基于OpenGL的3维场景矢量打印输出研究与实现

3维场景的打印输出是3维GIS的基本功能之一。目前的3维GIS的可视化功能大多数是基于OpenGL实现的。OpenGL为了保持其与操作系统的无关性,没有直接提供场景的打印功能。因此,需要采用特殊的方法实现OpenGL的场景打印。通常,有三种方式实现该功能:位图打印、渲染打印和反馈打印。前两种输出的是当前屏幕渲染的栅格图像;后者输出的是投影在屏幕上的矢量图形。相对于位图打印和渲染打印,反馈打印(即矢量打印)的输出精度较高。目前的GIS平台实现矢量打印输出的较少。提出一种矢量打印输出的方法,并给出在VC 开发环境下的一些实现细节。     

1951—2015年乌鲁木齐市升温过程频数及强度气候特征

利用乌鲁木齐市气象站1951年1月1日至2015年12月31日的逐日气温资料,以日最高气温及其升温幅度为指标,整理出乌鲁木齐市近65年升温过程数据库,将升温过程分为Ⅰ级(弱)、Ⅱ级(中等强度)、Ⅲ级(较强)、Ⅳ级(强)以及Ⅴ级(极强)5个等级,分析了乌鲁木齐市各级升温过程发生频数、持续日数、过程不同时段升温幅度、过程最高气温、过程最高气温距平偏高幅度等要素气候特征。结果如下：(1)1951—2015年,乌鲁木齐市出现升温过程5677次,平均每年87.3次,其中Ⅰ级(弱)升温过程占67.8 %。升温过程发生频数的季节分布较均匀,但在春季相对较多。近65年来,年平均升温过程发生频数在7个年代际中差异不大,没有明显的线性变化趋势。(2)1951—2015年,乌鲁木齐市5677次升温过程的平均持续日数为2.14?d,其中持续1 d的过程占43.0 %。随升温过程等级由Ⅰ级到Ⅴ级提高,过程持续日数最高出现频率也从1?d过渡到3?d。升温过程持续日数在春季4、5月份最长。(3)1951—2015年,乌鲁木齐市过程升温幅度平均为5.76℃,在春季最大、秋季最小。Ⅳ级(强)以及Ⅴ级(极强)的过程升温幅度最大的月份分别是5月和3月。65年来,乌鲁木齐市升温过程的最大24h、48h和72h升温幅度平均值分别为3.72℃、6.12℃和8.23℃,最大24 h升温幅度在冬季最大、夏季最小,最大48 h和72 h升温幅度都是在春季最大、秋季最小。(4)1951—2015年,乌鲁木齐市升温过程的最高气温平均值为14.52℃,在夏季7、8月最高,在冬季各月最低,带有显著的季节背景特征。过程最大日气温距平的平均值为2.93℃。Ⅳ级(强)和Ⅴ级(极强)升温过程的日气温距平偏高幅度最大月份分别出现在1月(11.73℃)和12月(19.10℃)。     

天然气中甲烷和CO2的二元同位素特征

不同成因的天然气由于形成温度不同,往往会有不同的稳定同位素特征。但是,由于经常不能同时获得天然气以及它的生成母体的同位素成分,很难用单独的C或H同位素成分来确定它的形成温度。在形成天然气时,不同的温度会形成不同的二元同位素的浓度,温度越低,二元同位素的比例越大,因此只需要知道天然气本身的二元同位素的浓度,就可以确定形成温度,从而避免了需要知道天然气生成母体的同位素成分这一难题。本文利用高级量子化学计算,预测了不同温度下天然气中甲烷和CO2气体的二元同位索（Clumped isotope）的特征,提供用于天然气成因分析的新方法。     

高精度重磁勘探在推覆体下找煤中的应用

应用高精度重磁勘探方法解决在推覆体下找煤问题.利用磁异常研究辉绿岩体的赋存状态,肯定了推覆体的存在;根据重力异常及数据处理结果研究推覆体下煤系地层的分布,指出太山-许台重力低带是测区内找煤最为有利的靶区.高精度重磁勘探是推覆体下寻找煤系地层前期勘探的有效手段之一.     

冬季东亚中纬度西风急流对我国气候的影响

利用1957—2001年欧洲中期数值天气预报中心再分析资料及地面台站观测资料,分析了冬季东亚西风急流与我国气候的关系。首先定义了冬季东亚西风急流强度指数(区域30°~35°N,127.5°~155°E冬季200 hPa纬向风u200平均值的标准化值)和切变指数(区域15°~25°N,100°~115°E与区域30°~40°N,100°~115°E的平均u200之差的标准化值),这两个指数能较好地反映冬季东亚西风急流的强度变化和位置的南北移动,二者相关系数为-0.48,通过99%信度检验。西风急流强度与亚洲和西太平洋大范围的大气环流有密切关系,而西风急流位置移动则与印度洋、中东太平洋的大气环流有密切关系,并分析了冬季急流强度指数和切变指数与我国温度和降水的关系。结果表明：当西风急流强度偏强时,西风急流位置偏北,此时在急流入口区左侧由于气流辐合造成低层气压上升,在出口区左侧则由于气流发生强烈辐散,引起低层气压下降,所以西伯利亚地区上空从对流层低层到中层高度值升高,北太平洋高度值降低,东西向气压差加大的形势,同时东亚大槽偏强,海陆气压差加大和东亚大槽偏强,导致冬季风强度偏强,引起我国从北到南的陆面降温,同时30°~40°N低层有下沉气流,使得华北、华中和长江中下游地区降水偏少;当西风急流强度偏弱时,西风急流位置偏南,整个东亚地区存在南风异常,东亚冬季风较弱,在25°N附近有上升气流,此时华南和内蒙古、华北降水偏多,内蒙古地表温度偏高。     

水体细菌碱性磷酸酶及其编码基因研究进展

水体溶解性反应磷是浮游植物可直接利用的主要磷营养形式,细菌碱性磷酸酶催化的有机磷矿化过程则是维持溶解性反应磷供给的重要途径.通过总结细菌碱性磷酸酶的种类与分布特征,发现主要包括Pho A、Pho X和Pho D 3种类型细菌碱性磷酸酶,其中超过50%的Pho X分布于细菌细胞的外部环境,对溶解性反应磷的循环再生尤为重要.综述水体产碱性磷酸酶细菌群落组成的研究进展,以及影响编码基因表达的环境因素,对比分析产碱性磷酸酶细菌群落鉴定方法的特点及发展趋势.细菌碱性磷酸酶编码基因的研究多关注寡营养海洋生态系统,对于同样存在磷限制问题的富营养化湖泊生态系统鲜有涉及,而构建针对典型富营养化湖泊生态系统的细菌宏基因组数据库,则可为建立淡水生态系统细菌碱性磷酸酶及其编码基因的研究方法奠定基础,有助于认识湖泊水华频发的微生物学驱动机制.     

TECTONO-SEDIMENTARY EVOLUTION OF THE TERTIARY BASINS IN EASTERN TIBET: CONSTRAINING THE RAISING OF TIBETAN PLATEAU

TECTONO-SEDIMENTARY EVOLUTION OF THE TERTIARY BASINS IN EASTERN TIBET: CONSTRAINING THE RAISING OF TIBETAN PLATEAU1　YinA ,HarrisonTM .TheTectonicEvolutionofAsia[M] ..Cambridge :CambridgeUniversityPress,1996 .4 4 2～ 4 85. 2　SunH ,ZhengD .FormationevolutionanddevelopmentofTibetanPlateau[M ] .Guangzhou :GuangdongScienceandTechnologyPress,1998.73～ 2 30 . 3　ShiY ,LiJ,LiB .UpliftandEnvironmentalChangesofTibetanPlateauintheLateCen…     

Complete genome of Cobetia marina JCM 21022T and phylogenomic analysis of the family Halomonadaceae

Cobetia marina is a model proteobacteria in researches on marine biofouling. Its taxonomic nomenclature has been revised many times over the past few decades. ~To better understand the role of the surface-associated lifestyle of C. marina and the phylogeny of the family Halomonadaceae, we sequenced the entire genome of C. marina JCM 21022 ~T using single molecule real-time sequencing technology(SMR~T) and performed comparative genomics and phylogenomics analyses. ~The circular chromosome was 4 176 300 bp with an average GC content of 62.44% and contained 3 611 predicted coding sequences, 72 t RNA genes, and 21 r RNA genes. ~The C. marina JCM 21022 ~T genome contained a set of crucial genes involved in surface colonization processes. ~The comparative genome analysis indicated the significant diff erences between C. marina JCM 21022 ~T and Cobetia amphilecti KMM 296(formerly named C. marina KMM 296) resulted from sequence insertions or deletions and chromosomal recombination. Despite these diff erences, pan and core genome analysis showed similar gene functions between the two strains. ~The phylogenomic study of the family Halomonadaceae is reported here for the first time. We found that the relationships were well resolved among every genera tested, including Chromohalobacter, Halomonas, Cobetia, Kushneria, Zymobacter, and Halotalea.     

Investigation on semi-direct and indirect climate effects of fossil fuel black carbon aerosol over China

A Regional Climate Chemistry Modeling System that employed empirical parameterizations of aerosol-cloud microphysics was applied to investigate the spatial distribution, radiative forcing (RF), and climate effects of black carbon (BC) over China. Results showed high levels of BC in Southwest, Central, and East China, with maximum surface concentrations, column burden, and optical depth (AOD) up to 14 μg?m^?3, 8 mg?m^?2, and 0.11, respectively. Black carbon was found to result in a positive RF at the top of the atmosphere (TOA) due to its direct effect while a negative RF due to its indirect effect. The regional-averaged direct and indirect RF of BC in China was about +0.81 and ?0.95 W?m^?2, respectively, leading to a net RF of ?0.15 W?m^?2 at the TOA. The BC indirect RF was larger than its direct RF in South China. Due to BC absorption of solar radiation, cloudiness was decreased by 1.33 %, further resulting in an increase of solar radiation and subsequently a surface warming over most parts of China, which was opposite to BC’s indirect effect. Further, the net effect of BC might cause a decrease of precipitation of ?7.39 % over China. Investigations also suggested large uncertainties and non-linearity in BC’s indirect effect on regional climate. Results suggested that: (a) changes in cloud cover might be more affected by BC’s direct effect, while changes in surface air temperature and precipitation might be influenced by BC’s indirect effect; and (b) BC second indirect effect might have more influence on cloud cover and water content compared to first indirect effect. This study highlighted a substantial role of BC on regional climate changes.     

Acceleration by Magnetic Mirrors and Alfven Waves in Molecular Outflows

The configuration of the magnetic field associated with a protostar surrounded by a circumstellar disk is assumed to be a kind of magnetic mirror, which reflects the particles at its throat located nearby the disk midplane, and then extracts them out of the star and the disk. Turbulent Alfven waves are excited due to anisotropic temperature distribution caused by the existing magnetic field in the environment. Accelerated by turbulent Alfven waves, the particles coming out of the young stellar object and the circumstellar disk can reach the expected velocities around 300 km s^-1 at a typical distance 0.1 pc from the central star. The wave energy is converted from the thermal energy stored in the system consisting of the early stage star associated with the disk and their environment, and a small fraction of which is enough. The coefficient η, indicating the efficiency of converting thermal energy to wave energy, is equal to 10^-11. This revised version was published online in July 2006 with corrections to the Cover Date.