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991.
石油包裹体显微测温和体积分析已经被广泛应用于重构石油包裹体组分和压力-温度(P-T)捕获条件, 然而, 其P-T捕获条件准确预测除精确的均一温度(Thoil)和气泡充填度(Fv)测试外, 还依赖于石油饱和压力和体积预测能力.基于改进石油流体饱和压力和气、液相摩尔体积预测精度, 建立了石油流体C7+组分摩尔含量与其Thoil和室温(20 ℃)下Fv之间的定量关系.尽管利用该定量关系可以极大地简化石油包裹体热动力学模拟过程, 还是不能避免Fv对热动力学模拟精度的影响.因此, 根据大量已知组分石油流体建立了甲烷摩尔含量约束的新的石油包裹体捕获压力预测模型.新模型中唯一变量即为石油包裹体甲烷摩尔含量, 并且不再依赖于专业的热动力学模拟软件(PVTsim、VTflinc、PIT和FIT-OIL), 从而极大地简化了传统石油包裹体捕获压力重构过程.最终, 新模型捕获压力预测精度得到评价, 石油包裹体甲烷摩尔含量对捕获压力重构具有重要控制作用, 单个石油包裹体甲烷含量定量化是未来石油包裹体捕获压力重构的主要研究方向. 相似文献
992.
通过原油裂解动力学和石油包裹体热动力学模拟方法系统阐述了地质条件下原油裂解过程对油包裹体均一温度及捕获压力的影响.结果表明:初始裂解阶段(TR<13%,T<160 ℃),油包裹体均一温度随原油裂解呈增大趋势,捕获压力呈减小趋势;随着裂解程度增大(TR<24%,T<190 ℃),油包裹体均一温度随原油裂解呈减小趋势,捕获压力呈增大趋势,但此阶段油包裹体均一温度仍高于初始捕获时均一温度,捕获压力仍小于初始捕获压力;此后,随着原油裂解程度不断增大,油包裹体均一温度持续减小甚至到负值,捕获压力则持续增大甚至超过静岩压力.封闭条件下低程度的原油裂解(T<160 ℃,TR<13%)只会形成常压或者低压;而较高程度的原油裂解(TR>40%)才会形成超压,甚至超过上覆静岩压力(TR>70%).深部原油裂解气勘探中要特别注意地层温度位于160~190 ℃范围内的常压到低压油气藏,而地层温度高于190 ℃原油裂解气勘探应以找超压-超高压油气藏为主. 相似文献
993.
994.
本实验旨在研究稻田土壤中甲烷产生率对稻田CH_4排放的影响.观测结果表明:土壤各深度的甲烷产生率有很大的变化范围(1—4639ng·h~(-1)·g~(-1)d.w.).主要的甲烷产生区域是7—17cm深的土壤层,其中以13cm深的土壤层上的生成速率最大.土壤中甲烷产生率与稻田CH_4排放率在水稻生长的某些阶段有较好的相关性,但它的季节变化却不能与排放的季节变化完全耦合.在水稻生长期,土壤中甲烷产生率随时间而增大,并在8月份水稻收割前达到最大,其日平均值在38—767 ng·h~(-1)·g~(-1)d.w.间变动.稻田土壤中甲烷产生率也存在日变化,一般在下午达到最大值,但却没有发现它与土壤温度有明显的相关关系.在不同施肥及水稻品种的稻田土壤中也观测到不同的甲烷产生率.在土壤中产生的甲烷最多只有28.8%被排放到大气中,而其余多于71.2%的则被氧化在土壤中. 相似文献
995.
Gordon E. Sarty Bogumil Pilecki Daniel E. Reichart Kevin M. Ivarsen Joshua B. Haislip Melissa C. Nysewander Aaron P. LaCluyze Helen M. Johnston Robert R. Shobbrook Lászl L. Kiss Kinwah Wu 《中国天文和天体物理学报》2011,(8)
We searched for long period variation in V-band,IC-band and RXTE X-ray light curves of the High Mass X-ray Binaries(HMXBs) LS 1698 /RX J1037.5-5647,HD 110432 /1H 1249-637 and HD 161103 /RX J1744.7-2713 in an attempt to discover orbitally induced variation. Data were obtained primarily from the ASAS database and were supplemented by shorter term observations made with the 24-and 40-inch ANU telescopes and one of the robotic PROMPT telescopes. Fourier periodograms suggested the existence of long period variat... 相似文献
996.
997.
The Cimmerian terrane forms an almost unbroken chain stretching >13,500 km, from central southern Europe to western Indonesia, via SE Europe, the Middle East, Afghanistan, Tibet, SW China and Myanmar. Ar-guably, it is Earth’s most spectacular example of a “sliver” terrane, dwarfing in size more recently devel-oped examples, for instance the Palawan Block in the western Philippines, and the Lord Howe Rise in the Tasman Sea. The presentation will first outline the in-triguing geological features associated with this unique tectonic entity. Following that, recently obtained results following paleomagnetic investigations of two lower Permian rift-related basalt suites will be summarized (Abor Volcanics in northeastern India and Woniusi Ba-salts in Yunnan, China). The two studies are part of a larger programme of ongoing research aimed at deducing (I) the geodynamic configuration that generated the un-usual rifting system, and (II) exactly how Cimmeria fit-ted against Gondwana prior to its dispersal in the Early Permian. The critical unit is Baoshan, which we fit against Gondwana within a narrow longitudinal belt close to where northern India and northwestern Australia were once in close proximity (Fig. 1). Furthermore, we suggest that Sibumasu lay to directly the east, offshore of Australia; Qiangtang and Lhasa almost certainly sat to the west (off northern Greater India-SE Arabia), but we are uncertain as to their exact configuration. Our findings will be compared with several rather different models that have been published in recent years. The new pa-leomagnetic constraint highlights the flexibility authors currently have in reconstructing the region, principally because of the overall lack of similar high-quality data from the various blocks. We explain how new data could resolve these ambiguities, thereby offering more robust explanations for eastern Gondwana’s late Paleozoic de-velopment. 相似文献
998.
Karlo L. QUEA?O Carla B. DIMALANTA Graciano P. YUMUL JR. Decibel V. FAUSTINO-ESLAVA Edanjarlo J. MARQUEZ Noelynna T. RAMOS Keisuke ISHIDA Shigeyuki SUZUKI Ricky C. SALAPARE Michael Peter M. SANCHEZ Juan Miguel R. GUOTANA Rose Ann B. CONCEPCION 《地球学报》2012,33(S1):58-58
A number of geological studies have already been conducted on the Zambales Ophiolite Complex (ZOC), a north-south trending complete ophiolite sequence exposed in the western portion of Central Luzon, Philippines. Previous works recognized the ZOC as being made up of two blocks, the Acoje and the Coto, acting as an arc-back arc pair sometime during the Eocene. 相似文献
999.
Four different varieties of charnockitic rocks,with different modes of formation,from the Mesoproterozoic Natal belt are described and new C isotope data presented.Excellent coastal exposures in a number of quarries and river sections make this part of the Natal belt a good location for observing charnockitic field relationships.Whereas there has been much debate on genesis of charnockites and the use of the term charnockite.it is generally recognized that the stabilization of orthopyroxene relative to biotite in granitoid rocks is a function of low aH2O(±high CO2),high temperature,and composition (especially Fe/(Fe +Mg)).From the Natal belt exposures,it is evident that syn-emplacement.magmatic crystallization of chamockite can arise from mantle-derived differentiated melts that are inherently hot and dry(as in the Oribi Gorge granites and Munster enderbite),as well as from wet granitic melts that have been affected through interaction with dry country rock to produce localized charnockitic marginal facies in plutons(as in the Portobello Granite).Two varieties of post-emplacement sub-solidus chamockites are also evident.These include charnockitic aureoles developed in leucocratic,biotite.garnet granite adjacent to cross-cutting enderbitic veins that are attributed to metamorphic-metasomatic processes(as in the Nicholson’s Point granite,a part of the Margate Granite Suite),as well as nebulous,patchy charnockitic veins in the Margate Granite that are attributed to anatectic metamorphic processes under low-aHO fluid conditions during a metamorphic event.These varieties of chamockite show that the required physical conditions of their genesis can be achieved through a number of geological processes,providing some important implications for the classification of charnockites,and for the interpretation of charnockite genesis in areas where poor exposure obscures field relationships. 相似文献
1000.
幔源角闪石巨晶中硫化物熔融包裹体研究 总被引:1,自引:0,他引:1
硫化物熔融包裹体研究是认识硫化物矿床成矿元素来源和演化的重要手段,由于硫化物熔融包裹体的体积较小(粒径仅为10~20μm),其详细化学元素组分的难以获得一直是制约进一步研究的瓶颈。笔者在前人研究的基础上,借助于扫描电镜、电镜能谱和二次飞行时间离子探针(Tof-SIMS)对产于铜陵地区角闪石巨晶中的硫化物熔融包裹体进行了详细的研究,首次获得了一套精确的矿物化学资料和元素分布图。矿物学研究表明,角闪石巨晶在上地幔和下地壳均有结晶,温压区间分别为T:850~900℃(温度),P:0.70×109~0.82×109Pa(压力),对应深度D:23.10~27.06km;和T:900~950℃,P:1.09×109~1.17×109Pa,D:35.97~38.61km。元素分布图显示,硫化物熔融包裹体主要有两种元素组成体系:S-Fe-Mn-Ni-Rb-Sr-Ba和S-Fe-Cu-Sr,幔源硫化物体系中Mn、Ni、Rb、Ba等元素具有相似的性质特征可共溶,与Cu则表现出不混溶。在铜陵地区,上地幔的部分熔融形成了一套碱性玄武岩浆,后受岩浆底侵作用和壳幔相互作用影响,底侵进入下地壳深位岩浆房,发生结晶分异和同化混染作用,形成一套轻度演化的玄武岩浆,可能为辉长质。上地幔和下地壳的角闪石巨晶分别是由上地幔碱性玄武岩浆和下地壳轻度演化的玄武岩浆(辉长质)高压下结晶的产物。当上地幔碱性玄武岩浆上侵到下地壳深位岩浆房以后,发生结晶分异作用,又由于地壳硅镁层的混染作用,使得玄武岩浆中硫溶解度降低,促其熔离,从而释放大量的硫(S,以及Ni、Cu、Cr)。角闪石巨晶中的硫化物熔融包裹体正是在下地壳深位岩浆房中,由正在结晶的角闪石巨晶在结晶分异和轻度演化的玄武质岩浆中捕获的不混溶硫化物熔融液滴形成的。铜陵地区在中生代经历了一个长期的大规模的岩浆底侵作用和壳幔相互作用过程,由于下地壳硅镁层混染作用使得轻度演化的玄武岩浆释放大量硫,必然会在莫霍面附近形成大规模高浓度的硫富集区,这些组分在岩浆上侵作用、地壳减薄作用或者裂谷作用的影响下很容易再活化,进入区域岩浆-热液流体系统,最终参与形成区域大规模的硫化物矿床。 相似文献