华南及邻近海域夏季深对流活动气候特征

利用具有较高时空分辨率与很好时空完整性的11年(1996—2007年，无2004年)6—8月静止卫星数字红外云图和TBB资料，给出了华南及邻近海域夏季深对流活动气候分布特征，并同文献中给出的雷暴日分布和闪电分布进行了对比分析。结果表明，华南及邻近海域夏季深对流活动有5个活跃中心，其月变化特征与大尺度环流背景密切相关。6月华南陆地区域深对流活动较活跃，7、8月南海海域深对流活动较活跃。华南及邻近海域深对流活动具有间歇性发展特征，其周期大约为3～5候，但华南海岸线附近为海陆过渡区域，深对流活动持续比较活跃且间歇性特征不突出；深对流活动旬与候变化特征表明华南陆地区域和南海海域深对流活动呈现反相关变化趋势。深对流活动的日变化特征显示该区域陆地与海洋、山地与盆地的热力差异所导致的海陆风环流与山谷风环流使得华南海岸线附近区域的深对流活动具有午后向陆地传播、午夜后向海洋传播的特征，山地与盆地的深对流活动具有显著的午夜后向盆地传播的特征。深对流活动日变化特征还表明该区域不仅具有一般热对流、海洋深对流和双峰型深对流等多种类型对流活动，且两广海岸线邻近区域具有持续时间长、日变化较不显著的海岸线深对流和其它天气系统触发和维持的深对流。     

关于OH/IR星的质量损失率计算公式的讨论

利用几种不同的半经验公式计算一批OH／IR星的质量损失率,并通过比较计算结果来讨论所用的公式．在一些情况下,计算质量损失率必须先给定气尘比．通过计算出样品星的气尘比,并讨论气尘比的变化情况,以修正由尘埃质量损失率到总质量损失率的关系式．     

Structural properties of (Mn1-x Fe x )Nb2O6 columbites from X-ray diffraction and IR spectroscopy

A suite of (Mn_1-x Fe _x )Nb₂O₆ (x=0, 0.05, 0.25, 0.50, 0.75, 1) columbite samples has been prepared by solid-state reaction from oxides. X-ray diffraction and spectroscopic investigations have been carried out in order to gain different perspectives on how the solid solution adapts at different length scales to cation mixing. X-ray powder diffraction and powder absorption IR spectroscopy data are presented. The powder diffraction data show that there is no significant excess volume of mixing on the Fe–Mn columbite join. All the unit-cell parameters decrease linearly as a function of increasing Fe content. Substitution of Fe²⁺ for the larger Mn²⁺ cation causes a decrease in the volume of the A polyhedron, which also becomes more regular with respect to both bond-length and edge-length distortion parameters. No significant variation of the B site has been observed. Wavenumber shifts of the IR peaks nearly all vary linearly with composition, consistent with linear variations of the lattice parameters. Line broadening has been quantified by autocorrelation analysis of the IR spectra. This is interpreted as suggesting that there is some element of local strain or positional disorder at the length scale of second or third nearest neighbours around sites occupied by Fe.     

2007年夏季我国深对流活动时空分布特征

利用逐时FY-2C卫星红外亮温 (T_BB) 资料讨论了2007年夏季 (6—8月) 我国深对流活动的时空演变特征,并同10年的深对流活动特征进行了对比分析。从T_BB≤-52℃统计特征来看,2007年夏季我国大陆深对流活动主要集中在4个区域:华南沿海地区,青藏高原,云贵高原东部及四川、重庆,江淮流域。我国中东部地区深对流日际变化特征表明:不同月份深对流分布特征不同,深对流活动具有明显的间歇性、波动性特征。对比10年T_BB≤-52℃统计结果来看,2007年夏季深对流日变化具有如下异常特征:华南地区深对流具有午后发展特征;青藏高原深对流活动持续时间明显短于10年统计结果,并且东传特征不明显;贵州东部、四川东北部山区、湖北西部山区、山东丘陵地带、江淮流域与华北平原深对流日变化表现出明显的多峰特征;江淮流域深对流日变化具有明显的向东传播特征。     

四川盐边基性—超基性杂岩体中角闪石矿物学研究

本文采用光学法、探针分析法、红外光谱法、单晶X射线衍射法对杂岩体中角闪石进行了详细的研究,总结了各期岩体中角闪石的特征。从早期到晚期,角闪石光性呈递变关系,2V由(-)76.7→(+)84.2;化学成分呈规律性变化,Si、Fe含量减少,Al、Mg、Na含量增加,矿物种属明显地呈浅闪石质角闪石→含铁韭闪石→韭闪石的变化规律,因而首次在该区确定了含铁韭闪石、韭闪石矿物的存在;红外光谱随T类阳离子Al~(Ⅳ)/Si值,C类阳离子Fe/Mg值呈规律性变化;晶胞参数也显示规律性变化,a由9.838—9.866A,b由18.047—17.980A,c由5.308—5.295A,V由910.73—906.55A~3。清楚地反映了该区角闪石各期演化上的“血缘”关系和差异。同时,探讨了各期角闪石的结晶温度(770—1114℃);成因类型为基性及超基性岩浆型,岩浆来源于上地幔;超基性岩具有地幔交代成因特征。     

Application of a cloud-texture analysis scheme to the cloud cluster structure recognition and rainfall estimation in a mesoscale rainstorm process

It is thought that satellite infrared (IR) images can aid the recognition of the structure of the cloud and aid the rainfall estimation. In this article, the authors explore the application of a classification method relevant to four texture features, viz. energy, entropy, inertial-quadrature and local calm, to the study of the structure of a cloud cluster displaying a typical meso-scale structure on infrared satellite images. The classification using the IR satellite images taken during 4–5 July 2003, a time when a meso-scale torrential rainstorm was occurring over the Yangtze River basin, illustrates that the detailed structure of the cloud cluster can be obviously seen by means of the neural network classification method relevant to textural features, and the relationship between the textural energy and rainfall indicates that the structural variation of a cloud cluster can be viewed as an exhibition of the convection intensity evolvement. These facts suggest that the scheme of following a classification method relevant to textural features applied to cloud structure studies is helpful for weather analysis and forecasting.     

渤海湾盆地石炭纪—二叠纪煤的有机组分红外光谱研究

通过对渤海湾盆地石炭纪－二叠纪煤中主要有机组分进行显微傅里叶红外分析,揭示了孢子体,角质体,树脂体及基质镜质体等有机组分化学组成,结构的特点和对油气形成贡献的差异。结果表明,角质体,树脂体和孢子体都具有富氢指数高,富氧指数低的特点,但树脂体对油气生成的贡献更大而且时间较早,孢子体较差而且时间较晚,就基质镜质体而言,晚石炭世太原组（Ｃ２ｔ）煤比早二叠世山西组（Ｐ１ｓ）煤富氢指数高,富脂链参数也大,表     

活动色球双星HR1099近红外分光光度观测

本文发表了强活动色球双星ＨＲ１０９９（＝Ｖ７１１Ｔａｕ）在１９８９年１２月特大能量白光耀发前后的近红外分光光度观测结果，给出该星从２．３－４．１μｍ首次ＣＶＦ低色散光谱，以及耀发前后的变化；计算了同期观测到的子星表面黑子的影响，给出双星黑体近似辐射能谱，并与多波段测光以及ＩＲＡＳ观测作了对比，揭示了该双星有很强的星周物质的２．３μｍ发射带和３．１μｍ波段吸收带特征，本文对可能的星周物质成分和分布亦作了初步讨论。     

New merlin observations of OH/IR stars: OH357.31-1.33 and OH0.9+1.3

We present recent radio interferometer measurements of the OH 1612 MHz maser emission from the OH/IR sources OH0.9+1.3 and OH357.31 obtained with the enhanced MERLIN. Some preliminary results are briefly discussed. These results are part of an on-going observational campaign to obtain the best radio maps of bright OH/IR stars with MERLIN, VLA and VLBA, in order to understand the nature and dynamics of their circumstellar matter and evolution.