- 更多网络例句与岩浆玄武岩相关的网络例句 [注:此内容来源于网络,仅供参考]
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This conclusion, combined with the data obtained from the short-lived Hf-W and Sm-N d isotopic systematics, suggests that the Moon was initially accreted at 4.5 Ga, followed by development of the global lunar magma ocean. The primary lunar crust is composed by ferroan anorthosite which was produced by flotation of plagioclase during crystallization of the LMO. However, the mafic minerals, coevally crystallized with the plagioclase, sank to the base of the LMO due to their high density, and made up the main part of the lunar mantle, which served as the source during later mare basaltic magmatism.
根据这一年代资料,结合对月岩样品进行的短半衰期Hf-W与Sm-Nd同位素体系的研究结果,认为月球大致形成于45亿年,其后开始由岩浆海导致的内部核-幔-壳的分异,岩浆结晶的低密度斜长岩构成最初的月壳,而密度大的岩石构成月幔,而此月幔则成为后来月海玄武岩的主要岩浆源区。
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Based on major and trace elements and isotope geochemical data, it is inferred that Sandouding suite is formed by magma melting of Late Archeozoic continent tholeiite source, and its geochemical variation is controlled by hornblende fractional crystallization. Besides fractional crystallization, the geochemical variation of Huanglingmiao suite is related to the mixing between dacitic magma and felsic magma. Dalaoling suite is probably derived from early Precambrian volcanics.
根据岩石化学和同位素组成推断,三斗坪岩套的源岩主要是晚太古代大陆拉斑玄武岩,母岩浆相当于英安质,岩套内的成分变化主要受角闪石分离结晶作用控制;黄陵庙岩套除受分离结晶作用影响外,成分变化主要与英安质母岩浆和某种长英质岩浆的混合有关;大老岭岩套的源岩亦为早前寒武纪火山岩。
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The formation and evolution of magma have experienced three stages:① thermal fluid led to higher partial melting of lithosphere mantle and then formed hypoalkaline basalt with saturated initial sulfur when ascending asthenosphere contacted with the lithosphere mantle;② the initial magma intruded into the lower crust to form magma chamber, the crystallization of magma produced stratiform-like cumulate, including olivine, hypersthene, augite, magnetite, and then formed residual gabbroic magma with the participance of crustal material;③ the residual magma and ore-bearing cumulate intruded upward successively to shape original mafic complex rocks in Wuxing when the magma chamber cracked.
岩浆形成与演化经历了3个阶段:①上升的软流圈与岩石圈地幔接触,热流体作用导致岩石圈地幔发生高度部分熔融,形成初始硫饱和的次碱性玄武岩;②初始岩浆上侵,在下地壳形成岩浆房,岩浆结晶作用形成以似层状橄榄石、紫苏辉石、普通辉石和磁铁矿等为主的堆晶岩,在地壳物质的参与下形成残余辉长质岩浆;③岩浆房破裂,残余岩浆和含有熔体(0%)的堆晶岩相先后上侵形成五星原始镁铁质杂岩。
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Well-documented Lu-Hf isotope data from the oceanic basalts show that,the starting area of magma melting for the MORBs derived from the DMM component would be in the the depth of garnet peridotite,i.e.at the depth of 80―90 km instead of less than 60 km,which is at the depth of spinel peridotite as proposed early.The HIMU component,which is characterized by its high rediogenic lead,is refered as a special mantle component differentiated at some time in geological history from the lower mantle.A correlation study of Hf-Nd isotope between the chondrite and oceanic basalts implies that no isolated primitive mantle might have remained.
大量的大洋玄武岩Lu-Hf同位素研究表明:具亏损地幔端元来源的洋中脊玄武岩岩浆部分熔融的初熔区位于石榴石稳定场深度,即深度为80-90 km的石榴石二辉橄榄岩地幔,而不是原来所认为的尖晶石二辉橄榄岩区(深度小于60 km);以高放射成因Pb为特征的高U地幔端元应代表了下地幔物质在某一特定时期发生分异作用的结果;球粒陨石与大洋玄武岩Hf同位素对比研究表明,没有原始地幔物质能保留至今的迹象。
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On the basis of the study on the petrology, Trace element, and isotopic geochemistry, the primary magma of volcanic rocks can be divided into two series according to their originated rocks and degree of partial melting. One is the basanite-alkaline basalt-Olivine tholeiite magma series, which are generated by partial melting from spinel Iherzolite; the other is nephelinite magma-alkaline picritic basalt magma, which are generated by partial melting of the garnet Iherzolite.
岩石化学、微量元素、同位素地球化学证据都表明,华北、华南地区的火山岩根据源岩和局部熔融程度的不同,可以分为两个原生岩浆系列:一个是源岩为尖晶石二辉橄榄岩,随着局部熔融程度的增加,形成的碧玄岩岩浆-碱性玄武岩岩浆-橄榄拉斑玄武岩岩浆;另一个是源岩为石榴石二辉橄榄岩,随着局部熔融程度的增加形成的霞石岩岩浆-碱性苦橄玄武岩系列。
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Following evidences indicate that lherzolite and garnet pyroxenite xenoliths in basalts are captures of mantle fragments when host magma ascending: crystallizing temperatures and pressures of cpx megacrysts and some phenocrysts in host magmas are greater than equilibrium temperatures and pressures of xenoliths; calculated REE partition pattern of assumed equilibrium melts is not comparable with that of studied host basalt rocks; olivine in xenoliths is not in equilibrium with basalt rocks.
寄主玄武岩的单斜辉石斑晶—熔体平衡温度高于石榴石二辉橄榄岩和石榴石辉石岩包体的平衡温度,单斜辉石巨晶和部分斑晶—熔体平衡压力大于包体平衡压力,寄主碱性玄武岩的稀土配分型式和所计算的与尖晶石二辉橄榄岩包体平衡的熔体的稀土配分型式不同,包体橄榄石与寄主岩浆之间的Fe-Mg交换系数低于0.30,均表明包体与寄主玄武岩浆之间不存在平衡关系,因此,包体是被寄主玄武岩浆捕虏的上地幔碎块。
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On the basis of an integrated analysis of the geochemical features of these volcanic rock associations,this paper concludes that thebasalts originated mainly from interaction between mantle-derived magma and low-crustal materials, and rhyolitic volcanic rocks resulted from thermal and chemical interaction between basaltic magma and the upper part of crustal materials.Basalts and rhyolites in different cycles have different source regions,and they are products of multiperiodic pulsive layer partial melting.
根据对火山岩地球化学特征的综合分析表明,玄武岩主要为幔源岩浆与下部地壳岩石相互作用的产物,而流纹岩则为玄武岩浆与上部地壳物质进行热及成分交换的结果,不同旋回的玄武岩和流纹岩有不同的源区,为多次脉动分层部分熔融的产物。
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There are two evolutional trends for sodic basalts: alkaline basalt to sub-alkaline basalt and to the contrary. The fact that alkaline basalt has the higher concentration of incompatible elements and the sub-alkaline lower indicates the increasing degree of the partial melting in the mantle sources. The variety of Sr, Nd isotope compositions in different types of rocks shows their different mantle sources.
钠质玄武岩存在着碱性玄武岩到亚碱性玄武岩和亚碱性玄武岩到碱性玄武岩的变化序列;碱性玄武岩到亚碱性玄武岩不相容元素丰度逐渐降低,表明为部分熔融程度逐渐增高的产物;Sr、Nd同位素组成与岩性之间的相关性表明,各种岩浆是不同地幔源区部分熔融的产物。
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Trachyte has as the same isotope feature as the basalts, indicating that they were derived from the same source, and resulted from products during different evolution phases of the same magma source, which is similar to that of the basalts in Emeishan.
该区粗面岩类与玄武岩的同位素特征类似,说明二者具有相同的源区,并可能代表了同源岩浆不同演化阶段的的产物,这与峨眉山地幔柱岩浆活动的玄武岩与粗面岩所具有的演化关系相同。
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Some characteristic ratios suggest the picrites and ankaramites were derived from asthenospheric mantle, and high Os/Ir ratios reflect the involvements of pelagic sediments. Pd/Ir versus Ni/Cu diagram implies that the picrites and ankaramites were not primary magmas, but MgO-high basalts with excess olivines, whereas Pd versus Cu diagram suggests a S-undersaturated primary magma.
一些铂族元素的特征比值指示了苦橄岩和富辉玄武岩起源于软流圈地幔,而高的w/w比值则暗示了源区中有深海沉积物的加入。w/w-w/w图解说明本区的苦橄岩不是原始岩浆,而是原始的高镁玄武岩中有过剩橄榄石的加入,而w-w图解则说明原始岩浆硫不饱和。
- 更多网络解释与岩浆玄武岩相关的网络解释 [注:此内容来源于网络,仅供参考]
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achondrite:无球粒陨石
无球粒陨石(Achondrite)由岩浆结晶的不含球粒(宇宙源的球状体)的石陨石,约占已知陨石的4%,外观上与玄武岩、橄榄岩和辉岩等含硅量低的地球火成岩相似. 地球的岩浆曾形成基性岩和超基性岩,无球粒陨石也许是从和岩浆相似的熔融物质中结晶而成;
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mantle plume:地函热柱
根据最新的铀系元素分析结果显示,热点(hot spot)火山的岩浆来源很可能确实是来自於地函热柱(mantle plume). 最近在自然期刊(Nature)由Bourdon等人发表了根据铀系元素在海岛玄武岩(Ocean Island Basalt)中的含量特性.
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picrite:苦橄岩
苦橄岩(picrite)是一种稀少的岩石类型,由于它接近于原始岩浆成分,所以历来为岩石学家所重视.它主要形成于洋岛和大陆溢流玄武岩和大洋溢流玄武岩的环境中,也有少量分布于岛弧环境中.前者被认为与地幔柱有关,尽管其所占的岩浆体积比例很少,
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tektite:玻璃陨石
其最大特点是玻璃陨石(tektite)是一种黑色块状天然玻璃. 是一种经过熔融很快冷在高地玄武岩中,有一种富钾(K)、稀土(REE)和磷(P)的岩石,称为克里普(KREEP)岩. 这种岩石地球上未曾发现,是岩浆分异或残余熔浆结晶形是根据地震波传播的低速层(LVZ)确定的.
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volcanic rock:火山岩
喷出岩(extrusive rock)为岩浆流到地表冷凝而成,又称为火山岩(volcanic rock),超基性岩浆(Ultramafic)铁镁质含量更高,二氧化矽含量更少,这类岩浆通常在地底下,玄武岩(Basalt)属於喷出的基性火成岩,所有的海洋地壳都属於此类,
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shield volcano:盾状火山
'''盾状火山'''(Shield Volcano)具有宽广缓和的斜坡,整体看来就像是一个[[盾牌]]. 此种火山通常由玄武岩岩浆构成,流动性高,故能够分布在很大的区域,才能形成宽广的山形. 最著名的例子是[[夏威夷群岛]],这个群岛的每个岛屿都是一座巨大的盾状火山.
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magma basalt:玻璃玄武岩
magma association 岩浆共生组合 | magma basalt 玻璃玄武岩 | magma consolidation 岩浆固结
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magma basalt:岩浆玄武岩
"岩浆型","magma type" | "岩浆玄武岩","magma-basalt" | "岩浆玻璃灰","magma-glass-ashes"
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alkali olivine basalt magma:碱性橄榄玄武岩岩浆
alkali metal 碱金属 | alkali olivine basalt magma 碱性橄榄玄武岩岩浆 | alkali rock series 碱性岩系