巴尔哲碱性花岗岩中的熔体和熔体-流体包裹体: 岩浆-热液过渡的信息

熔体包裹体由被封存在矿物中的原始岩浆组成,有效的保存了有关其主矿物形成时周围岩浆介质的物理化学信息,是研究岩浆演化和成矿作用的原始样品。本文以内蒙古巴尔哲超大型稀有稀土金属矿床中伟晶岩壳和石英斑晶中的熔体包裹体和流体-熔体包裹体为研究对象,使用高温热台和激光拉曼进行分析。结果显示熔体包裹体的熔融温度在750~1027℃之间(平均为916℃),熔体-流体包裹体的均一温度在475~650℃之间(平均为562℃),而包裹体内的硅酸盐矿物和稀土矿物的存在表明巴尔哲岩体的岩浆-热液演化及其对稀有稀土矿化的制约。     

雷琼新生代玄武岩中地幔岩包体矿物中的流体─熔体包裹体的REE组成特征

雷琼地区新生代玄武岩中地幔岩包体的１２件单矿物稀土元素中子活化分析表明,雷州和琼北地幔岩包体中不含流体－熔体包裹体的同类矿物的ＲＥＥ组成有明显差异,反映了雷州与琼北玄武岩地幔源区ＲＥＥ组成的不均一性。通过对比同一地幔岩包体中含包裹体与不含包裹体相同矿物的微量元素组成,发现雷琼地幔岩包体矿物中的流体－熔体包裹体富含ＲＥＥ,尤其是ＬＲＥＥ;并且不同产地地幔包体同类矿物中和同一包体不同矿物中包裹体的丰度及其ＲＥＥ含量也有明显差异,表明地幔流体本身也存在不均一性。     

山东沂南金铜铁矿床中的液态不混溶作用与成矿：流体包裹体和氢氧同位素 证据

沂南矽卡岩型金铜铁矿床产于燕山期中酸性侵入岩与新太古界—寒武系地层接触带附近。氢、氧同位素研究表明,早期干矽卡岩阶段(Ⅰ)和湿矽卡岩-磁铁矿阶段(Ⅱ)的成矿流体主要为岩浆水,晚期石英-硫化物阶段(Ⅲ)和碳酸盐阶段(Ⅳ)的成矿流体则显示有大气降水混入的岩浆水特点。流体包裹体研究表明,成矿各阶段热液矿物中的包裹体类型丰富,以气液两相盐水包裹体、含子晶多相包裹体和CO2-H2O包裹体为主,次为纯液相水包裹体和纯气相水包裹体,偶见晶质熔融包裹体。由Ⅰ→Ⅱ→Ⅲ→Ⅳ阶段,气液水包裹体均一温度(520～430℃→430～340℃→250～190℃→190～130℃)呈现逐渐降低的趋势。在Ⅰ、Ⅱ阶段的石榴子石和绿帘石中,晶质熔融包裹体与同期次捕获的具不同气相分数的气液水包裹体及含子晶的多相包裹体共生,表明它们被捕获时是一种熔体与流体共存的不混溶状态。在Ⅲ阶段的石英(少量Ⅱ阶段的绿帘石)中,常见气相充填度变化很大的气液水包裹体与同期次捕获的纯液相水包裹体、纯气相水包裹体、含子晶的多相包裹体以及CO2-H2O包裹体共生,且共生的不同类型包裹体均一温度相近,表明此阶段成矿流体曾发生过广泛的沸腾(不混溶)。因而认为,在沂南矿床由岩浆...     

不透明矿物流体包裹体红外显微测温研究：进展、存在问题与解决方案

流体包裹体是古地质流体的唯一直接记录,为反演地质过程涉及的物理化学条件等提供了最为重要的证据。流体包裹体是研究热液矿床成矿流体最有利手段,常规的测试对象为透明的脉石矿物,而矿石矿物中的流体包裹体更为直接、准确地记录了成矿流体信息。大多数矿石矿物在显微镜透射光下不透明,其捕获的流体包裹体研究需要使用配备有红外成像系统的显微镜进行。近20 年来,不透明矿物流体包裹体红外显微测温研究获得了长足的进展,但其中仍有一些问题尚未解决,制约了该方法的应用;同时,国内该研究领域正处在起步阶段,多个实验室已安装了红外测试仪器,但尚未开展系统的研究工作。因此,需要对该研究领域进行综述,探讨存在的问题,以促进该研究方法的发展。本文首先介绍了红外显微镜仪器工作原理及样品制备注意事项,阐述了影响不透明矿物红外透明度的因素,讨论了红外显微测温研究中的主要问题和难点,并针对测温过程中相变观察困难、红外光可能影响测温结果等问题提出可行的解决方案,最后论述了红外显微测温系统在矿床学领域的应用前景。     

西藏班公湖带多不杂超大型富金斑岩铜矿的高温高盐高氧化成矿流体：流体包裹体证据

多不杂富金斑岩铜矿床位于斑公湖-怒江缝合带北侧多不杂构造岩浆弧中,成矿与侵位于中侏罗统雁石坪群和早白垩统美日切组地层中的石英闪长玢岩、花岗闪长斑岩有关.由于斑岩体的侵位,在岩体内及其围岩中形成强烈蚀变且分带明显,由含矿斑岩中心向外可划分出钾硅化带、中级泥化带、泥化带、伊利石-水白云母化-褐铁矿化带-角岩带或青磐岩化带（围岩是中基性火山岩时）.矿化为细脉-浸染状,含矿斑岩全岩矿化,少量矿化产于围岩中,成矿为铜-金组合,为典型的富金斑岩铜矿.初步识别出（1）钾化带中主要发育M型、EB型、A型及部分B型脉;（2）绿泥石化带（中级泥化带）中发育B型、C型、石英-绿泥石脉及S型、G型脉;（3）在粘土化带（泥化带）中主要发育C型脉、G型脉及S型细网脉;（4）在围岩中主要发育B型、C型、D型及G型细网脉以及碳酸盐脉、M型脉等.矿区范围内发育丰富的热液磁铁矿、赤铁矿、金红石等,铜、金沉淀与热液磁铁矿的形成关系密切;矿石中主要为黄铜矿、少量斑铜矿和辉铜矿,而黄铁矿很少,总体上为黄铜矿＞斑铜矿,黄铜矿＞黄铁矿.在石英斑晶及各种脉系中识别出三个大类和十个亚类的流体包裹体.包裹体显微测温数据表明最高（达935℃、压力200MPa）的均一温度出现在石英斑晶中,这种由含不透明子矿物、简单多相、含硅酸盐子矿物、赤铁矿多相包裹体类型构成的具45%NaCleq盐度的多相包裹体可能代表本矿床最原始的成矿流体组成;这种成矿流体上升到3km左右、冷却到580℃左右发生沸腾,分离出超高盐度（60%～80%NaCl eq）流体包裹体和富气相包裹体,并导致大量磁铁矿的结晶和还原硫的释放,且伴随部分金属硫化物及部分金沉淀,形成早期的M、A型脉;随着温度的进一步降低和分离出的流体包裹体的聚集,在500℃～480℃之间、22～40MPa之间、深度约1.5km发生沸腾,大量释放出的硫与金属离子结合,导致了大量铜、金的沉淀,形成如B型脉等一系列脉系及浸染状的铜矿化.在450℃～400℃之间、压力20～32MPa之间、深度1.1km左右又发生了明显的沸腾事件,形成了如C型脉、S型等舍铜脉系.在370℃～200℃之间、压力5～30MPa之间,包裹体以液相包裹体和多相包裹体为主,其盐度变化较大,可能是由于岩浆流体的稀释作用或少量大气降水参与循环所致,形成了D型脉及面状硅化.我们的研究结果揭示多不杂富金斑岩铜矿是主要由直接从岩浆熔体中出溶（600℃～950℃）的具高氧化性、（超）高盐度的富合成矿元素的岩浆流体形成的,是斑岩矿床系列中正岩浆端元的典型代表.     

西藏班-怒带西段荣那铜（金）矿床流体包裹体特征及矿床成因

荣那铜(金)矿床是班公湖-怒江缝合带西段新发现的矿床,是多龙矿集区的重要组成矿床之一,已探明储量达大型规模,具有超大型矿床的成矿潜力。荣那铜(金)矿床矿石矿相学与岩相学研究显示其具有典型高硫化型浅成低温热液型矿床的矿物组合(明矾石、硫砷铜矿等)和矿化蚀变特征。通过资料收集与野外观察,本文将荣那铜(金)矿床的成矿过程划分为石英-黄铁矿阶段、石英-多金属硫化物阶段与碳酸盐阶段,其中石英-多金属硫化物阶段为主成矿阶段。为查明该矿床的成矿流体特征,进一步确定矿床成因类型,对取自深部矿石中的石英脉(均为主成矿阶段含黄铁矿、黄铜矿石英脉)开展了流体包裹体的岩相学观察、显微测温和激光拉曼光谱分析。结果表明,上述矿物中主要发育富液相、富气相和含子矿物三相包裹体;富液相包裹体的均一温度与盐度分别为:80~440℃和4.63%~11.95%NaCl eqv;富气相包裹体的均一温度和盐度分别为:320~440℃和5.55%~10.74%NaCl eqv;含子矿物三相包裹体的均一温度与盐度分别为200~400℃和29.4%~32.56%NaCl eqv;富液相与富气相包裹体的气体成分除少量N2外,气体成分均为H2O。综合分析认为,荣那矿床成矿流体发生了强烈的沸腾作用,流体沸腾作用是该矿床的重要成矿机制。可见,荣那矿床具有高硫型浅成低温热液矿床的矿物组合及蚀变特征,但主成矿阶段石英脉流体包裹体特征与典型斑岩型铜(金)矿床的流体包裹体特征相似。因此,推测荣那高硫型浅成低温热液铜金矿的深部存在斑岩型铜金矿化,该矿床应属浅成低温热液型-斑岩型铜金矿床。     

西藏多不杂超大型富金斑岩铜矿的蚀变-矿化特征及高氧化成矿流体初步研究

多不杂富金斑岩铜矿位于斑公湖-怒江缝合带北侧的铁格山岩浆弧中。具O型埃达克岩特征的闪长玢岩、花岗闪长斑岩侵位于中侏罗统雁石坪群中。岩体内及其围岩中蚀变强烈，分带明显，各种细脉、细网脉特别发育，矿化为细脉-浸染状，含矿斑岩全岩矿化，少量矿化产于围岩中，矿化为铜-金组合。发育丰富的热液磁铁矿、赤铁矿、金红石等，铜、金沉淀与热液磁铁矿的形成关系密切；矿石矿物总体上为黄铜矿>斑铜矿>黄铁矿，黄铁矿很少，矿区内还发育丰富的石膏脉，说明母岩浆是高氧化性的。流体包裹体岩相学和显微测温结果显示高温阶段气相和含子矿物包裹体普遍共存，中高温阶段液相和气相包裹体共存，暗示流体沸腾可能是主要的成矿机制，成矿流体是直接从岩浆熔体中出溶（600~900°C）的具高氧化性、（超）高盐度的富含Cu、Au、S元素的岩浆流体。成岩成矿时代为早白垩世，系古特提斯洋闭合俯冲增生阶段的产物。     

Experimental study on liquid immiscibility of lamprophyre-sulfide melt at high temperature and high pressure and its geological significance

With lamprophyre and pyrite from the Laowangzhai gold deposit, Yunnan Province, China, as starting materials, and at pressures from 1.5 to 3.0 GPa and temperatures from 1160 to 1560℃ , an experimental study was carried out on the liquid immiscibility of lamprophyre-sulfide melt at high temperature and ultra-high pressure in the DS-29A cubic 3600T/6-type high pressure apparatus. Results showed that the liquid immiscibility of lampro-pyre-sulfide melt in the magmatic system would happen during the early magma...     

Magmatic evolution of Li–F, rare-metal granites: a case study of melt inclusions in the Khangilay complex, Eastern Transbaikalia (Russia)

We report compositions of homogenized quartz-hosted melt inclusions from a layered sequence of Li-, F-rich granites in the Khangilay complex that document the range of melt evolution from barren biotite granites to Ta-rich, lepidolite–amazonite–albite granites. The melt inclusions are crystalline at room temperature and were homogenized in a rapid-quench hydrothermal apparatus at 200 MPa before analysis. Homogenization runs determined solidus temperatures near 550 °C and full homogenization between 650 and 750 °C. The compositions of inclusions, determined by electron microprobe and Raman spectroscopy (for H₂O), show regular overall trends of increasing differentiation from the least-evolved Khangilay units to apical units in the Orlovka intrusion. Total volatile contents in the most-evolved melts reach over 11 wt.% (H₂O: 8.6 wt.%, F: 1.6 wt.%, B₂O₃: 1.5 wt.%). Concentrations of Rb range from about 1000 to 3600 ppm but other trace elements could not be measured reliably by electron microprobe. The resulting trends of melt evolution are similar to those described by the whole-rock samples, despite petrographic evidence for albite- and mica-rich segregations previously taken as evidence for post-magmatic metasomatism.

Melt variation trends in most samples are consistent with fractional crystallization as the main process of magma evolution and residual melt compositions plot at the granite minimum in the normative Qz–Ab–Or system. However, melts trapped in the highly evolved pegmatitic samples from Orlovka deviate from the minimum melt composition and show compositional variations in Al, Na and K that requires a different explanation. We suggest that unmixing of the late-stage residual melt into an aluminosilicate melt and a salt-rich dense aqueous fluid (hydrosaline melt) occurred. Experimental data show the effectiveness of this process to separate K (aluminosilicate melt) from Na (hydrosaline melt) and high mobility of the latter due to its low viscosity and relatively low density may explain local zones of albitization in the upper parts of the granite.     

Multiphase carbonate-salt immiscibility in carbonatite melts: data on melt inclusions from the Krestovskiy massif minerals (Polar Siberia)

Minerals of olivine–melilite and olivine–monticellite rocks from the Krestovskiy massif contain primary silicate-salt, carbonate-salt, and salt melt inclusions. Silicate-salt inclusions are present in perovskite I and melilite. Thermometric experiments conducted on these inclusions at 1,230–1,250°C showed silicate–carbonate liquid immiscibility. Globules of composite carbonate-salt melt rich in alkalies, P, S, and Cl separated in silicate melt. Carbonate salt globules in some inclusions from perovskite II at 1,190–1,200°C separated into immiscible liquid phases of simpler composition. Carbonate-salt and salt inclusions occur in monticellite, melilite, and garnet and homogenize at close temperatures (980–780°C). They contain alkalies, Ca, P, SO₃, Cl, and CO₂. According to the ratio of these components and predominance of one of them, melt inclusions are divided into 6 types: I—hyperalkaline (CaO/(Na₂O+K₂O)≤1) carbonate melts; II—moderately alkaline (CaO/(Na₂O+K₂O)>1) carbonate melts; III—sulfate-alkaline melts; IV—phosphate-alkaline melts; V—alkali-chloridic melts, and VI—calc-carbonate melts. Joint occurrence of all the above types and their syngenetic character were established. Some inclusions demonstrated carbonate-salt immiscibility phenomena at 840–800°C. A conclusion in made that the origin of carbonate melts during the formation of intrusion rocks is related to silicate–carbonate immiscibility in parental alkali-ultrabasic magma. The separated carbonate melt had a complex alkaline composition. Under unstable conditions the melt began to decompose into simpler immiscible fractions. Different types of carbonate-salt and salt inclusions seem to reflect the composition of these spatially isolated immiscible fractions. Liquid carbonate-salt immiscibility took place in a wide temperature range from 1,200–1,190°C to 800°C. The occurrence of this kind of processes under macroconditions might, most likely, cause the appearance of different types of immiscible carbonate-salt melts and lead to the formation of different types of carbonatites: alkali-phosphatic, alkali-sulfatic, alkali-chloridic, and, most widespread, calcitic ones.     

Anatexis and fluid regime of the deep continental crust: New clues from melt and fluid inclusions in metapelitic migmatites from Ivrea Zone (NW Italy)

We investigate the inclusions hosted in peritectic garnet from metapelitic migmatites of the Kinzigite Formation (Ivrea Zone, NW Italy) to evaluate the starting composition of the anatectic melt and fluid regime during anatexis throughout the upper amphibolite facies, transition, and granulite facies zones. Inclusions have negative crystal shapes, sizes from 2 to 10 μm and are regularly distributed in the core of the garnet. Microstructural and micro‐Raman investigations indicate the presence of two types of inclusions: crystallized silicate melt inclusions (i.e., nanogranitoids, NI), and fluid inclusions (FI). Microstructural evidence suggests that FI and NI coexist in the same cluster and are primary (i.e., were trapped simultaneously during garnet growth). FI have similar compositions in the three zones and comprise variable proportions of CO₂, CH₄, and N₂, commonly with siderite, pyrophyllite, and kaolinite, suggesting a COHN composition of the trapped fluid. The mineral assemblage in the NI contains K‐feldspar, plagioclase, quartz, biotite, muscovite, chlorite, graphite and, rarely, calcite. Polymorphs such as kumdykolite, cristobalite, tridymite, and less commonly kokchetavite, were also found. Rehomogenized NI from the different zones show that all the melts are leucogranitic but have slightly different compositions. In samples from the upper amphibolite facies, melts are less mafic (FeO + MgO = 2.0–3.4 wt%), contain 860–1700 ppm CO₂ and reach the highest H₂O contents (6.5–10 wt%). In the transition zone melts have intermediate H₂O (4.8–8.5 wt%), CO₂ (457–1534 ppm) and maficity (FeO + MgO = 2.3–3.9 wt%). In contrast, melts at granulite facies reach highest CaO, FeO + MgO (3.2–4.7 wt%), and CO₂ (up to 2,400 ppm), with H₂O contents comparable (5.4–8.3 wt%) to the other two zones. Our results represent the first clear evidence for carbonic fluid‐present melting in the Ivrea Zone. Anatexis of metapelites occurred through muscovite and biotite breakdown melting in the presence of a COH fluid, in a situation of fluid–melt immiscibility. The fluid is assumed to have been internally derived, produced initially by devolatilization of hydrous silicates in the graphitic protolith, then as a result of oxidation of carbon by consumption of Fe³⁺‐bearing biotite during melting. Variations in the compositions of the melts are interpreted to result from higher T of melting. The H₂O contents of the melts throughout the three zones are higher than usually assumed for initial H₂O contents of anatectic melts. The CO₂ contents are highest at granulite facies, and show that carbon‐contents of crustal magmas are not negligible at high T. The activity of H₂O of the fluid dissolved in granitic melts decreases with increasing metamorphic grade. Carbonic fluid‐present melting of the deep continental crust represents, together with hydrate‐breakdown melting reactions, an important process in the origin of crustal anatectic granitoids.     

Alkaline gabbroids of the Chirii outcrop (North Minusa depression): mineralogy and melt evolution

We studied the chemical composition of rock-forming minerals in gabbroids from the Chirii outcrop and the evolutionary features of parental basic melt during the crystallization of these rocks. Results were compared with data for basanites from pipes of the North Minusa depression. The mineralogical composition and thermobarogeochemical data of the gabbroids were examined in detail, and chemical analyses of rock-forming minerals (clinopyroxene, plagioclase, amphibole, biotite, titanomagnetite, and apatite) were carried out. Based on the homogenization temperatures of primary melt inclusions, we established the minimum temperatures and sequence of mineral crystallization in the gabbroids: clinopyroxene (>1160 °C), plagioclase, magnetite → amphibole (>950 °C) → biotite. The rock crystallization proceeded at shallow depths. Thermometric data are confirmed by results of modeling of equilibrium gabbroid crystallization. The crystallization of parental basic melt was accompanied by the accumulation of SiO₂, Al₂O₃, alkalies, and Cl and depletion in femic components. The melt evolved to granodiorite and alkali-syenite compositions. Compared with basanites from pipes, the parental melt had a longer evolution. The geochemical features of the gabbroids indicate that they, like basanites, crystallized from intraplate alkali-basaltoid magmas. But in petrochemistry and mineralogy the Chirii gabbroids differ considerably from the pipe basanites.     

长白山天池火山千年大喷发岩浆含水量研究——熔融包裹体含水量的红外光谱测试

长白山天池火山在公元一千年左右曾发生过大规模喷发,其产物为大面积分布的灰白色碱流质浮岩和碎屑流,在其斑晶矿物橄榄石、钙铁辉石和碱性长石中均可见到熔融包裹体。在最主要的斑晶矿物——碱性长石中含有数量众多且个体也较大的熔融包裹体,多数含有一个以上的气泡,其中部分含有子晶,根据形貌特征的不同可分为截然不同的两组包裹体。这些熔融包裹体带有大量喷发前地下岩浆的信息,成为研究地下深部的岩浆在复杂的溢流-爆炸喷发中所发生变化的最好媒介。也是本文的研究对象,通过其中挥发份尤其是水的含量,可以推知天池火山发生大喷发的原因。经Nicolet Magna-IR 550红外光谱仪测定,这些熔融包裹体的含水量较高,达1．6％-3．6％,为当时天池火山发生了巨大规模爆炸喷发的原因提供了强有力的证据。但目前红外光谱仪的应用范围还比较有限,有待今后拓宽其应用领域。     

Liquid immiscibility between silicate,carbonate and sulfide melts in melt inclusions hosted in co-precipitated minerals from Kerimasi volcano (Tanzania): evolution of carbonated nephelinitic magma

The evolution of a carbonated nephelinitic magma can be followed by the study of a statistically significant number of melt inclusions, entrapped in co-precipitated perovskite, nepheline and magnetite in a clinopyroxene- and nepheline-rich rock (afrikandite) from Kerimasi volcano (Tanzania). Temperatures are estimated to be 1,100°C for the early stage of the melt evolution of the magma, which formed the rock. During evolution, the magma became enriched in CaO, depleted in SiO₂ and Al₂O₃, resulting in immiscibility at ~1,050°C and crustal pressures (0.5–1 GPa) with the formation of three fluid-saturated melts: an alkali- and MgO-bearing, CaO- and FeO-rich silicate melt; an alkali- and F-bearing, CaO- and P₂O₅-rich carbonate melt; and a Cu–Fe sulfide melt. The sulfide and the carbonate melt could be physically separated from their silicate parent and form a Cu–Fe–S ore and a carbonatite rock. The separated carbonate melt could initially crystallize calciocarbonatite and ultimately become alkali rich in composition and similar to natrocarbonatite, demonstrating an evolution from nephelinite to natrocarbonatite through Ca-rich carbonatite magma. The distribution of major elements between perovskite-hosted coexisting immiscible silicate and carbonate melts shows strong partitioning of Ca, P and F relative to Fe_T, Si, Al, Mn, Ti and Mg in the carbonate melt, suggesting that immiscibility occurred at crustal pressures and plays a significant role in explaining the dominance of calciocarbonatites (sövites) relative to dolomitic or sideritic carbonatites. Our data suggest that Cu–Fe–S compositions are characteristic of immiscible sulfide melts originating from the parental silicate melts of alkaline silicate–carbonatite complexes.     

新疆西天山哈勒尕提铁铜矿床流体包裹体和氢氧同位素特征及其成矿意义

哈勒尕提铁铜矿床位于新疆西天山博罗科努多金属成矿带,矿体呈似层状、透镜状产于晚泥盆世中酸性侵入体与上奥陶统碳酸盐岩接触带上,是一个典型的矽卡岩矿床。本文从流体包裹体和氢氧同位素研究入手,讨论了成矿流体的特征、来源和演化及其与成矿的关系。岩相学观察表明,本矿床热液矿物中流体包裹体存在5种类型:富液相气液两相盐水包裹体(Ⅰ类)、含子矿物多相包裹体(Ⅱ类)、富气相气液两相盐水包裹体(Ⅲ类)、纯液相水包裹体(Ⅳ类)和纯气相水包裹体(Ⅴ类)。其中,Ⅰ类包裹体数量最多,各阶段热液矿物中均有发育;Ⅱ类包裹体数量较少,只见于进化交代蚀变阶段的石榴石和早退化阶段的绿帘石中;Ⅲ、Ⅳ和Ⅴ类包裹体数量最少,主要发育于晚退化阶段的石英和方解石中。流体包裹体显微测温表明,从进化交代蚀变阶段→早退化阶段→晚退化阶段,成矿流体经历了从高温(404~562℃)、中-高盐度(11.1%~51.6%NaC leqv)、中-低密度(0.47~0.80g/cm~3)到中-高温(207~465℃)、中-低盐度(2.9%~44.1%NaC leqv)、中-低密度(0.64~0.89g/cm~3)再到中-低温(117~337℃)、低盐度(1.6%~4.5%NaC leqv)、中-高密度(0.90~0.97g/cm~3)的演化过程。氢氧同位素研究表明,进化交代蚀变阶段和早退化阶段的成矿流体主要源于岩浆水,晚退化阶段则有大气降水的加入。根据流体包裹体岩相学特征,结合矿床宏观地质特征,认为流体不混溶(沸腾)是导致本矿区金属沉淀成矿的主要机制。     

矿物流体包裹体中稀有气体的保存能力初探

查明流体包裹体中稀有气体的保存能力,对于判断其初始组分特征是否因后生作用而发生改变具有重要意义.文章以Ar为例,从扩散动力学角度对稀有气体地球化学研究中常用的矿物中流体包裹体稀有气体的保存能力进行了定量分析和系统比较,计算了Ar在这些矿物中的封闭温度以及不同温度条件下的保存时间,得出相同条件下各矿物对Ar、He等保存能...