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371.
Jian-Ning Fu Chao Zhang Kanokwan Marak Chayan Boonyarak Pongsak Khokhuntod Shi-Yang Jiang 《中国天文和天体物理学报》2008,8(2):237-244
New time-series photometric observations of BL Cam in the V band and white light were made during 2005 to 2007 at the Xinglong Station of China. The frequency analysis confirms two closely separated frequencies, 25.181 d-1 and 25.571 d-1, but the frequency of 31-32 d-1 reported in the literature was not detected in the new data. New times of maximum light were determined from both our light curves and those available on Internet, allowing a more comprehensive study of the O - C diagram, together with the times of maximum light in the literature. A new interpretation, including the period increasing before 1988 and decreasing since 1992 of BL Cam and the light-time effect in a binary system, looks plausible. 相似文献
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为了研究西藏纳如松多矿集区的电性结构特征和对成矿作用的约束,对覆盖矿集区的大地电磁测深数据进行全面的数据处理分析,得到了可靠的二维电性结构模型.研究结果表明,分别在深度为40~50 km,20~30 km和10 km处见高导体,推测这些高导体可能为部分熔融和水流体共同所致.由于纳如松多矿集区内矿床为岩浆-热液型,深部岩浆的上涌在成矿作用中起到关键作用,所以壳内高导体可能为与成矿有关岩浆房的电性痕迹,将这些高导体连起来可能代表着深部热液向上运移的古通道.电性结构主要体现了壳内高导体与区域成矿动力作用的关系,向上运移的富矿岩浆也可能通过局部的隐伏构造运移到Pb-Zn和Fe-Cu矿床的位置,再演化形成矿体. 相似文献
374.
为探究成岩作用过程中所形成的次生黏土矿物对储层物性的影响,借助偏光显微镜及扫描电镜的镜下分析,并结合储层物性等数据,对渤中凹陷附近沙垒田凸起东南部CFD18-2油田东三段高岭石的特征、类型、成因及其对储层物性的影响进行了研究。研究结果表明:1)研究区高岭石为有机酸溶蚀长石形成的自生高岭石,呈现典型的"手风琴状"及"蠕虫状",常充填于粒间孔、长石次生溶孔及碳酸盐胶结物溶孔中并形成良好的晶间孔隙。2)研究区主要发育两期高岭石,第一期主要充填于早期碳酸盐胶结物溶孔中,呈微小"蠕虫状";第二期充填于铁方解石与铁白云石胶结物溶孔中,部分高岭石具碱性溶蚀特征,且第二期高岭石与晚期伊利石共生。3)研究区东三段储层具备一定的渗流能力,使长石溶蚀形成的"副产物"被流体带走;但在破坏性成岩作用下,储层渗流能力会逐渐变差,最终使得"副产物"堆积于孔隙,降低储层物性。4)高岭石及同期硅质胶结物对储层物性的影响是一把"双刃剑",当高岭石及硅质的体积分数低于6.81%时,长石溶蚀有利于改善储层物性;当高岭石及硅质的体积分数高于6.81%时,则不利于储层物性的改善。 相似文献
375.
Extensional and compressional structures are globally abundant on Mars. Distribution of these structures and their ages constrain the crustal stress state and tectonic evolution of the planet. Here in this paper, we report on our investigation over the distribution of the tectonic structures and timings of the associated stress fields from the Noachis-Sabaea region. Thereafter, we hypothesize possible origins in relation to the internal/external processes through detailed morphostructural mapping. In doing so, we have extracted the absolute model ages of these linear tectonic structures using crater size-frequency distribution measurements, buffered crater counting in particular. The estimated ages indicate that the tectonic structures are younger than the mega impacts events(especially Hellas) and instead they reveal two dominant phases of interior dynamics prevailing on the southern highlands, firstly the extensional phase terminating around3.8 Ga forming grabens and then compressional phase around 3.5-3.6 Ga producing wrinkle ridges and lobate scarps. These derived absolute model ages of the grabens exhibit the age ca. 100 Ma younger than the previously documented end of the global extensional phase. The following compressional activity corresponds to the peak of global contraction period in Early Hesperian. Therefore, we conclude that the planet wide heat loss mechanism, involving crustal stretching coupled with gravitationally driven relaxation(i.e.,lithospheric mobility) resulted in the extensional structures around Late Noachian(around 3.8 Ga). Lately cooling related global contraction generated compressional stress ensuing shortening of the upper crust of the southern highlands at the Early Hesperian period(around 3.5-3.6 Ga). 相似文献
376.
对一株具有细胞毒活性的南极青霉属真菌Penicillium sp.S-1-16进行发酵条件的初步优化。通过对基础发酵培养基、发酵温度及培养基配制用水的筛选,以次级代谢产物量为主要指标,同时参考生物量及细胞毒活性指标来进行初步优化,获得一个较优的摇瓶发酵条件:酵母提取粉0.3%,蛋白胨0.5%,麦芽糖0.3%,葡萄糖1%,蔗糖5%,自来水,初始p H=7.0,接种量15%,18℃,180 r·min-1发酵15 d。采用初步优化后的条件进行发酵,与初始发酵条件相比,其次级代谢产物量提高到568.75%,对A549肿瘤细胞的抑制作用增强至265%,并且对He La肿瘤细胞和SGC-7901肿瘤细胞的抑制率分别从0提高到48.19%和69.18%,效果显著,为获得菌株中活性次级代谢产物奠定了基础。 相似文献
377.
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379.
M.M. Massaferro J. Massaferro G. Roman Ross A.J. Amos A. Lami 《Journal of Paleolimnology》1999,22(2):137-148
Stratigraphy of Lake El Trébol (41°S 71°W, 758 m a.s.l.) described from an 11 m long sediment core provided a continuous record of patecenvironmental changes occurred during the last 14,000 years in southern South America east of the Andes. Located in an ecotonal area within a strong humidity gradient, this lake offers a unique opportunity to develop paleolimnological studies. Using a geochemical approach that includes elemental analysis, bulk organic matter, major nutrients and pigments combined with chironomids and pollen analysis, three zones were identified in the sedimentary record of this take. The oldest one (between 680 and 1,100 cm) corresponds to the late Glacial period. During that time, clayish laminated sediments were formed in a proglacial environment. Low organic matter, biogenic silica and nitrogen contents and the absence of pigments, pollen and chironomids characterise this period. At the end of this period, ca. 14,000 yr BP, a sharp increase in phosphorus concentrations predates major changes in limnological parameters. The transition zone (between 560 and 680 cm) is related to major changes in the drainage system that started soon after ca. 14,000 yr BP and continued to ca. 10,500 yr BP. The chemical composition of the sediments was affected by an increase in physical weathering mechanisms almost coincident with the increase in the regional volcanic activity that produced suspended volcanic detritus. The increase of mainly coarser detritical components may indicate a reorganisation of the fluvial system by that time. Simultaneously, an increase in the productivity of the lake accompanied by a gradual replacement of open vegetation with Nothofagus, Poaceae and Ericaceae, by Nothofagusforest, was observed. In the last zone (between 0 and 560 cm) the productivity of Lake El Trébol achieves maximum values. The trends in geochemical and biological indicators observed at Lake El Trébol can be up to some extent, correlated to those registered in Lake Mascardi. The results support earlier paleoctimatic scenarios from southern South America. 相似文献
380.
周国荣 《中国天文和天体物理学报》1999,(1)
讨论了在以冷暗物质为主的宇宙中,超新星爆发对矮星系演化的反馈作用。建立了星系的质量丢失模型,提出了理论模型与观测进行比较的方法。对数值计算结果的理论分析表明,当星系外围存在一个暗物质晕时,由超新星爆发引起的质量丢失虽然受到了极大的限制,却不像人们预期的那么困难。如果假定星系的形成红移为z=2~8,那么,在所选取的参数范围内,理论计算和观测结果是相符合的。这种定性上的符合显示出,星系的质量越小,它们就形成得越早. 相似文献