Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares

We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%.     

Infrared spectral evolution of carbon stars

We collected almost all Highly Processed Data Products(HPDP)of ISO SWS01 spectra for the Galactic visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich proto-planetary nebulae(PPNs).Those infrared spectra are primarily analyzed and discussed.It is shown that either spectral shapes/peaks,or main molecular/dust features are evidenced to change in the sequence of visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich PPNs.Statistically,in this sequence,continua are gradually changed from blue to red and locations of spectral peaks of continua are also gradually changed from short wavelengths to long wavelengths.In addition,in this sequence,intensifies of main molecular/dust features are also gradually changed from prominent in the short wavelengths to prominent in the long wavelengths.Furthermore,from 2MASS and IRAS photometric data,the sequence is also proved.Results in this paper strongly support the previous suggestion for the evolution sequence of carbon-rich objects in our Galaxy,that is the sequence of visual carbon stars→infrared carbon stars→extreme carbon stars→carbon-rich PPNs.     

Primordial non-Gaussianity from LAMOST surveys

The primordial non-Gaussianity (PNG) in the matter density perturbation is a very powerful probe of the physics of the very early Universe. The local PNG can induce a distinct scale-dependent bias on the large scale structure distribution of galaxies and quasars, which could be used for constraining it. We study the detection limits of PNG from the surveys of the LAMOST telescope. The cases of the main galaxy survey, the luminous red galaxy (LRG) survey, and the quasar survey of dif- ferent magnitude limits...     

法国高层大气所空间综合孔径项目研究进展

概述了法国高层大气所空间综合孔径项目背景、科学目标以及有效载荷,介绍了该项目演示系统的基本工作原理,探讨了该演示系统的望远子系统、指向子系统、共相子系统和成像子系统,并分别给出了该演示系统在非共相控制和共相控制情况下对半导体激光器和白光点光源的成像结果,实验结果表明演示系统不同独立望远镜之间已经基本实现了共相成像。最后对该演示系统进行了总结,并指出该系统可以进一步优化之处。该演示系统对我国综合孔径成像实验研究具有一定的借鉴意义。     

用于测量圆顶视宁度的微温脉动仪的研制

为评价云南天文台丽江2.4m望远镜的圆顶视宁度,研制了一种能测量温度、气压和微温脉动的仪器。在天文圆顶附近,望远镜前方光路上,放置几组微温传感器,可以测得圆顶附近影响天文观测的湍流强度的分布情况。介绍了这套仪器的基本原理,电路设计,程序设计,实验定标以及一个简单的测试。     

Geological Evolution of Longhushan World Geopark in Relation to Global Tectonics

The South China fold belt has experienced a complex series of tectonic events that span 1.0 billion years of earth history. Longhushan (龙虎山) World Geopark is located on the Proterozoic suture between the Yangtze craton and Cathyasia block and highlights the long history of this belt. Collision of the Cathyasia and Yangtze cratons 1.0 billion years ago was associated with the formation of the Rodinian supercontinent where most of the planet's landmasses were amalgamated into one block. Jurassic through Early...     

塔里木盆地寒武系层状硅质岩与硅化岩的元素、δ30Si、δ18O地球化学研究

塔里木盆地寒武系发育层状硅质岩和硅化岩,层状硅质岩主要发育于塔东下寒武统深水沉积相区;硅化岩发育于塔东上寒武统斜坡沉积区与西部台地区寒武系白云岩中。根据显微结构特征,可将硅化岩分为放射状硅化岩与交代残余结构硅化岩两种。分析结果表明,层状硅质岩在Al—Fe-Mn三元图中位于正常海水沉积硅质岩区内,在微量元素平均地壳标准化图解上显示平缓右倾的特征;层状硅质岩Si同位素组成护。δ30Si为0．99‰～1．4‰,O同位素组成δ18O为21．4‰～24．4‰,与沉积型硅质岩相吻合,指示了正常海水沉积成因。硅化岩区别于层状硅质岩的典型特征是具有高U异常的特征;罗西斜坡放射状硅化岩具有较高的微量元素和稀土元素含量（∑REE为18．8～96．9μg／g）与较低的Si、O同位素值（δ18O和δ30Si值分别为15．8‰和1．7‰）;西部台地区交代残余结构硅化岩具有较低微量元素和稀土元素含量（∑REE为0．58～2．61μg／g）与较高的δ30Si（1．0‰～3．8‰）、δ18O（21．6‰～27．0‰）值特征。盆地东西部硅化岩的地球化学差异可能与硅化流体的温度差异有关,罗西斜坡放射状硅化岩硅化温度相对更高;另一方面,硅化过程对h430SiO4选择性较高,因而形成的交代石英具有较高的铲勘值。根据古城4井硅化岩包裹体均一温度与交代石英的O同位素值计算得到交代流体的δ18O值为9．1‰,该值与酸性岩浆水的δ18O值相似,指示了硅化流体可能来自于岩浆或变质水;以δ18O值（9．1‰）作为西部台地区硅化流体的O同位素值,计算得到西部台地区硅化岩硅化流体温度为101．3～158．5℃。根据石英O同位素温度计计算的硅化流体温度呈东高西低的趋势,指示了硅化流体可能来自台地东部。     

Techniques and methods of arsenic contaminated groundwater exploration in the Hetao plain of Inner Mongolia,China

1990年报道了在中国内蒙古河套平原由于饮用污染的地下水而患砷中毒的病例.估计目前内蒙受到砷中毒影响的居民已超过41万人.从1997年至2004年,在长达8年的时间里,我们进行了水文地质调查、地质调查和医学调查,并装置了管道输送的供水系统.这些调查揭示了河套平原地下水受砷污染的机理:由于被吸收的砷释放进入地下水,蓄水层中不断加强的还原环境造成铁氢氧化物的溶解.为了防止砷中毒病人数量的进一步增加,停止饮用污染过的水和供应安全的饮用水是重要的.我们需要根据当地的地质和水文地质条件来了解砷污染的机理.     

海底扩张的潮汐模式

2000年6月底，东京以南的伊豆岛开始发生火山与地震活动。此后，在伊豆岛观测到异常的地壳变形，8月底，火山与地震活动达到高潮。对潮汐与火山和地震活动的关系进行了分析，认为：地壳变形是由伊豆岛的岩脉侵入引起的，并且与强潮汐天文条件相对应。根据观测和计算数据提出了海底扩张的潮汐模式。     

Connections Between Different Types of El Nio and Southern/Northern Oscillation

It has long been acknowledged that there are two types of El Nio events, i.e., the eastern Pacific El Nio (EE) and the central Pacific El Nio (CE), according to the initial position of the anomalous warm water and its propagation direction. In this paper, the oceanic and atmospheric evolutions and the possible mechanisms of the two types of El Nio events were examined. It is found that all the El Nio events, CE or EE, could be attributed to the joint impacts of the eastward advection of warm water from...