紫外线指数及其预报技术介绍     

邓英姿  董蕙青  覃天信  廖俊华 《气象研究与应用》2000,21(3):38-40

对南宁市近7a来的紫外线辐射强度与太阳辐射总量、总云量、低云量的关系进行统计分析,建立了紫外线指数与太阳辐射总量之间的气候平均值对应关系,在此基础上,制作南宁市未来24h的紫外线指数预报,并根据预报结果提醒人们采取相应的防护措施,服务于社会公众.  相似文献   

Variability of heterotrophic activity in Mediterranean stream biofilms: A multivariate analysis of physical-chemical and biological factors     

Anna M. Romaní  Sergi Sabater 《Aquatic Sciences - Research Across Boundaries》2000,62(3):205-215

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四川稀土矿（氟碳铈矿）稀土总量的测定方法   总被引：1，自引：0，他引：1  

毛英 《四川地质学报》2000,20(1):79-80

氟碳铈矿矿样经高氟酸分解、脱硅后,稀土元素以氢氧化物和草酸盐形成进行沉淀与干扰元素分离,氢氧化物沉淀使稀土与钙、镁分离,草酸盐沉淀,使稀土与铁、铝、锆、钛等元素分离。适应矿石稀土含量１％～７４％的含量测定。该方法用于氟硕铈矿稀土总量的测定,方法简便、快速、准确。  相似文献   

The most metal-poor galaxies     

D. Kunth  G. Östlin 《Astronomy and Astrophysics Review》2000,10(1-2):1-79

Summary. Metallicity is a key parameter that controls many aspects in the formation and evolution of stars and galaxies. In this review we focus on the metal deficient galaxies, in particular the most metal-poor ones, because they play a crucial r?le in the cosmic scenery. We first set the stage by discussing the difficult problem of defining a global metallicity and how this quantity can be measured for a given galaxy. The mechanisms that control the metallicity in a galaxy are reviewed in detail and involve many aspects of modern astrophysics: galaxy formation and evolution, massive star formation, stellar winds, chemical yields, outflows and inflows etc. Because metallicity roughly scales as the galactic mass, it is among the dwarfs that the most metal-poor galaxies are found. The core of our paper reviews the considerable progress made in our understanding of the properties and the physical processes that are at work in these objects. The question on how they are related and may evolve from one class of objects to another is discussed. While discussing metal-poor galaxies in general, we present a more detailed discussion of a few very metal-poor blue compact dwarf galaxies like IZw18. Although most of what is known relates to our local universe, we show that it pertains to our quest for primeval galaxies and is connected to the question of the origin of structure in the universe. We discuss what do QSO absorption lines and known distant galaxies tell us already? We illustrate the importance of star-forming metal-poor galaxies for the determination of the primordial helium abundance, their use as distance indicator and discuss the possibility to detect nearly metal-free galaxies at high redshift from Ly emission. Received 19 August 1999 / Published online: 15 February 2000  相似文献   

A brief introduction to recent applications of several sediment-analysis techniques in palaeolimnological studies-dry bulk density and water content, mineral magnetism, carbonate content, and content of total organic carbon, nitrogen content and c     

WANG Hong-ya 《地理学报(英文版)》2000,(1)

ChalacteriStics of lacustrine sediments are often capable of ~ring the hydrological regales of the lakeand its environment and human achvihes in itS catclunent during the sedimentahon of these sedimentS.Therefore, by identifying these characteristics of sedimentS, it is likely to postUlate the physicalconditions in and around the lake during geological periods. Such reconstrUction of palaeoenvironmentshas become an increasingly important branch of ear sciences as there has been an expanded n…  相似文献   

The star formation histories of two northern LMC fields     

A. E. Dolphin 《Monthly notices of the Royal Astronomical Society》2000,313(2):281-290

Ground-based UBV photometry of two fields in the northern disc of the Large Magellanic Cloud (LMC) is presented. A distance modulus of ( m − M )₀=18.41±0.04 and an extinction of A _V =0.30±0.05 have been calculated for these fields. The measurable star formation history of the LMC began no more than 12 Gyr ago with a strong star‐forming episode with [Fe/H]=−1.63±0.10 that accounted for approximately half (by mass) of the total star formation of the LMC in the first 3 Gyr. The data do not give accurate star formation rates during intermediate ages, but there appears to have been a recent increase in the star formation rate in these fields, beginning approximately 2.5 Gyr ago, with the current metallicity in the region being [Fe/H]=−0.38±0.10. The two fields have had very similar star formation rates until 200 Myr ago, at which point one shows a large increase.  相似文献   

Detection of the old stellar component of the major Galactic bar     

P. L. Hammersley  F. Garzón  T. J. Mahoney  M. López-Corredoira  M. A. P. Torres 《Monthly notices of the Royal Astronomical Society》2000,317(3):L45-L49

We present near-infrared colour–magnitude diagrams and star counts for a number of regions along the Galactic plane. It is shown that along the l =27°, b =0° line of sight there is a feature at 5.7±0.7 kpc with a density of stars at least a factor of 2 and probably more than a factor of 5 times that of the disc at the same position. This feature forms a distinct clump on an H versus J − H diagram and is seen at all longitudes from the bulge to about l =28°, but at no longitude greater than this. The distance to the feature at l =20° is about 0.5 kpc further than at l =27°, and by l =10° it has merged with, or has become, the bulge. Given that at l =27° and l =21° there is also a clustering of very young stars, the only component that can reasonably explain what is seen is a bar with half-length of around 4 kpc and a position angle of about 43°±7°.  相似文献   

近千年来内蒙古岱海气候环境演变的湖泊沉积记录   总被引：46，自引：11，他引：35  

曹建廷  王苏民  沈吉  张振克 《地理科学》2000,20(5):391-396

内陆封闭湖泊是气候环境变化的敏感指示计。通过对内蒙古岱海湖泊岩芯的有机碳同位素、总有机碳、碳酸盐含量和磁化率等多环境指标的综合分析,结合Ｐｂ－２１０测定的沉积速率,讨论了岱海地区近千年来的气候环境演化过程。揭示了本区现代小冰期的前期冷湿,后期冷干的气候特征。记录的最后两次冷期与根据冰芯、树轮、历史文献重建的１０年平均温度推得的１４５０’ｓ～１５１０’ｓ、１７９０’ｓ～１８９０’ｓ两次冷期极相吻合。  相似文献   

三峡库区紫色土微量元素含量的变化   总被引：3，自引：3，他引：0  

董杰  杨达源  周彬  陈可锋  胥勤勉 《地理科学》2006,26(5):592-596

以三峡库区典型坡面紫色土为例,对土壤中微量元素的含量及其在不同坡度、不同利用方式下的变化进行初步研究。结果表明,库区紫色土中Fe、Mn、Ni、Zr、Sr和Ti的含量相对较多,Mo的含量较为丰富,Zn和Pb的含量相对较低。Pb、Cu和Co的含量在一定坡度范围内随坡地坡度的增大而减少,Zr和Cr的含量则增加。紫色土中Cu、Pb、Co、Ti、Zr、Ni、Cr、Sr等微量元素的含量随坡度的变化具有一定的相关性。耕作土和非耕作土中微量元素含量差异明显,人为活动是引起库区紫色土微量元素含量变化的主要因素。  相似文献   

利用地震资料反演地层的碳酸盐含量   总被引：1，自引：0，他引：1  

熊艳  钟广法  李前裕  吴能友  李学杰  马在田 《地球科学》2006,31(6):851-856

基于碳酸盐含量与地层速度、密度之间的关系, 在井资料约束下, 使用人工神经网络方法反演高分辨率地震资料所反映的地层碳酸盐含量, 并应用于南海北部陆坡ODP184航次1146和1148孔区, 取得较好效果.方法的关键是从井旁地震道中提取多种属性, 利用逐步回归法, 确定6种与碳酸盐含量相关性最好的地震属性, 分别是平均频率、道积分绝对振幅、主频、时间、道微分瞬时振幅和瞬时频率, 然后进行地层碳酸盐含量反演.反演结果相对于岩心分析的碳酸盐含量的误差大多在±5%之内, 较为精确地揭示了地震地层剖面上碳酸盐含量的分布.   相似文献