南京冬季城、郊下垫面能量平衡特征分析   总被引：7，自引：5，他引：2  

彭江良  吴息  江志红  刘红年 《气象科学》2008,28(1):21-29

本文利用2006年2月17日-3月2日在南京市区和郊区测得的辐射、湍流通量和脉动风速资料,定量分析了城、郊不同下垫面辐射收支、热量平衡特征及各分量的变化,结果表明:(1)不同天气条件下辐射平衡特征城、郊有一定差异,在晴天时差异最大,在下雪天时差异最小,但多云时更接近各辐射分量城、郊差异的平均特征;(2)城、郊下垫面感热和潜热分布不均,尤其是潜热城、郊对比有较大差异;(3)观测期间平均波文比(Qh/Qe)市区为7.8,与荒漠干旱地区接近,郊区为1.8.  相似文献   

1994-2006年长江三角洲和东北平原酸性气体浓度变化   总被引：6，自引：0，他引：6  

徐晓斌  林伟立  颜鹏  张忠华  俞向明 《气候变化研究进展》2008,4(4):195-201

 利用长江三角洲和东北平原地区大气本底站的二氧化硫（SO2）和氮氧化物（NOx）历史资料和近期取得的观测数据,探讨两个地区人为排放对这些气候相关酸性气体的不同贡献。从两种酸性气体过去和现在的浓度水平,估算了它们在两个地区的增长率,比较了NOx与SO2比值的不同变化趋势。结果表明,早在20世纪90年代中期,长江三角洲酸性气体污染水平已经较高,其后主要是NOx浓度显著升高,从而使该地区成为硫和氮污染并重的地区;东北平原酸性气体过去浓度很低,但这些气体以很高的速率增长,虽然目前浓度水平仍然比较低,但未来形势不容乐观。  相似文献   

GPS授时服务系统在气象业务中的应用   总被引：1，自引：0，他引：1  

艾艳  王敏  武鹏  王婉  刘和平 《气象与环境科学》2008,31(4):85-87

介绍了利用GPS的时间信息组建内部局域网的授时服务系统的方法:首先通过微控制器(MCU)将GPS接收器送出的二进制信息转换成各种不同的格式输出供服务器调用,然后通过基于网络时间协议的服务器/客户端时间校对软件,实现内部局域网计算机的自动对时.此外,针对GPS失锁或出现异常不可用的情况,提出了系统应对处理方法.  相似文献   

贵州矿山地质环境恢复治理效果评估方法改进研究——以贵州省毕节市某煤矿为例          下载免费PDF全文

来瑞娟  周文喜  谢朝贵  粟永标  申鹏 《贵州地质》2024,(1):61-66

在收集矿山地质环境恢复治理相关规范和技术要求的基础上,结合矿山开采造成的地质环境问题的现状、分布,从众多常用的矿山地质环境恢复治理评价指标中,选取普适性较强的地质灾害治理效果、水环境恢复效果、景观植被恢复效果、管护措施这4个评价指标作为评价因子,从而验证上述普适性较强的评价因子可以较好的反映治理恢复效果。根据评价因子的重要性,分别赋予不同的权重,采用加权综合法进行计算,对恢复治理效果评估方法进行改进量化,综合判定地质环境恢复治理效果。本文以贵州省毕节市某煤矿为例,采用的矿山地质环境恢复治理评估方法通过验证,可以为同类型矿山开展地质环境恢复治理效果评估提供借鉴。  相似文献   

The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall     

Christian Wolf  Alfonso Aragón-Salamanca  Michael Balogh  Marco Barden  Eric F. Bell  Meghan E. Gray  Chien Y. Peng  David Bacon  Fabio D. Barazza  Asmus Böhm  John A. R. Caldwell  Anna Gallazzi  Boris Häußler  Catherine Heymans  Knud Jahnke  Shardha Jogee  Eelco van Kampen  Kyle Lane  Daniel H. McIntosh  Klaus Meisenheimer  Casey Papovich  Sebastian F. Sánchez  y Taylor  Lutz Wisotzki  Xianzhong Zheng 《Monthly notices of the Royal Astronomical Society》2009,393(4):1302-1323

We investigate the properties of optically passive spirals and dusty red galaxies in the A901/2 cluster complex at redshift ∼0.17 using rest-frame near-ultraviolet–optical spectral energy distributions, 24-μm infrared data and Hubble Space Telescope morphologies from the STAGES data set. The cluster sample is based on COMBO-17 redshifts with an rms precision of  σ _cz ≈ 2000 km s⁻¹  . We find that 'dusty red galaxies' and 'optically passive spirals' in A901/2 are largely the same phenomenon, and that they form stars at a substantial rate, which is only four times lower than that in blue spirals at fixed mass. This star formation is more obscured than in blue galaxies and its optical signatures are weak. They appear predominantly in the stellar mass range of  log  M _*/M_⊙=[10, 11]  where they constitute over half of the star-forming galaxies in the cluster; they are thus a vital ingredient for understanding the overall picture of star formation quenching in clusters. We find that the mean specific star formation rate (SFR) of star-forming galaxies in the cluster is clearly lower than in the field, in contrast to the specific SFR properties of blue galaxies alone, which appear similar in cluster and field. Such a rich red spiral population is best explained if quenching is a slow process and morphological transformation is delayed even more. At  log  M _*/M_⊙ < 10  , such galaxies are rare, suggesting that their quenching is fast and accompanied by morphological change. We note that edge-on spirals play a minor role; despite being dust reddened they form only a small fraction of spirals independent of environment.  相似文献   

The Origin of the Element Eu in Extremely Metal-poor Halo Stars     

Jun-an Dai  Qiu-he Peng 《Chinese Astronomy and Astrophysics》2009

The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied.  相似文献   

Effects of strong ground motion on the susceptibility of gully type debris flows   总被引：5，自引：0，他引：5  

Chia-Nan Liu  Jia-Jyun Dong  Yih-Ferng Peng  Hsiao-Fung Huang 《Engineering Geology》2009,104(3-4):241-253

Typhoon Herb in 1996 caused widespread debris flows in central Taiwan. The 7.3 Chi-Chi earthquake on September 21, 1999, which also took place in central Taiwan, induced many landslides in the region. These landslides turned into debris flows when Typhoon Toraji struck Taiwan in 2001. This research selects three regions which suffered a ground motion class of 5, 6, and 7 on the Richter scale during the Chi-Chi earthquake as study areas. Air photos from 1997 and 2001 of these regions are used to map the gully-type debris flows that took place after Typhoons Herb and Toraji, respectively. The gullies adjacent to the debris flow, but without a trace of debris flows, are also mapped as the non-debris flow data. The topography, hydrogeology, and rainfall factors – where debris flow occurred and in which there was no occurrence of debris flows in these gullies were retrieved from DTM, geological maps, and iso-countour maps, and of rainfall through GIS processing. These characteristic are introduced into a probabilistic neural network to build a predicting model for the probability of the occurrence of debris flows. Three series of cross analyses are conducted to compare the probability of the occurrence of debris flows of the same dataset predicted by different prediction models. The results reveal that the susceptibility of debris flows was elevated after the Chi-Chi earthquake struck. The upsurge of susceptibility was more obvious for the regions that received a higher class of ground motion.  相似文献   

内蒙古苏莫查干敖包萤石矿区流纹岩锆石SHRIMP定年及地质意义   总被引：5，自引：1，他引：4  

聂凤军  许东青  江思宏  胡朋 《地质学报》2009,83(4):496-504

内蒙古苏查（苏莫查干敖包）萤石矿区晚古生代火山沉积岩分布广泛,主要岩石类型有碳泥质板岩、结晶灰岩、凝灰岩、千枚岩、英安岩和流纹岩,其中碳泥质板岩和流纹岩为苏查特大型萤石矿床的顶和底板围岩。采用锆石SHRIMP UPb铅法分别对底板围岩中蚀变流纹岩和顶板围岩中未蚀变流纹岩样品进行了同位素年代测定,所获数据分别为276±10 Ma和271±8 Ma。蚀变和未蚀变流纹岩的形成时间均为海西晚期（早二叠世）。苏查萤石矿区早二叠世流纹岩是华北陆台与西伯利亚板块从碰撞挤压到松弛张裂转折期,酸性岩浆喷发活动的产物,其成岩物质来自壳、幔混合源。早二叠世流纹岩的出现不仅标志着苏查到西里庙地区海西期构造岩浆活动的终结,同时也为苏查特大型萤石矿床的成矿作用提供了动力、热力和物质来源。早二叠世流纹岩成岩时代的厘定不仅为阐明华北陆台北缘西段构造演化历史提供了科学依据,而且对于查明流纹岩的原岩性质和圈定新的萤石矿床找矿靶区也具有重要意义。  相似文献   

四川犍为晚侏罗世一新的肉食龙类     

李飞  彭光照  叶勇  江山  黄大喜 《地质学报》2009,83(9):1203-1214

记述了四川盆地西南部晚侏罗世上沙溪庙组顶部的中国盗龙型肉食龙类化石材料,并依此建立一新属新种——犍为乐山龙 (Leshansaurus qianweiensis gen. et sp. nov.)。它以上枕骨中嵴呈尖峰状,额骨最大长度与最大宽度之比约2.86,基蝶骨之基翼骨突细长,环椎间椎体马蹄形,背椎横突相当细长,背椎和荐椎神经棘非常薄,荐椎椎体具有明显的腹嵴,肠骨内侧髋臼缘存在一明显的嵴等特征区别于其他肉食龙类。犍为乐山龙是目前所知四川盆地产出层位最高的肉食龙材料,它的发现扩大了肉食龙类的时代分布和地理分布,对探讨肉食龙的演化具有比较重要的意义。  相似文献   

Distribution and significance of novel low molecular weight sterenes in an immature evaporitic sediment from the Jinxian Sag,North China     

Hong Lu  Tengshui Chen  Kliti Grice  Paul Greenwood  Ping’an Peng  Guoying Sheng 《Organic Geochemistry》2009,40(8):902-911

An unusual series of C₂₂–C₂₇ monounsaturated sterenes and C₂₄–C₃₀ tetracyclic terpanes (17,21-secohopanes) were detected in relatively high concentrations in an immature evaporitic marl sediment of the Jinxian Sag, Bohai Bay Basin, North China. The site of unsaturation in these novel sterenes is assigned tentatively to the D ring on the basis of mass spectral interpretation, which also distinguishes them from reported unsaturated sterenes. Other hydrocarbon biomarker or stable isotope characteristics are indicative of microbial (e.g. methyl hopanes), phytoplankton or higher plant (depleted δ¹³C values of isoprenoids and hopanes) inputs and an anoxic carbonate depositional environment (hexacyclic hopanes; tetracyclic terpanes). The hydrocarbon composition showed no obvious biodegradation and the relatively high concentration of unsaturated terpenoids (e.g. gammacerene) and low values of other established maturity parameters (T_s/T_m = 0.23; R_o = 0.44%; T_max = 417 °C), are consistent with sediments of low maturity. The novel, low molecular weight sterenes and the tetracyclic terpanes may be early diagenetic products of microbial sources in a carbonate environment.  相似文献