread occurrence of microorganisms was demonstrated in deep marine and terrestrial sediments. With this discovery inevitably the question of the potential carbon and energy sources for this deep subsurface microbial life arises. In the current study a new method for the investigation of low molecular weight (LMW) organic acids linked to the kerogen matrix is presented. These LMW organic acids form a potential feedstock for deep microbial populations. Twelve coal samples of different maturity (vitrinite reflectance (R₀) of 0.28–0.80%) from several coal mines on the North and South Island of New Zealand (NZ) were examined to assess the amount of bound LMW organic acids. Formate, acetate and oxalate were detected in significant amounts whereas the amounts of these compounds decrease with increasing maturity of the coal sample. This decrease of LMW organic acids mainly correlates to the phase of diagenetic alteration of the organic matter characterized by the release of oxygen containing compounds. Concomitantly, it coincides with temperature conditions assumed to be still compatible with microbial life in the deep subsurface. First assessments of the feedstock potential and generation rates of LMW organic acids indicate that the NZ coals investigated exhibit the potential to feed deep terrestrial microbial life with appropriate substrates over geological time spans.     

华北克拉通东部新元古代宏体化石生物地层序列

华北克拉通东部是中国晚前寒武纪地层出露最为完整、连续的地区,特别是华北克拉通东缘连续出露了新元古代自老至新的全部地层,是对比和衔接中国南、北方晚前寒武纪地层的关键地区。在该地区所发现和建立的宏体化石群——“龙凤山生物群”、“辽南生物群”和“淮南生物群”可能是新元古代“南华大冰期”前后较为独特的生物群落,其中相当部分可能归属于多细胞后生动物和多细胞藻类,是地球早期生命景观的重要代表。因此,对这些新元古代早期生物群的研究将可能揭示比陡山沱期更早的多细胞后生动植物的演化面貌,在演化生物学上意义重大。近年来,在地调项目的资助下,开展了华北克拉通东部地区的新元古代年代地层及生物地层的研究。本文综合现有资料,详细记述了华北克拉通东部（燕山地区和辽南、徐淮地区）含宏体化石的新元古代地层及其宏体化石特征、组合面貌和生物地层序列。同时,依据宏体化石记录,探讨了中国新元古代地层的对比问题。     

铜矿数字矿床模型专家系统的原理与技术实现

数字矿床模型是指将传统的地质学语言描述的矿床特征,转化成计算机可以识别的数字和符号,并加入人工智能的推理规则和知识,使之具备矿床自动推理和勘查辅助决策的功能。本项研究是在基于前人的工作基础上,结合国内外数字矿床模型的先进理论和经验进行了系统的实现。本文论述了铜矿床数字化的方法原理以及在系统实现时的关键性技术问题。系统知识库和规则库的建立是在多位铜矿专家的协助下完成的,专家对一系列先验概率等相关参数进行赋值,并用统计学方法下进行了处理。铜矿专家系统中知识库和规则库的保存和管理使用了数据库开发技术,采用数据挖掘作为知识发现的新手段。系统使用产生式规则,采用主观贝叶斯方法为推理的总体算法,搜索策略采用广度优先向前搜索的策略;在地质证据的输入方面不只提供与铜矿类型直接相关的证据,同时系统也提供了更为充分的地质证据,使推理的过程更加可靠和合理,同时地质词典功能的加入方便用户对相关地质术语进行查询和检索。系统不仅能实现单一成因的矿床进行推理,也能对复合矿床类型进行推理。     

酸性流体对碳酸盐岩储层的改造作用

普遍认为CO2、有机酸及H2S是碳酸盐岩储层溶蚀作用的酸性流体。CO2对碳酸盐岩储层的溶蚀作用已有不少学者进行了研究,本文则以一个全新的模拟实验方式对不同类型碳酸盐岩在有机酸和H2S水溶液中的相对溶蚀能力进行了研究,结果发现随温度从常温升高至200℃,有机酸对碳酸盐岩的溶蚀能力由弱变强再变弱,在90℃左右溶蚀能力最强。而H2S水溶液对碳酸盐岩的溶蚀作用则明显不同,60℃时基本达到最大溶蚀率,温度继续升高后,溶蚀能力一直维持在较高的水平并略有增加,150℃后突然降低。由于H2S主要是硫酸盐高温热还原产物（TSR）,因而在碳酸盐岩成岩早期阶段,溶蚀作用的流体可能主要是有机酸和C02,而在深埋阶段,H2S水溶液则可能是溶蚀作用的主要流体。