河南小秦岭大湖金－钼矿床地球化学及其矿床成因

秦岭造山带是华北与扬子两大古板块的接合带，在空间上，自北而南，秦岭造山带可分为华北板块南缘（华熊地块）、北秦岭造山带、南秦岭造山带和扬子板块北缘等4个构造单元。小秦岭金矿田位于华熊地块北缘，是国内外学者共识的造山型金矿田，河南灵宝大湖金－钼矿床位于小秦岭金矿田，属断控脉状矿床。大湖金－钼矿床最先正是以金矿床进行勘查的，其黄金储量28t，平均品位8.7g/t。随着开采深度的加大，部分含金石英脉向深部转变为辉钼矿－石英脉，目前探明钼资源量已达中型规模。 本论文主要从区域地质背景、矿床地质特征、元素地球化学、同位素地球化学、流体包裹体地球化学、矿床年代学及成矿机理等角度对大湖金－钼矿床进行了较为系统的研究，主要获得如下认识： 成矿过程经历3个阶段：早阶段为黄铁矿-石英脉，遭受变形、破碎，应形成于挤压或压剪过程；中阶段为细粒的辉钼矿-黄铁矿-石英网脉，贯入到早阶段黄铁矿或石英矿物的裂隙（可呈共轭状），应形成于剪切环境；晚阶段石英-碳酸盐细脉具梳状构造，充填于张性或张扭性裂隙。 大湖金-钼矿床的金属硫化物ISr=0.70470-0.71312，平均0.70854；(143Nd/144Nd)i=0.51143-0.51215，平均0.51162；(206Pb/204Pb)i=17.033-17.285，(207Pb/204Pb)i=15.358-15.438，(208Pb/204Pb)i = 37.307-37.582。其围岩太华群样品平均值ISr＝0.72294，(143Nd/144Nd)i=0.51107，(206Pb/204Pb)i=17.127-18.392，(207Pb/204Pb)i =15.416-15.604，(208Pb/204Pb)i=37.498-37.814，它们的平均值分别是17.547，15.470，37.616。通过金属硫化物及围岩太华群的对比，可以看出，成矿物质具有太华群和深部地幔混合的特征。 通过对不同阶段的含矿石英脉中的流体包裹体特征研究表明，早阶段只发育CO2-H2O型流体包裹体；中阶段流体包裹体类型复杂，有纯CO2型、CO2-H2O型、H2O-NaCl型和含子晶包裹体，指示流体沸腾作用强烈；而晚阶段只发育水溶液包裹体。早、中、晚3个阶段的流体包裹体均一温度分别集中在400-500℃、290-470℃、220-260℃；估计的早、中阶段流体的最低捕获压力分别为138-331MPa和78-237MPa，对应于成矿深度分别为13.8-11.0km和7.8-8.0km。早、中阶段的压力反应出静岩压力到静水压力的转变。成矿温度和压力明显高于浅部含金石英脉的成矿温度120-310℃，成矿压力100-150MPa。与野外观察到的“上金下钼”的空间关系一致。 大湖金－钼矿床辉钼矿－石英脉Re-Os同位素模式年龄较集中，介于215.4±5.4－255.6±9.6Ma，Re-0s等时线年龄为218±41Ma(MSWD=38，2σ误差)，表明大湖金－钼矿的辉矿化形成于印支期。 三叠纪末，随着古秦岭洋的逐渐封闭，处在弧后转换带的深部岩石在挤压作用下发生变质脱水而形成初始成矿流体，成矿流体沿断裂带（韧性剪切带）向上迁移而引起大湖钼矿床成矿系统的发育。随着区域构造环境由挤压转为伸展，区域的变质脱水更强，形成大量成矿流体，变质流体上侵为浅层流体循环提供了的热能，而浅层构造也因减压扩容而为流体循环提供了通道，这无疑有利于浅层流体循环和混入成矿系统。同时，增温和减压也有利于成矿流体发生沸腾。因此，充足的流体、热以及强烈的流体沸腾等，势必导致发生最为强烈的成矿物质快速沉淀作用。随着挤压作用的减弱，伸展作用的增强，区域热异常消失，地壳深部组分发生亏损，流体以浅源大气降水占主导，成矿作用迅速衰竭，形成石英-碳酸盐网脉，对成矿作用贡献减弱。总之，通过对大湖金钼矿床研究表明，大湖金钼矿床形成于由挤压转向伸展的构造背景，这与矿床地质的特征一致。

贵州凉风洞石笋的古气侯记录与古生态环境意义

自20世纪60年代以来，探索全球性气候变化规律和环境变迁史的研究工作在世界各国广泛开展。大规模的深海岩芯的研究、中国北方黄土的系统研究、大型湖泊沉积岩芯的研究及对树木年轮、泥炭、珊瑚、冰芯等“自然环境历史档案”开展的研究工作，都为重建古气候和古生态环境提供了大量的资料。洞穴化学沉积物（石笋）由于其特有的微层结构及其内的稳定氧、碳同位素和微量元素所蕴含的古气候与古生态环境信息，并且具有分布广、时间长、信息保存完整等特点，因此，它是研究地球环境变化很好的自然环境历史档案。本论文通过对凉风洞洞穴体系的综合研究和对凉风洞石笋（微层）生长特征及石笋的碳、氧稳定同位素组成的研究，系统探讨了贵州凉风洞石笋的古气候记录和古生态环境意义，得出以下主要结论：1，地表植被的类型及生物量等信息可综合反映于洞穴体系的不同组．分（气样、土样、水样）中。而洞穴的水动力条件也能很好的被洞穴滴水中所含微量（常量）元素记录。根据分析，洞穴综合体系对外界气候与生态环境的响应关系存在一定规律性。通过对比说明，我们所选的凉风洞基岩的溶蚀和缓冲对水体中的信息影响不大，即洞穴滴水较好的继承了土壤水所携带的地表气候与生态环境信息，是理想的研究对象。2．凉风洞石笋具有多个沉积旋回，不同沉积旋回的纹层组合及纹层结构存在一定的差异，指示不同的沉积环境。根据年龄数据判断，旋回①至旋回⑧之间年龄跨度为1570-8000 aBP，以呈缓平顶（柱）对称叠复状的沉积形态组合为主，示洞顶滴水量较大，滴水点相对稳定，且均匀，与全新世较为稳定的气候与环境变化的主旋律相一致。旋回⑧以下至底部石葡萄状沉积物之上部分之间年龄跨度为8000-14220 aBP，期间经历末次冰期晚期向全新世大暖期过渡，受诸如新仙女木事件（Younger Dryas）等的影响，气候变化幅度大，且经历多次反复，石笋生长的沉积学特征表现为斜锥（柱）、尖顶锥不对称叠复纹层组合，示洞顶滴水水量较小但变化较大，且洞穴滴水不稳（固）定。与此时间段内不稳定的气候与环境变化的主旋律也相一致。3．凉风洞石笋上段微层具有典型南方石笋微层发育的特性：微层发育较差，层面多弯曲，层间界面模糊等。下段因为沉积间断较多、风化层面厚及受到若干时段内碳酸钙重结晶而导致晶体穿插层位生长的影响，尽管在某些层位有微层发育，但无法对石笋微层作连续观察记录。根据高精度的石笋TIMS、ICP-MS测年数据和在显微镜下所数石笋微层数量的对比，扣除若干个沉积间断及风化层导致的微层缺失，以及显微镜下肉眼对细小微层计数的误差，我们认为，凉风洞石笋微层是年生长层的可能性较大。4，由于部分测年数据仍在测试中，目前无法精确控制石笋中沉积间断的存在导致的信息缺失，因此，我们仅仅根据部分石笋测年数据，建立了凉风洞石笋在不同时段的生长速率。全新世以来石笋的生长速率在22μm／yr-51μm／yr之间，明显高于末次冰期晚期向全新世过渡这一时间段内的石笋生长速率（16μm／yr）。这些数据间接印证了石笋生长响应于外界气候，尤其是降雨的变化。5．通过对洞穴体系的综合分析对比，我们判断凉风洞洞穴综合体系相对完整，洞穴化学沉积物的6先值较为直接的响应了土壤c压的61t值变化，即反映了地表的植被（c3植物和c；植物）的组成状况。贵州地区降雨80％集中在5-10月份，在此期间，基本受西南季风和东亚季风所控制。西南季风盛行时贵州各地的降雨频繁，是一年中雨量最集中的时期，在东亚季风影响时期，贵州多晴少雨，往往形成干早的天气。又西南季风控制区大气降雨创的值的加权平均值明显低于东亚季风控制区大气降雨δ18O值的加权平均值。因此，贵州地区年均降雨量和年均降雨δ18O值主要取决于西南（印度洋）季风的强弱：西南季风加强，降雨量增加，年均降雨剐、值偏负；西南季风减弱，降雨量减少，年均降雨δ18O值偏正。洞穴滴水的6旧O值变化基本继承了大气降水的别勿值变化。因此，对地处我国西南地区贵州南部的凉风洞，源于洞穴滴水的凉风洞石笋的别勺值变化直接响应了外界的大气降雨量的变化和西南季风与东亚季风相互的强弱交替。6．对凉风洞石笋碳、氧同位素组成的时间序列曲线作20点移动平均，发现，特别是进入全新世后，石笋的引3c值和扩、值几乎具有完全一致的同步变化，只是在变化幅度上在某些时段存在差异。说明在凉风洞石笋反映的14220-1570 aBP时间段内，尤其是10500-1570 aBP期间，本区域气候具有雨热（或干冷）同期的气候特征：在气温较高时间段，西南季风增强，气候湿润多雨，更有利于地表。植物的生长。气温降低时，随着东亚季风增强，西南季风减弱，气候干旱少雨，地表C；植物的生长占有一定的比例。据此重建和恢复了本地区14220-1570 aBP期间的古气候和古生态环境：（1）．14220-10500aBP，处于末次冰期晚期，气温较低。凉风洞石笋此时段的司、值都大于-9.8‰，最小值为-9.31‰，最大值达-7.290‰，平均值为-8.552‰。说明凉风洞洞穴地表的生长植被。植物占有一定的组分，石笋的δ18C值受C3植物和C4植物的共同影响。此时段内石笋6、值也存在一定的波动（-5.651‰－6.942‰），考虑到末次冰期晚期先全新世过渡期间气温变幅较大，O'Neil等（1969）所建立的氧同位素平衡分馏方程中的温度变化已不能忽略，并且大气降雨的温度效应作用也比较明显，因此我们对此时段的季风和大气降雨量的变化不作讨论。（2）. 10500-9300 aBP，新仙女木事件结束，进入全新世，气温逐渐回升。凉风洞石笋此时段的扩3c值大都小于-9.8‰，最小值为-10.377‰，最大值为-9.267‰，平均值为-9.910‰。凉风洞洞穴地表植被已逐渐由C3植物占主导。此时段石笋δ18C值明显卜降，最小值为-7.420‰，最大值为-6.077‰，平均值为-6.854‰。反映在全新世早期夏季风盛行，降雨量较大，西南季风对本地区全年降雨贡献率大。（3）．9300-8300 aBP，经历一段明显温度波动变化。仟3c值在-9.8‰上下波动，最小值为-10.155‰，最大值为-9.096‰，平均值为-9.712‰。凉风洞洞穴地表植被C4植物所占比例存在反复。此时段石笋岁a0值变化幅度不是很大，最小值为-6.796‰，最大值为-6.260‰，平均值为-6.490‰。受冬季风影响，夏季风有一定的减弱，总体降雨量一般，东亚季风对本地区全年降雨贡献率比全新世初期有所增大。（4）．8300-3l000BP，俗称全新世大暖期，此时段全球气温明显回升，石笋δ18C值总体逐渐降低，最小值为-n．926编，平均值为-10.496‰。凉风洞洞穴地表植被基本由C3植物所控制。但在扩飞值总体逐渐降低的趋势一F，也存在若干扩3c值明显增大时段，如7700-6700 aBP时段，61七值最大值达-8.110‰，地表C4植物所占比例已不能忽略。此时段石笋6150值变化幅度较大，最小值为-7.373‰，最大值为-5.047‰，平均值为-6.261‰。反映在全新世大暖期的大背景下西南季风和东亚季风的交替以及大气降雨量的变化存在较大的波动，说明了季风气候的不稳定性。（5）．3100-1570 aBP，在3100aBP前后，凉风洞石笋的δ18C值和δ18O值均急剧上升，标志进入晚全新世。此时段气温变幅很大，δ18C值总体虽然仍偏低，平均值为-10.275‰，但刻畜介于-6.495-12.097‰之间；δ18C值平均值为-6.184‰，变幅介于-4.677-8.65‰之间，均超过以往任何时段。此时段凉风洞洞穴地表植被基本上仍然由C。植物所控制，始于3100 aBP的急速降温事件使得在全新世晚期开始时段C4植物所占比例有一定的上升。此时段内西南季风和东亚季风反复多次交替，大气降雨量存在较大幅度的变化，说明了季风气候在此时段的很不稳定性。对于169于巧70 oBP百年时间段内石笋的δ18C值和司、值巨大幅度的急剧升高，有待进一步研究，也不排除石笋表层长期裸露受外界污染所致。

Embrapa Trigo - 31 anos.

Slide 1: Embrapa Trigo - 31 anos. Slide 2: Localização. Slide 3: Histórico. Slide 4: Missão. Slide 5: Infra-estrutura. Slide 6: Recursos Humanos. Slide 7: Missão nacional. Slide 8: Apoio regional. Slide 9: Áreas de pesquisa. Slide 10: Principais resultados. Slide 11: Cultivares de trigo. Slide 12: Cultivares. Slide 13: Cultivares. Slide 14: Sistema plantio direto. Slide 15: Controle biológico de pulgões. Slide 16: Máquinas e equipamentos para o sistema plantio direto. Slide 17: Rotação de culturas e integração lavoura-pecuária. Slide 18: Qualidade tecnológica do trigo. Slide 19: Zoneamento agroclimático. Slide 20: Manejo integrado de pragas em grãos armazenados. Slide 21: Obrigado.

Canada's missionary congress; addresses delivered at the Canadian National Missionary Congress, held in Toronto, March 31 to April 4, 1909, with reports of committees.

http://www.archive.org/details/canadasmission00unknuoft/

Permanent Genetic Resources added to Molecular Ecology Resources Database 1 December 2009-31 January 2010

This article documents the addition of 220 microsatellite marker loci to the Molecular Ecology Resources Database. Loci were developed for the following species: Allanblackia floribunda, Amblyraja radiata, Bactrocera cucurbitae, Brachycaudus helichrysi, Calopogonium mucunoides, Dissodactylus primitivus, Elodea canadensis, Ephydatia fluviatilis, Galapaganus howdenae howdenae, Hoplostethus atlanticus, Ischnura elegans, Larimichthys polyactis, Opheodrys vernalis, Pelteobagrus fulvidraco, Phragmidium violaceum, Pistacia vera, and Thunnus thynnus. These loci were cross-tested on the following species: Allanblackia gabonensis, Allanblackia stanerana, Neoceratitis cyanescens, Dacus ciliatus, Dacus demmerezi, Bactrocera zonata, Ceratitis capitata, Ceratitis rosa, Ceratits catoirii, Dacus punctatifrons, Ephydatia mülleri, Spongilla lacustris, Geodia cydonium, Axinella sp. Ischnura graellsii, Ischnura ramburii, Ischnura pumilio, Pistacia integerrima and Pistacia terebinthus. © 2010 Blackwell Publishing Ltd.

Nomenclature and syntaxonomic notes on some high-rank syntaxa of the European grassland vegetation

We present descriptions of a new order (Ranunculo cortusifolii-Geranietalia reuteri and of a new alliance (Stachyo lusitanicae-Cheirolophion sempervirentis) for the herbaceous fringe communities of Macaronesia and of the southwestern Iberian Peninsula, respectively. A new alliance, the Polygalo mediterraneae-Bromion erecti (mesophilous post-cultural grasslands), was introduced for the Peninsular Italy. We further validate and typify the Armerietalia rumelicae (perennial grasslands supported by nutrient-poor on siliceous bedrocks at altitudes characterized by the submediterranean climate of central-southern Balkan Peninsula), the Securigero-Dasypyrion villosae (lawn and fallow-land tall-grass annual vegetation of Italy), and the Cirsio vallis-demoni-Nardion (acidophilous grasslands on siliceous substrates of the Southern Italy). Nomenclatural issues (validity, legitimacy, synonymy, formal corrections) have been discussed and clarified for the following names: Brachypodio-Brometalia, Bromo pannonici-Festucion csikhegyensis, Corynephoro-Plantaginion radicatae, Heleochloion, Hieracio-Plantaginion radicatae, Nardetea strictae, Nardetalia strictae, Nardo-Callunetea, Nardo-Galion saxatilis, Oligo-Bromion, Paspalo-Heleochloetalia, Plantagini-Corynephorion and Scorzoneret alia villosae. 

Bolsa Familia Program and school enrolment: An analysis of the 2010 Brazilian demographic census

The Bolsa Família Program goal is to promote social development and poverty reduction, through the direct transfer of conditional cash, in association with other social programs. This study aims to analyze whether Bolsa Família had an association with children’s school attendance, which is one of the educational conditions of the program. Our main hypothesis is that children living in households receiving Bolsa Família had greater chances of attending school. Data from the Ministry of Social Development and Combating Famine indicated that children living in households with Bolsa Família had greater school enrolment levels. By using data from the 2010 Demographic Census, collected by the Brazilian Institute of Geography and Statistics (IBGE), some descriptive analyzes and binary logistic regression models were performed for different thresholds of household per capita income. These estimates were made by comparing children who lived in households receiving Bolsa Família to those children not receiving the program. We took into consideration characteristics about the household, mothers, and children. The results were clustered by the municipality of residence of the child. In all income thresholds, children benefi ting from Bolsa Família were more likely to be enrolled in school, compared to children not receiving the benefi t.

Chemical composition of B-type supergiants in the OB 8, OB 10, OB 48, OB 78 associations of M 31

Absolute and differential chemical abundances are presented for the largest group of massive stars in M31 studied to date. These results were derived from intermediate resolution spectra of seven B-type supergiants, lying within four OB associations covering a galactocentric distance of 5-12 kpc. The results are mainly based on an LTE analysis, and we additionally present a full non-LTE, unified model atmosphere analysis of one star (OB 78-277) to demonstrate the reliability of the differential LTE technique. A comparison of the stellar oxygen abundance with that of previous nebular results shows that there is an off set of between similar to0.15-0.4 dex between the two methods which is critically dependent on the empirical calibration adopted for the R 23 parameter with [O/H]. However within the typical errors of the stellar and nebular analyses (and given the strength of dependence of the nebular results on the calibration used) the oxygen abundances determined in each method are fairly consistent. We determine the radial oxygen abundance gradient from these stars, and do not detect any systematic gradient across this galactocentric range. We find that the inner regions of M31 are not, as previously thought, very "metal rich". Our abundances of C, N, O, Mg, Si, Al, S and Fe in the M31 supergiants are very similar to those of massive stars in the solar neighbourhood.