下地壳麻粒岩包体研究进展及其意义

产于火山岩中的下地壳麻粒岩包体是人们窥视深部地壳的一个窗口，现已成为人们探索大陆下地壳物质组成和演化最直接的研究对象。下地壳岩石包体一般具有麻粒岩相矿物组合，主体由镁铁质麻粒岩组成，以出现紫苏辉石矿物为标志下地壳包体的平衡温度为700－1040℃，平衡压力在0．8－1．4GPa之间。在绝大多数地区，基性下地壳包体占优势，其共同特征是低SiO2、高CaO和Mg^ ，过渡族元素和不相容元素含量变化很大，不机构造背景和不同岩石类型的包体同位素成分也有差异，全球各大陆下地壳包体Nd、Pb同位素组成分布具有“块体效应”特征。利用出露于地表的下地壳麻粒岩包体可以探讨下地壳物质组成和成分，建立下地壳物性剖面和岩石圈模型，并可作为幔源岩浆底侵作用的重要判据之一。世界范围内下地壳麻粒岩包体研究表明，在探讨下地壳的组成特点上，由火山岩中麻粒岩包体和出露的麻粒岩地体两类岩石样品所获得的下地壳组成特点存在比较大的差异，前者较后者反映的下地壳组成更偏基性。下地壳包体的类型与成因对揭示大陆地壳的增生、演化方式以及壳－幔交换作用具有重要的指示意义。     

下地壳麻粒岩包体研究进展及其意义

产于火山岩中的下地壳麻粒岩包体是人们窥视深部地壳的一个窗口 ,现已成为人们探索大陆下地壳物质组成和演化最直接的研究对象。下地壳岩石包体一般具有麻粒岩相矿物组合 ,主体由镁铁质麻粒岩组成 ,以出现紫苏辉石矿物为标志 ,下地壳包体的平衡温度为 70 0～10 4 0℃ ,平衡压力在 0 .8～ 1.4GPa之间。在绝大多数地区 ,基性下地壳包体占优势 ,其共同特征是低SiO2 、高CaO和Mg# ,过渡族元素和不相容元素含量变化很大 ,不同构造背景和不同岩石类型的包体同位素成分也有差异 ,全球各大陆下地壳包体Nd、Pb同位素组成分布具有“块体效应”特征。利用出露于地表的下地壳麻粒岩包体可以探讨下地壳物质组成和成分 ,建立下地壳物性剖面和岩石圈模型 ,并可作为幔源岩浆底侵作用的重要判据之一。世界范围内下地壳麻粒岩包体研究表明 ,在探讨下地壳的组成特点上 ,由火山岩中麻粒岩包体和出露的麻粒岩地体两类岩石样品所获得的下地壳组成特点存在比较大的差异 ,前者较后者反映的下地壳组成更偏基性。下地壳包体的类型与成因对揭示大陆地壳的增生、演化方式以及壳—幔交换作用具有重要的指示意义     

大别造山带现今地壳结构-岩石组成研究

通过大别造山带岩石地震波速的高温高压实验测定值与地震测深断面观察值的对比，结合地表出露岩石对深部岩石组成的地球化学示踪，揭示了该造山带现今地壳各结构层的基本岩石组成：上地壳主要由长英质岩石组成，榴辉岩在其中仅占0～20％；中地壳(低速层)主体由长英质片麻岩和花岗岩组成；下地壳上部由80％镁铁质麻粒岩和20％长英质麻粒岩组成；下地壳下部由幔源底侵岩浆作用形成的镁铁质麻粒岩组成。下地壳和上地幔的泊松比为0.265～0．280，明显高于榴辉岩的泊松比，表明其中即使有榴辉岩存在，含量也应极少。各构造单元出露的白垩纪花岗岩具有相似的化学组成，其铅、钕与锶同位素组成均可与北大别的核杂岩相对比，表明花岗岩浆均应以深部核杂岩为源岩。因此，被白垩纪花岗岩侵入的南大别超高压变质岩单元和宿松高压变质岩单元深部均应由核杂岩组成，亦即超高压和高压变质岩应呈拆离的构造岩片覆盖于核杂岩之上。鉴于白垩纪花岗岩的钕模式年龄(tDM)均集中于古元古代(1．8～2．2Ga)，表明花岗岩的源区应限于核杂岩中构成原中地壳下部的古元古代结晶基底岩层。这为中地壳主要由长英质片麻岩组成提供了佐证。考虑到大量花岗岩浆的抽出，应留下更大体积的镁铁质岩残留体，后者在地壳流变增厚调整过程中可能因密度增大而下沉，也可能因地震波速增大而显示下地壳的特征，更可能由于这两方面的原因而使由镁铁质残留体组成的原中地壳下部转变成现今下地壳上部的组成。根据大别碰撞后基性火山岩和侵入岩的地球化学研究，还可证明组成大别下地壳的镁铁质岩更可能是1.1Ga前而非中生代形成的底侵岩层。实践表明，上述两方面研究的结合可较好揭示区域地壳结构一组成。     

滇西地区下地壳铅同位素的组成及其意义

滇西地区新生代碱性侵入岩中广泛分布的麻粒岩包体可以代表该地区的下地壳岩石,为了确定滇西下地壳岩石的铅同位素组成,我们系统采集了该区碱性岩中的麻粒岩包体,挑选出其中的长石、石榴子石等造岩矿物,测定了其铅同位素组成,在Zartman等的铅构造演化模式图上,剔除个别异常的铅同位素组成,圈出投影于下地壳铅同位素演化趋势线上及附近的铅同位素分布范围,由此确定了该区下地壳的铅同位素组成的区域,并进一步结合作者先前确定的该区上地壳及上地幔铅同位素组成,构建了该区三维岩石圈铅同位素组成,并将这一结果用于滇西金顶超大型铅锌矿床的成矿物质来源的研究中,发现颇受争议的金顶铅锌矿床中的铅并非来自上地幔,而相当于下地壳来源的铅与兰坪盆地沉积岩铅二者的混合铅。     

制约深部大陆地壳物质成分与构造作用的地质证据

地震反射研究在深部陆构造认识取得了重要突破。区域麻粒岩区常具有下地壳的一般特征，代表上部地壳与最下部地壳之间的过渡区，记录了板垫托作用过程。许多麻粒岩区在深部地壳经历长期近等压冷却，最终上隆至地表常由与麻粒岩相变质无关的构造事件造事件造成，指示下地壳具有稳定性。其中，板底垫托的镁铁质岩浆岩根带可能是其难以出露地表关保持稳定的重要原因。对地表出露的地壳剖面的研究揭示了陆壳具有垂向分带特征，下地壳以麻     

汉诺坝新生代玄武岩中下地壳麻粒岩包体的变形显微构造特征及其地质意义

新生代玄武岩中的下地壳包体,由于从下地壳被快速携带至地表,因此保留了下地壳的直接信息.华北北部汉诺坝新生代玄武岩中除了含有丰富的幔源包体之外,还含有许多下地壳麻粒岩包体.本文的主要目的是通过对该区下地壳麻粒岩包体的变形显微构造和位错亚构造特征的详细研究,探讨下地壳的变形特征和变形机制.光学显微镜下观测表明,下地壳麻粒岩包体的低温(＜800℃)样品中确实发育显微破裂,但变形双晶、变形条带、扭折带也同样发育,动态重结晶作用也开始出现.随着温度、压力的升高,变形双晶、变形条带、变形纹、扭折带和重结晶新晶粒等塑性变形特征占主导地位,而显微破裂则主要表现为由塑性失配引起的显微破裂以及流体包裹体面.而明显不同于Ivrea带地体麻粒岩,在这些包体中未发现与韧性剪切有关的变形显微构造特征.透射电镜观测表明,包体中的斜长石和辉石颗粒普遍发育自由位错、位错列、亚晶界、新晶界、变形双晶、包裹体列和出溶片晶等位错亚构造.上述观测结果表明,下地壳变形作用以塑性变形为主而不是准脆性变形,其变形机制主要为位错的滑移和攀移机制,其中包括机械双晶作用和动态重结晶作用.     

湖南道县辉长岩包体的组构与波速各向异性研究及其意义

辉长岩包体的主要造岩矿物斜长石、单斜辉石的组构测定结果表明 :条带状辉长岩的斜长石组构为结晶b轴的优选定向 ,推测其成因是在重力作用占主导并伴有低应力的情况下形成的。宏观呈块状的辉长岩 ,在微观组构上仍有定向线理存在。经由组构、岩石密度、矿物组成计算得到的理论波速各向异性与实测波速得到的一致 ,从而表明地震波的各向异性对矿物组构的强烈依赖性。推测道县辉长岩包体的波速各向异性反映了下地壳地震波的一般特征。其组构特征反映了该区中、新生代下地壳的变形特征。     

花岗岩部分熔融及其对青藏高原南部地壳速度结构的约束

青藏高原南部地壳平均速度偏低和壳内广泛存在低速层是地壳物质组成、岩石物性状态和温度压力等综合因素在岩石弹性性质上的表现。依据岩石物理学和部分熔融实验获得的青藏高原南部地壳岩石弹性参数和熔体分布的结构信息,本文模拟青藏高原南部地壳岩石在不同的地温梯度条件下波速和密度随深度的变化,从而为探讨青藏高原南部地     

华北东部岩石圈减薄中的下地壳过程：岩浆底侵、置换与拆沉作用

最近研究表明，华北中生代岩石圈减薄不仅是岩石囤地幔减薄，而且下地壳也发生了一定程度的减薄和置换。本文强调下地壳过程，如岩浆底侵、置换和拆沉作用是理解岩石囤减薄机制的关键因素之一。火山岩及其捕虏体的信息似乎支持在华北东部南、北缘存在局部造山带型的下地壳与岩石囤的拆沉作用。但是华北东部整体上的减薄机制难以用造山带的拆沉模式来解释。华北东部克拉通内部的火山岩中的下地壳捕虏体有两类，一类是经历了麻粒岩相变质的底侵辉长岩和辉石岩以及榴辉岩相变质的石榴辉石岩，形成时代约在140～120Ma；另一类是经过了中生代变质叠加的前寒武纪麻粒岩。中生代华北东部曾发生过大规模的岩浆底侵作用，现今的下地壳很可能已大部分不是前寒武纪的下地壳，它们由中生代变质的辉长岩、镁铁质岩石以及经历了很强烈改造的前寒武纪下地壳麻粒岩组成。此外，在华北东部普遍存在着化学成分类似于“埃达克岩”的中生代高锶花岗岩类岩石，它们的形成与岩浆底侵作用和镁铁质下地壳的部分熔融有关，其熔融残留应是榴辉岩或石榴角闪岩。尽管如此，要通过下地壳部分熔融形成一个厚的密度很大的榴辉岩层，由它的重力不均衡来带动80～120公里厚的岩石圈地幔一起拆沉进入软流圈的机制很难发生在华北克拉通内部。岩浆底侵和置换作用是下地壳过程非常重要的形式，与岩石圈的减薄具有密切联系，其具体机制尚不完善。     

火成岩中下地壳岩石包体的特征及其研究意义

根据国内外研究资料，结合自己的科研成果，简要论述了下地壳岩石包体的矿物学，形成条件，物理性质，化学成分，同位素组成及塑性变形特征，讨论了下地壳岩石包体在了解下地壳成分，性质和地质作用过程方面的重要意义。     

Granulite xenoliths from western Saudi Arabia: the lower crust of the late Precambrian Arbian-Nubian Shield

Mafic and intermediate granulite xenoliths, collected from Cenozoic alkali basalts, provide samples of the lower crust in western Saudi Arabia. The xenoliths are metaigneous two-pyroxene and garnet granulites. Mineral and whole rock compositions are inconsistent with origin from Red Sea rift-related basalts, and are compatible with origin from island arc calc-alkaline and low-potassium tholeiitic basalts. Most of the samples are either cumulates from mafic magmas or are restites remaining after partial melting of intermediate rocks and extraction of a felsic liquid. Initial⁸⁷Sr/⁸⁶Sr ratios are less than 0.7032, except for two samples at 0.7049. The Sm-Nd data yield T_DM model ages of 0.64 to 1.02 Ga, similar to typical Arabian-Nubian Shield upper continental crust. The isotopic data indicate that the granulites formed from mantle-derived magmas with little or no contamination by older continent crust. Calculated temperatures and pressures of last reequilibration of the xenoliths show that they are derived from the lower crust. Calculated depths of origin and calculated seismic velocities for the xenoliths are in excellent agreement with the crustal structure model of Gettings et al. (1986) based on geophysical data from western Saudi Arabia. Estimation of mean lower crustal composition, using the granulite xenoliths and the Gettings et al. (1986) crustal model, suggests a remarkably homogeneous mafic lower crust, and an andesite or basaltic andesite bulk composition for Pan-African juvenile continental crust.     

Geochronology, petrology and geochemistry of the granulite xenoliths from Nushan, east China: implication for a heterogeneous lower crust beneath the Sino-Korean Craton

The occurrence of both Archean granulite terrains and granulite xenoliths in Cenozoic basalts from the Sino-Korean Craton (SKC) provides an ideal opportunity to define composition and evolution of continental lower crust of eastern China. The granulite xenoliths in Quaternary basanites from Nushan (southeastern SKC) show a basic-intermediate composition that is distinctly different from mafic granulites from Hannuoba (western SKC). They instead resemble the Archean granulite terrains in terms of mineral and whole rock compositions. Trace element modeling suggests that the “protoliths” of the Nushan granulites were likely subjected to fractional crystallization and assimilation of old crustal components. Zircon SHRIMP U-Pb dating shows at least two episodes in the formation of the lower crust at Nushan. The protoliths of the Nushan granulites were most likely formed at ca. 2.5 Ga and metamorphosed at 1.9 Ga. This late Archean crustal growth was followed by Mesozoic (∼140 Ma) basaltic underplating, which was probably coeval with the widespread thermo-tectonic lithospheric reactivation in eastern China. The Nushan granulites are therefore interpreted as dominantly derived from the late Archean crystalline basement and subordinately from the mafic layer that was accreted to the basement during late Mesozoic lithospheric thinning. The consistencies between the depth to seismic Moho and the depth to crust-mantle boundary, and between the calculated V_p (mostly < 7.0 km/s) for granulite xenoliths and the observed velocity structure strongly suggest no obvious high-velocity lowermost crust beneath Nushan and the granulite xenoliths as the dominant components in the lower crust at this locality. The modeled composition of the Nushan lower crust has SiO₂ of ca. 52%, which is more basic than that at Hannuoba (SiO₂ ≈ 58%, Liu et al., 2001). Such a compositional difference, in conjunction with contrasting age and seismic velocity structure of the lower crust at the two localities, highlights two fundamentally distinct tectonic domains in the SKC. The data presented in this study also yield implication for the origin of the compositional difference between granulite xenoliths and terrains.     

拉萨地体东南部整体地壳成分及其成因分析

造山带地壳结构和成分的基本特征对于认识大陆地壳成分演化和区域成矿背景具有重要意义.综合青藏高原拉萨地体东南部地球物理、高温高压岩石物性和岩浆岩地球化学资料,分析该地区地壳整体成分特征,并探讨其可能成因.该地区平均地壳波速显著低于全球大陆和造山带地壳的平均值,表明地壳整体具有中酸性成分,下地壳特征也可由中性岩石(残余体性质的中性含石榴石麻粒岩)解释.拉萨地体东南部整体地壳成分特征应与多阶段长英质化有关,包括碰撞前大陆弧演化阶段(以堆晶或残余体下地壳拆沉为主)和碰撞后高原垮塌阶段(以加厚下地壳拆沉为主,伴随印度古老长英质陆壳物质的俯冲回返/构造底侵).拉萨地体是研究大陆地壳成分演化的绝佳区域,亟待进一步开展多学科综合研究.     

Links between Mesozoic intermediate–felsic igneous rocks and lower crustal granulite xenoliths,North China Craton: O and Pb isotopic evidence

We present and compare whole-rock and zircon O and Pb isotopic compositions for the Hannuoba granulite xenoliths and Mesozoic intermediate-to-felsic igneous rocks from the Zhangjiakou region, northern margin of the North China Craton, northeast China. The xenoliths have an overall Pb isotopic range similar to rocks from the regionally exposed Neoarchaean granulite terrain. Mesozoic zircons from different types of granulite xenoliths have a narrow range of δ¹⁸O values (6.0–7.7‰) higher than normal mantle δ¹⁸O values (～5.7‰). Mesozoic intermediate–felsic igneous rocks have O and Pb isotopic compositions indistinguishable from the Hannuoba intermediate–mafic granulite xenoliths. Our new data suggest that the Mesozoic igneous rocks and granulite xenoliths are genetically linked and that both were derived from the late Neoarchaean lower crust. This argues against previous proposals that the granulite xenoliths are either products of Mesozoic basaltic underplating or formed by mixing between mantle-derived and pre-existing crustal magmas.     

汉诺坝捕虏体辉石岩和麻粒岩的成因探讨

汉诺坝新生代玄武岩中含有丰富的地幔和地壳岩石捕虏体,其中捕虏体辉石岩和庥粒岩由于外观上具有一定的相似性,两者容易混淆,导致研究上的误区.本文以辉石岩和麻粒岩捕虏体作为研究对象,通过岩相学观察结合矿物主量元素分析、单斜辉石微量元素和Sr-Nd同位素分析,对两种捕虏体进行深入的研究和对比以探讨其成因意义.结果表明,上述各方面二者都存在明显的差别,捕虏体麻粒岩具有层状堆晶构造,两种辉石矿物(次透辉石和古铜辉石)相对贫MgO富FeO,单斜辉石的REE相对富集,以高87Sr/86 Sr低143Nd/144Nd为特征;而捕虏体辉石岩一般呈块状构造,两种辉石矿物(透辉石和古铜辉石-顽火辉石)相对富MgO贫FeO,单斜辉石REE总量极低呈亏损模式,同位素组成上介于捕虏体橄榄岩和麻粒岩之间.捕虏体麻粒岩特征表明它是幔源岩浆底侵作用形成,岩浆受到了下地壳的混染;而捕虏体辉石岩明显不同于橄榄岩和麻粒岩的成因,来自于富集地幔.     

A composite geologic and seismic profile beneath the southern Rio Grande rift, New Mexico, based on xenolith mineralogy, temperature, and pressure

A complete understanding of the processes of crustal growth and recycling in the earth remains elusive, in part because data on rock composition at depth is scarce. Seismic velocities can provide additional information about lithospheric composition and structure, however, the relationship between velocity and rock type is not unique. The diverse xenolith suite from the Potrillo volcanic field in the southern Rio Grande rift, together with velocity models derived from reflection and refraction data in the area, offers an opportunity to place constraints on the composition of the crust and upper mantle from the surface to depths of  60 km. In this work, we calculate seismic velocities of crustal and mantle xenoliths using modal mineralogy, mineral compositions, pressure and temperature estimates, and elasticity data. The pressure, temperature, and velocity estimates from xenoliths are then combined with sonic logs and stratigraphy estimated from drill cores and surface geology to produce a geologic and velocity profile through the crust and upper mantle. Lower crustal xenoliths include garnet ± sillimanite granulite, two-pyroxene granulite, charnokite, and anorthosite. Metagabbro and amphibolite account for only a small fraction of the lower crustal xenoliths, suggesting that a basaltic underplate at the crust–mantle boundary is not present beneath the southern Rio Grande rift. Abundant mid-crustal felsic to mafic igneous xenoliths, however, suggest that plutonic rocks are common in the middle crust and were intraplated rather than underplated during the Cenozoic. Calculated velocities for garnet granulite are between  6.9 and 8.0 km/s, depending on garnet content. Granulites are strongly foliated and lineated and should be seismically anisotropic. These results suggest that velocities > 7.0 km/s and a layered structure, which are often attributed to underplated mafic rocks, can also be characteristic of alternating garnet-rich and garnet-poor metasedimentary rocks. Because the lower crust appears to be composed largely of metasedimentary granulite, which requires deep burial of upper crustal materials, we suggest the initial construction of the continental crust beneath the Potrillo volcanic field occurred by thickening of supracrustal material in the absence of large scale magmatic accretion. Mantle xenoliths include spinel lherzolite and harzburgite, dunite, and clinopyroxenite. Calculated P-wave velocities for peridotites range from 7.75 km/s to 7.89 km/s, with an average of 7.82 km/s. This velocity is in good agreement with refraction and reflection studies that report P_n velocities of 7.6–7.8 km/s throughout most of the Rio Grande rift. These calculations suggest that the low P_n velocities compared to average uppermost mantle are the result of relatively high temperatures and low pressures due to thin crust, as well as a fertile, Fe-rich, bulk upper mantle composition. Partial melt or metasomatic hydration of the mantle lithosphere are not needed to produce the observed P_n velocities.     

Accretion of juvenile crust at the Early Palaeozoic Antarctic margin of Gondwana: geochemical and geochronological evidence from granulite xenoliths

Geodynamic models for the Antarctic sector of the active Early Palaeozoic Palaeo-Pacific margin of Gondwana are based on the nature and age of the deep crust of the Robertson Bay terrane, the outermost lithotectonic unit of the margin. As this crustal block is covered with thick turbidite deposits, the only way to probe the deep crust is through the analysis of granulite xenoliths from Cenozoic scoria cones. Low-K felsic xenoliths yield the oldest (Middle Cambrian) laser-probe U–Pb ages on zircon areas with igneous growth zoning. This finding, along with the positive whole-rock ε_Nd(500Ma), suggests that these felsic rocks derived from a juvenile magma formed during the Early Palaeozoic Ross orogenic cycle. Mafic xenoliths have geochemical-isotopic compositions similar to those of modern primitive island arcs, suggesting the involvement of subducted oceanic crust in their magma genesis and accretion of juvenile crust at the Antarctic margin of Gondwana.     

Derivation of Mesozoic adakitic magmas from ancient lower crust in the North China craton

Three Mesozoic plutons were intruded into the Archean granulite terrains in northern margin of the North China craton adjacent to the granulite xenolith-bearing Tertiary Hannuoba basalts. They are Triassic Guzuizi and Honghualiang granites and Early Cretaceous Zhuanzhilian diorite. Rocks of the three intrusions are characterized by high Sr (576-1216 ppm) and Na₂O (?4.0%), low Y (?18 ppm) and heavy rare-earth elements (Yb < 1.8 ppm). These features are similar to modern adakites (siliceous rocks with high sodium, aluminum and strontium and low heavy rare-earth element and yttrium contents) from island arcs and Archean high-Al tonalite-trondhjemite-granodiorite (TTG). However, they are distinctly potassium-rich and their evolved strontium, neodymium, and hafnium isotopic compositions and inherited zircon ages coincide with those of the Archean granulites and the Hannuoba granulite xenoliths. Such features cannot readily be explained with previous models of the origin of adakites and TTGs. We propose that these adakitic rocks are formed by partial melting of ancient lower crust, and that the restites are represented by some of the Hannuoba granulite xenoliths; we further argue that this could be one major mechanism to generate voluminous Mesozoic adakitic magmas in the eastern North China craton. Our hypothesis can also explain the discrepancies in ages and compositions between the granulite terrains and xenoliths, and implies that crustal anatexis may be one of the major processes controlling the chemical differentiation of the continental crust.     

榴辉岩的地震波性质：对苏鲁超高压变质带地壳成分和折返机制的探讨

本文总结了榴辉岩的高温高压弹性波速测量结果,并将其应用于苏鲁超高压变质带地震资料的解释。由于榴辉岩具有高密度和高波速,它们和长英质片麻岩、大理岩、石英岩、角闪岩、麻粒岩、蛇纹石化橄榄岩的界面可以产生强反射。如果俯冲的陆壳物质以榴辉岩与围岩互层的形式在上地幔保留下来,就可能在造山带的上地幔产生地震反射。根据CCSD孔区地震剖面所建立的地壳成分模型表明:苏鲁超高压带地壳浅部的高速层可归因于夹在花岗质片麻岩、副片麻岩、角闪岩等岩石中的榴辉岩和超基性岩;中地壳主要由中酸性片麻岩、斜长角闪岩和副片麻岩组成;下地壳以中基性麻粒岩为主。在该超高压变质带现今的深部地壳,榴辉岩含量很少或几乎没有。因此,折返的超高压变质岩是以构造岩片的形式沿一系列剪切带逆冲并覆盖在正常的中下地壳之上,深部榴辉岩的缺乏可能与下地壳拆沉作用无关。     

滇西腾冲地块新生代火山岩中高温麻粒岩包体的发现及成因

腾冲地块芒棒乡新生代新近纪芒棒组火山岩的研究,发现粗面安山岩中含有较多麻粒岩包体,主要类型为长英质麻粒岩和二辉麻粒岩,直径一般为3~5 cm,略具定向排列构造,粒状变晶结构特征.长英质麻粒岩包体平衡温度和压力为:869~969 ℃,0.94~1.00 GPa,二辉麻粒岩包体平衡温度为:841~972 ℃,均显示为高温麻粒岩相变质;寄主岩粗面安山岩中斑晶结晶估算的温度和压力为:1 008~1 059 ℃,1.26~1.33 GPa,表明它们形成和起源于下地壳到上地幔顶部之间.二辉麻粒岩包体电子背散射衍射(EBSD)显微组构分析表明,斜方辉石(紫苏辉石)和单斜辉石(普通辉石)均具有明显晶格优选方位(LPO),斜方辉石和单斜辉石主滑移系分别为:(010)[001]和(100)[001]、(010)[001],变形机制为位错蠕变,说明麻粒岩包体经历了高温塑性变形变质作用.新生代新近纪火山岩中高温麻粒岩的发现和研究表明,腾冲新生代岩浆活动可能与印度板块和腾冲地块俯冲-碰撞造山后的伸展垮塌-拆沉和板片断离,以及随后的上地幔物质上涌减压熔融产生玄武质岩浆底侵,导致的下地壳发生高温变质及火山岩浆作用有密切关系.