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951.
雄安新区蓟县系雾迷山组中赋存丰富的地热资源,研究雾迷山组岩溶热储特征及优质储集层发育的主控因素是地热资源勘探的基础。综合运用野外剖面、岩心、薄片、钻井、测井、录井等地质与地球物理资料,对雾迷山组岩溶热储特征和演化过程进行了深入研究,明确了优质储集层形成的控制因素,预测了有利靶区。结果表明,雾迷山组岩溶热储主要岩性为晶粒白云岩、颗粒白云岩、微生物白云岩、硅质白云岩和角砾白云岩等,溶蚀孔洞、裂缝及其组合为主要的储集空间类型。雾迷山组热储平均孔隙度为3.18%,平均渗透率为91.48×10-3 μm2;其中角砾白云岩物性最好。雾迷山组岩溶热储经历了沉积—准同生期成孔(雾迷山沉积期)、Ⅰ期表生增孔(雾迷山沉积期后至青白口纪前)、Ⅰ期埋藏减孔(青白口纪前至三叠纪)、Ⅱ期表生增孔(三叠纪—古近纪)、Ⅱ期埋藏减孔(新近纪—第四纪)5个阶段,岩性及岩相、成岩作用和构造应力是雾迷山组有利热储形成的主控因素。藻云坪—云坪相、表生岩溶、埋藏溶蚀、准同生岩溶、岩溶高地—斜坡和地层裂缝段比率大于0.4的6项叠合区是研究区最有利的岩溶热储发育区。 相似文献
952.
杭州湾海域春、秋季鱼类种类组成和数量分布 总被引:8,自引:0,他引:8
采用底层拖网法, 用渔获率作为鱼类资源数量分布的指标, 进行了杭州湾调查海域2012年5月(春季)、10月(秋季)2个季节的鱼类种类组成、区系特点、数量分布等研究。结果表明: (1) 杭州湾海域春、秋两季共获得并鉴定出的鱼类有31种, 隶属于9目15科, 其中以石首鱼科和 虎鱼科的种类为最多, 各有5种, 分别占总种数的16.7%; 鳀科鱼类次之, 有4种, 占总种数的13.3%, 优势种有睛尾蝌蚪 虎鱼、龙头鱼、刀鲚、棘头梅童鱼; (2) 根据鱼类适温性可将该海域的鱼类分为暖水性、暖温性和冷温性3种适温类型, 以暖温性种类为主, 暖水性种类次之, 而冷温性种类极少, 仅有1种; (3) 根据其生态习性, 可分为河口性、沿岸性和近海性3种生态类群; (4) 渔获数量分布规律是春季在调查海域的内侧或者说中西部较高, 而湾口较低, 秋季则正好相反。 相似文献
953.
Field detection of chlorophyll-a concentration in the sea surface layer by an airborne oceanographic lidar 总被引:2,自引:0,他引:2
LIU Zhishen MA Sen WANG Xin LI Zhigang 《中国海洋大学学报(英文版)》2008,7(1):108-112
An airborne oceanographic lidar, with a frequency-tripled Q-switched Nd: YAG laser of 355 nm, has been designed to measure chlorophyll-a (Chl-a) concentration in the sea surface layer by the Ocean Remote Sensing Institute, OUC. The field experiment was carried out in the bay which is located south of the Liaodong Peninsula on the 10th of September 2005. After the flight, the raw data were processed and analyzed by the fluorescence-to-Raman ratio method with seawater attenuation coefficients calculated from signal profiles. The results of Chl-a concentration sea water were also compared with those of Chl-a concentration by measurements by lidar are shown. The measurements in clear a Moderate Resolution Imaging Spectroradiometer (MODIS). 相似文献
954.
鲈鱼苗烂鳃、烂尾病病原菌的研究 总被引:7,自引:2,他引:7
1997年4~5月,对花鲈(Lateolabraxjaponicus)鱼苗期细菌性烂鳃和烂尾病的病原菌进行了研究。从具有明显症状的病鱼的病灶组织分离到2株致病菌C-1和W-1,经人工感染及从人工感染发病鱼体再分离的W-4和W-5菌株的再感染试验结果表明,所分离的细菌为鲈鱼苗烂尾,烂鳃病的致病菌。经64项生物学特性,生理生化特征测试结果表明,这4株菌可归为一类,同属于鳗弧菌(Vibrioanguilarum)。药敏试验结果表明,痢特灵、CIN100、MEL25、呋喃妥因、氯霉素、磺胺药+TMP和美洛西林等7种药物对病原菌有显著的抑制作用。 相似文献
955.
MUKESH R K MANHAS A K TRIPATHI A K RAINA M K GUPTA S K KAMBOJ 《Journal of Earth System Science》2011,120(1):123-144
The peteromineralogical characterization of the soil was carried out for the 12 soil profiles exposed in the Shorea robusta dominated forests of the Siwalik forest division, Dehradun. The quartz was observed as the dominating light mineral fraction
(64–80%) in all the profiles studied. Biotite, hornblende, zircon, tourmaline, rutile and opaques comprising of iron minerals
constituted the heavy mineral fraction (20%). The mineralogy of both the sand and clay fractions revealed a mixed mineralogy.
The clay minerals in the order of their dominance were vermiculite, illite, kaolinite and mixed layer minerals. The presence
of vermiculite and illite in appreciable quantities indicates that these were synthesized from the K-rich soil solution, as
orthoclase and micas were present in significant quantities in the sand minerals. The mineral suites identified in the study
shows that the geological, climatological and topographical factors of the region collectively played a dominant role in their
formation and transformation. After critical appraisal of the results, it may be deduced that the mineralogical composition,
physicochemical properties and total elemental analysis of the soils do not show any deficiency of the bases and other plant
nutrients in general. The inherent fertility of the soil is good as indicated by the sand and clay mineralogy of the soil
and the biotite and feldspar together with the mica is an important source of nutrients for the vegetation in the soils of
the Doon valley. 相似文献
956.
Studying relativistic compact objects is important in modern astrophysics to understand several astrophysical issues. It is therefore natural to ask for an internal structure and physical properties of specific classes of compact stars from astrophysical observations. We obtain a class of new relativistic solutions with anisotropic distribution of matter for compact stars. More specifically, stellar models, described by an anisotropic fluid, establishing a relation between metric potentials and generating a specific form of mass function, are explicitly constructed within the framework of General Relativity. New solutions can be used to model compact objects, which adequately describe compact strange star candidates like SMC X-1, Her X-1 and 4U 1538-52, with observational data taken from Gangopadhyay et al. (Mon. Not. R. Astron. Soc. 431:3216, 2013). As a possible astrophysical application the obtained solutions could explain the physics of selfgravitating objects, and might be useful for strong-field regimes where data are currently inadequate. 相似文献
957.
Aaron T. David Charles A. Simenstad Jeffery R. Cordell Jason D. Toft Christopher S. Ellings Ayesha Gray Hans B. Berge 《Estuaries and Coasts》2016,39(3):767-780
During the transition of juveniles from fresh water to estuarine and coastal environments, the survival of Pacific salmon (Oncorhynchus spp.) can be strongly size selective and cohort abundance is partly determined at this stage. Because quantity and quality of food influence juvenile salmon growth, high rates of prey and energy acquisition during estuarine residence are important for survival. Human activities may have affected the foraging performance of juvenile salmon in estuaries by reducing the area of wetlands and by altering the abundance of salmon. To improve our understanding of the effects of wetland loss and salmon density on juvenile salmon foraging performance and diet composition in estuaries, we assembled Chinook salmon (Oncorhynchus tshawytscha) diet and density data from nine US Pacific Northwest estuaries across a gradient of wetland loss. We evaluated the influence of wetland loss and density on juvenile Chinook salmon instantaneous ration and energy ration, two measures of foraging performance, and whether the effect of density varied among estuaries with different levels of wetland loss. We also assessed the influence of wetland loss and other explanatory variables on salmon diet composition. There was no evidence of a direct effect of wetland loss on juvenile salmon foraging performance, but wetland loss appeared to mediate the effect of density on salmon foraging performance and alter salmon diet composition. Specifically, density had no effect on foraging performance in the estuaries with less than 50 % wetland loss but had a negative effect on foraging performance in the estuaries with greater than 50 % wetland loss. These results suggest that habitat loss may interact with density to constrain the foraging performance of juvenile Chinook salmon, and ultimately their growth, during a life history stage when survival can be positively correlated with growth and size. 相似文献
958.
兴凯湖沉积物有机碳和氮及其稳定同位素反映的28kaBP以来区域古气候环境变化 总被引:2,自引:0,他引:2
兴凯湖是东北亚最大的淡水湖,也是中俄界湖。我们是国内首次对兴凯湖一根长269 cm的沉积岩心进行了研究,结果显示:δ13Corg和TOC之间显示较好的负相关性,说明δ13Corg低值时期,气候温暖或湿润,δ13Corg值处于高值时期,气候冷干;C/N比值和TOC之间显示较好的正相关性,C/N比值平均值为11.4,显示兴凯湖沉积物有机质以内源浮游植物生产为主;δ15Norg高值对应于气候冷干期,此时沉积物有机质更多的来源于浮游植物,δ15Norg低值对应于暖湿期,但营养盐输入的减少也会造成δ15Norg值降低。兴凯湖沉积物有机碳和氮及其稳定同位素数据综合分析结果表明:28 480~26 160 cal.aBP,湖区气候冷干;26 160~22 880 cal.aBP,湖区气候温暖湿润;22 880~18 180 cal.aBP,流域处于末次盛冰期多年冻土环境;18 185~12 650 cal.aBP,对应于Blling/Older Dryas/Allerd气候波动暖期;90~78 cm段,对应于Younger Dryas事件;11 500~4 570 cal.aBP,进入全新世暖湿期,早期气候温干,晚期气候温湿;4 570~1 470 cal.aBP,气候冷干;1470 cal.aBP以来,又转为暖湿气候。 相似文献
959.
Melaine Saillenfest Marc Fouchard Giacomo Tommei Giovanni B. Valsecchi 《Celestial Mechanics and Dynamical Astronomy》2017,127(4):477-504
We use a secular representation to describe the long-term dynamics of transneptunian objects in mean-motion resonance with Neptune. The model applied is thoroughly described in Saillenfest et al. (Celest Mech Dyn Astron, doi: 10.1007/s10569-016-9700-5, 2016). The parameter space is systematically explored, showing that the secular trajectories depend little on the resonance order. High-amplitude oscillations of the perihelion distance are reported and localised in the space of the orbital parameters. In particular, we show that a large perihelion distance is not a sufficient criterion to declare that an object is detached from the planets. Such a mechanism, though, is found unable to explain the orbits of Sedna or (2012text {VP}_{113}), which are insufficiently inclined (considering their high perihelion distance) to be possibly driven by such a resonant dynamics. The secular representation highlights the existence of a high-perihelion accumulation zone due to resonances of type 1:k with Neptune. That region is found to be located roughly at (ain [100;300]) AU, (qin [50;70]) AU and (Iin [30;50]^{circ }). In addition to the flux of objects directly coming from the Scattered Disc, numerical simulations show that the Oort Cloud is also a substantial source for such objects. Naturally, as that mechanism relies on fragile captures in high-order resonances, our conclusions break down in the case of a significant external perturber. The detection of such a reservoir could thus be an observational constraint to probe the external Solar System. 相似文献
960.
The thermal impact of several kilometre-thick magmatic underplating in the lower continental crust is studied with analytical and numerical methods. Simple analytical solutions are derived for the thermal transient in the case of an infinite depth below the underplate and also for the case of a finite depth (down to the asthenosphere). It is shown that these solutions lead to simple approximations for when the transient surface heat flow is at its maximum, what the maximum is, and for how long the transient lasts. Even though these solutions assume that the underplate is emplaced instantaneously, they are useful in the interpretation of underplating over finite time spans. A numerical scheme is suggested for the modelling of underplating that handles both short time intervals as well as long intervals. The scheme treats magmatic underplating in a mass and energy conservative manner, and it is compared against the analytical solutions. Finally, the analytical and numerical results for thermal transients are applied to a transect from the Vøring margin (NE Atlantic), with respect to various degrees of early Cenozoic magmatic intrusion. It appears that more than half of the lower crustal body (LCB) in the Vøring margin must be magmatic underplating for the vitrinite reflectance to be substantially higher than for the non-magmatic case, where the LCB is assumed to comprise Caledonian crust. 相似文献