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1.
岩石的物理性质(弹性、电性等)明显受熔体连通性的制约.因此,研究熔体分布对理解深部地质作用、理解地球物理资料具有特殊意义.于高温高压条件下(T＝850-1100,p＝2.0-4.0GPa)在YJ3000吨六面顶砧压机上进行了三然块状斜长角闪岩的脱水部分熔融实验,测量了熔体与矿物相接触时所形成的二面角值.结果表明,熔体在低熔体系下(熔体体积百分比为5%),熔体以熔体薄膜形式存在于矿物相边界,二面角值<60℃时,熔体相互连通;不同固相矿物的二面角的颁有两个驱动力.通过测量二面角值可定性确定熔体的连通性及熔体连通的动力学制. 相似文献
2.
在采用天然基性岩样品进行的流变实验中,存在因实验温度低而样品处于半脆性变形域与因实验温度高而样品颗粒边界出现熔体的矛盾。文献中给出的流变参数中,应力指数n的可靠性高,具有良好的重复性,激活能Q在一定范围内具有重复性,而系数A重复性差。采用6种样品进行流变实验。结果表明,矿物成分对岩石流变的影响比根据端员组分确定的双组分和多组分岩石流变物理模型要复杂得多。由斜长石、单斜辉石和角闪石组成的样品中,当斜长石和单斜辉石含量接近,而角闪石含量低于10%,斜长石和单斜辉石控制了岩石的流变;如果样品中有超过10%的角闪石参与流变,角闪石在变形中所起作用非常显著。由斜长石、石英和角闪石组成的样品,当石英含量小于10%而斜长石和角闪石含量接近时,斜长石和角闪石控制了岩石的流变;当斜长石含量达到70%时,样品变形更接近长石特性;如果石英含量超过20%时,石英在变形中起到主要作用。选择与基性麻粒岩中主要矿物成分接近的天然辉长岩(辉绿岩),或者从天然基性麻粒岩中挑选出主要矿物,通过热压合成人工样品,进行高温流变实验是研究基性麻粒岩流变的最有效途径。 相似文献
3.
单斜辉石作为大陆下地壳以及上地幔岩石的重要组成矿物,其在高温高压条件下的流变行为已有大量的实验研究。本文在综述以往对单斜辉石流变实验研究的基础上,讨论了影响其流变行为的各种因素及其地质意义,并指出了现存的问题及今后的研究趋势。影响单斜辉石流变性质的因素主要有流体（包括水和熔体）、粒度、化学成分、氧逸度以及温度与压力条件等。微量结构水可以显著增大单斜辉石单晶和多晶集合体的蠕变速率,降低其流变强度。熔体对单斜辉石强度的影响与熔体的含量和分布状态有关,呈三联点分布于矿物颗粒间的熔体对样品强度影响较小,只有当熔体呈薄膜状湿润颗粒边界时,熔体的弱化作用才显著。粒度主要影响单斜辉石的变形机制,单斜辉石集合体晶粒粒度的减小会促使变形机制由位错蠕变转变为扩散蠕变,较细粒的单斜辉石在扩散蠕变域内的应力与粒度呈线性负相关,而在位错蠕变域,应力与粒度无明显相关性。关于铁含量对单斜辉石的影响尚未有直接的实验研究,而对比前人在相同实验条件下采用不同铁含量的单斜辉石的扩散蠕变实验研究显示,单斜辉石中铁含量与蠕变速率可能呈正相关。氧逸度的升高对单斜辉石单晶的蠕变强度有轻微的弱化作用,而关于氧逸度对单斜辉石集合体流变... 相似文献
4.
高温高压条件下实验变形石英闪长岩微观结构与熔体特征研究 总被引：1，自引：0，他引：1
本文以高温高压条件下石英闪长岩流变实验样品为研究对象,利用偏光显微镜进行微观结构观察,研究了样品在实验温度压力条件下的变形机制与斜长石结构对流变强度的影响;通过透射电镜能谱与电子探针,分析了熔体分布和成分特征,讨论了角闪石脱水熔融的影响因素与脱水熔融对岩石流变的影响。结果表明,随着温度升高,岩石从脆塑性过渡域逐渐向高温位错攀移和动态重结晶为主的塑性域转化。在高温条件下,角闪石出现了脱水与部分熔融,脱水熔融的熔体分布和成分体现出非均匀与非平衡熔融的特点,空间分布上,熔体主要出现在角闪石和黑云母矿物颗粒的边缘以及角闪石和长石颗粒之间的区域内;成分分布上,熔体的成分与参与熔融的矿物成分密切相关。角闪石边缘的熔体和黑云母边缘的熔体具有低硅铝、高铁镁特征,斜长石边缘的熔体具有高硅铝、低铁镁的特征,处于角闪石和斜长石颗粒中间的熔体,其成分间于斜长石与角闪石成分之间。实验中出现的非平衡非均匀部分熔融可以解释混合岩中的浅色体与暗色体的成因,富硅熔体可以形成富硅铝的花岗质岩石,而贫硅富铁镁的熔体可以形成基性岩。角闪石的脱水熔融程度依赖于样品的封闭条件,处于封闭环境的样品,角闪石不易脱水熔融,而处于开放环境时,角闪石脱水熔融显著。拆离断层带及其附近具备这样的开放环境,有利于角闪石发生脱水熔融。实验力学数据和微观结构显示,随机分布的斜长石对岩石强度影响并不明显,但斜长石的长轴方向与最大主应力方向呈大角度相交(近90°)会显著强化岩石的强度,这意味着岩石组构与主应力方向大角度相交或呈垂直方向时,不利于岩石变形和拆离断层的形成,反之,均匀岩石或岩石组构与最大主应力方向小角度相交,有利于岩石的变形,容易发育拆离断层。 相似文献
5.
在YJ3000t高压装置上,利用超声波脉冲透射-反射法测量恒压0.6GPa,1.0GPa和2.0GPa,室温至1 195℃条件下斜长角闪岩的纵波波速(Vp),统计了实验中间产物中各组分的体积百分含量和熔体形态(二面角),并根据主要矿物含量和弹性参数,利用VRH平均模型计算了高温高压下斜长角闪岩的Vp。结果显示,不同压力下,样品的Vp随温度升高首先缓慢降低,在温度达约850℃～950℃时转而快速下降。实验产物观测显示,随温度升高熔体含量显著增加,二面角不断减小,熔体由封闭囊状演变为连通薄膜,部分熔融是导致岩石Vp快速降低的主要因素。高温高压下Vp计算结果与测量结果有相同的Vp-T变化趋势,其对比研究表明,岩石初始熔融时,熔体尚未连通,此时熔体含量控制着岩石Vp的降低。部分熔融加剧导致熔体逐渐连通,此时不同压力下熔体导致Vp下降有差异,这可能与熔体连通过程中熔体薄膜的形态因子变化有关。 相似文献
6.
7.
部分熔融与高级变质岩流变机制——以内蒙古大青山高级变质岩为例 总被引：5，自引：0，他引：5
部分熔融作用与高级变质岩变形作用是相互制约,变形作用能够提高岩石部分熔融程度,降低熔融温度。熔体存在影响和制约岩石强度和变形机制。大青山高级岩经历了下部地壳构造层次变质变形和深熔作用改造,形成了复杂构造要素组合。宏观与微观构造特点表明:高级变质岩变形机制主要为熔体增强颗粒边界扩散和颗粒流动,使岩石发生大规模的塑性流动。在宏观上形成了不对称流动组构、熔融线理、岩石和矿物条带、层内底辟褶皱和大型穹窿构造。但是,在微观上矿物颗粒变形不明显,晶内变形组构不发育,表现为三边平衡结构,与静态结晶变质岩结构相似,形成了地壳深部构造层次上变质构造岩-构造片麻岩。 相似文献
8.
要想建立流体和熔体分凝的动力学模式就需要了解地球物质在部分熔融时的物理性质。在高温流变的情况下,稳定态的物理特性是由颗粒般大小的熔体相的准平衡分布决定的。熔融时流变相的影响主要是增加扩散变形(牛顿式)的动力;而且在所有的颗粒边界被熔体模式所取代而建立准平衡时影响最大。这种情形在实验室或天然硅酸盐部分熔融的样品中至今还未见到。所见到的“普通”熔体的形态是一种沿着三个颗粒交汇点和无熔体的颗 相似文献
9.
利用超声波透射-反射法,测量了0.6～2.0 GPa、最高1 085℃条件下角闪辉长岩的纵波波速(vp),详细统计了部分熔融阶段实验产物组分的体积百分含量,利用矿物含量和弹性参数,计算了角闪辉长岩的纵波波速.实验测量和理论计算显示了较一致的vp-t关系,即高压下角闪辉长岩的vp随温度升高先缓慢降低,在温度约800～900℃后转而大幅下降.实验产物显示,样品在温度达812℃(0.6 GPa)、865℃(1.0 GPa)和919℃(2.0 GPa)后发生矿物脱水和部分熔融,熔体含量随温度升高显著增加.熔体是导致高温阶段岩石vp快速降低的主要原因.在初熔阶段vp随熔体增加而降低尤为显著,可能是初熔时矿物脱水生成的自由水及含水量高的熔体,以微细熔体薄膜浸润矿物边界或裂隙所导致. 相似文献
10.
本文在高温高压条件下,开展了辉长岩矿物反应与部分熔融实验,利用偏光显微镜与扫描电镜对实验样品微观结构观察,研究实验中的新生矿物与熔体的分布;通过电子探针分析熔体成分特征。实验结果表明,在低压(300MPa)条件下,静压和塑性变形实验样品中,单斜辉石以固体反应方式生成橄榄石,在高压(1300MPa)塑性实验中所有实验样品都没有发现新生矿物颗粒,这与相图中低压条件下斜长石与橄榄石稳定共存,而高压下斜长石-辉石稳定共存相吻合。高压塑性变形条件下,单斜辉石和黑云母首先发生部分熔融,随着温度增高,斜长石逐渐参与熔融,熔体呈薄膜状分布在矿物颗粒边界,熔体成分依赖于参与熔融的矿物成分,表明出现的熔体为非平衡熔融结果。 相似文献
11.
T. Hiraga I. Anderson M. Zimmerman S. Mei D. Kohlstedt 《Contributions to Mineralogy and Petrology》2002,144(2):163-175
Olivine grain boundaries in deformed aggregates of olivine + basalt and partially molten lherzolite were analyzed with various electron microscopy techniques to test for the presence of thin (0.5-10 nm) intergranular melt films. High-resolution transmission electron microscopy (HREM) observations reveal that most of the boundaries do not contain a thin amorphous phase, although a small fraction of grains are separated by relatively thick (~1 µm) layers of melt. However, due to the anisotropy of the olivine-melt interfacial energy, melt often tapers from a triple junction into an adjoining grain boundary over a length of 1 to 2 µm, giving an effective dihedral angle of only ~2°. The chemistry of olivine-olivine grain boundaries was analyzed using energy dispersive X-ray (EDX) profiling by scanning transmission electron microscopy (STEM) with a probe size of <1.5 nm. Ca, Al and Ti segregate to grain boundaries forming enriched regions of <7 nm width. Although these elements are concentrated in the glass phases, the presence of glass films with the same chemical composition as the bulk glass phases cannot explain concentrations of other elements such as Si and Al at the boundaries. Combined with the HREM results, the STEM/EDX profiling demonstrates the existence of chemical segregation between solid grains but the absence of thin, grain boundary melt films. Additionally, if melt films exist along all of the grain boundaries, as reported for similar samples by other groups, the rock should be substantially weakened. Creep experiments on the partially molten rocks analyzed in this study reveal little weakening at small melt contents, consistent with our observations of melt-free grain boundaries. 相似文献
12.
A close look at dihedral angles and melt geometry in olivine-basalt aggregates: a TEM study 总被引：4，自引：0，他引：4
Martin Cmíral John D. Fitz Gerald Ulrich H. Faul David H. Green 《Contributions to Mineralogy and Petrology》1998,130(3-4):336-345
Olivine-basalt aggregates sintered at high P/T have been used as a simplest approximation of partially molten upper mantle peridotite. In the past, geometry of partial
melt in polycrystalline olivine (and other materials) has been characterised by dihedral (wetting) angles which depend upon
surface free energy. However, since olivine (like most other crystalline materials) is distinctively anisotropic, the simple
surface energy balance defining the dihedral angles cos(Θ/2)=gb/2sl is not valid and melt geometry is more complicated than can be expressed by a single dihedral angle value. We examine in
detail melt geometry in aggregates held at high temperature and pressure for very long times (240–612 h). We show the simple
dihedral angle concept to be invalid via transmission electron microscope images. Olivine-basalt interfaces are frequently
planar crystal faces (F-faces) which are controlled by the crystal structure rather than the surface area minimisation used
in the simple dihedral angle concept. Nevertheless, the dihedral angles may provide useful insights in some situations. They
may give a rough estimation of the wetting behaviour of a system, or be used to approximate the melt distribution if F-faces
are not present (possibly at large grain size and very low melt fraction). Our measurements, excluding F-faces, give a range
of dihedral angle values from 0 to 10° which is significantly lower than reported previously (20–50°). The nature of 0° angles
(films and layers up to 1 μm in thickness) is unclear but their frequency compared to dry grain boundaries depends on grain
size and melt fraction (e.g. 70% for grain size 43 μm and melt fraction 2%).
Received: 13 April 1997 / Accepted: 2 October 1997 相似文献
13.
In polycrystalline aggregates of olivine with mean grain sizes above 35 μm plus a low basaltic melt fraction, both wetted
and melt-free grain boundaries are observed after equilibration times at high pressures and temperatures of between 15 and
25 days. In order to assess a possible dependence of the wetting behaviour on the relative orientation of neighbouring grains,
a SEM based technique, electron backscatter diffraction (EBSD), is used to determine grain orientations. From the grain orientations
relative orientations of neighbouring grains are calculated, which are expressed as misorientation axis/angle pairs. The distribution
of misorientation angles and axes of melt-free grain boundaries differ significantly from a purely random distribution, whereas
those of wetted grain boundaries are statistically indistinguishable from the random distribution. The relative orientation
of two neighbouring grains therefore influences the character of their common grain boundary. However, no clustering towards
special (coincident site lattice) misorientation axes is observed, with the inference that the energy differences between
special and general misorientations are too small to lead to the development of preferred misorientations during grain growth.
Received: 8 December 1997 / Revised, accepted: 6 April 1998 相似文献
14.
The texture, distribution, and infiltration tendency of a quartz-albite melt in equilibrium with a synthetic, texturally-equilibrated quartzite was examined in a series of distribution and infiltration experiments at 1,250° C and 8 kbar hydrostatic pressure. Wetting angle measurements from melt distribution experiments show a dihedral angle () of 60 degrees, implying a quartz/quartz interfacial energy approximately 1.7 times the quartz/melt value. Because of this specific relationship between interfacial energies, the system can achieve its lowest surface free energy state with the melt either in pools or along grain edge intersections, possibly forming some interconnected channels. Stability of melt in pockets and along grain edge intersections was observed in a fourteen-day, dispersed-melt experiment, yet melt pools failed to disperse into the quartzite during infiltration experiments. Comparison of the observed dihedral angle with previously measured surface energy values for the melt and quartz shows excellent agreement, and also demonstrates that an aggregate of randomly orientated anisotropic grains acts approximately isotropically.While these experiments are not strictly applicable to real crustal systems, they do indicate that, at least in some felsic systems, the melt has no preference for uniform grainedge wetting relative to collection at grain corners or in large pools. This ambivalent behavior is attributable to the 60-degree wetting angle, which has been shown to separate systems in which melt tends to disperse in interconnected channels (<60°) from those in which melt tends to become isolated at grain corners (> 60°). 相似文献
15.
Catherine A. Stuart Sandra Piazolo Nathan R. Daczko 《Journal of Metamorphic Geology》2018,36(8):1049-1069
High‐strain zones are potential pathways of melt migration through the crust. However, the identification of melt‐present high‐strain deformation is commonly limited to cases where the interpreted volume of melt “frozen” within the high‐strain zone is high (>10%). In this contribution, we examine high‐strain zones in the Pembroke Granulite, an otherwise low‐strain outcrop of volcanic arc lower crust exposed in Fiordland, New Zealand. These high‐strain zones display compositional layering, flaser‐shaped mineral grains, and closely spaced foliation planes indicative of high‐strain deformation. Asymmetric leucosome surrounding peritectic garnet grains suggest deformation was synchronous with minor amounts of in situ partial melting. High‐strain zones lack typical mylonite microstructures and instead display typical equilibrium microstructures, such as straight grain boundaries, 120° triple junctions, and subhedral grain shapes. We identify five key microstructures indicative of the former presence of melt within the high‐strain zones: (a) small dihedral angles of interstitial phases; (b) elongate interstitial grains; (c) small aggregates of quartz grains with xenomorphic plagioclase grains connected in three dimensions; (d) fine‐grained, K‐feldspar bearing, multiphase aggregates with or without augite rims; and (e) mm‐ to cm‐scale felsic dykelets. Preservation of key microstructures indicates that deformation ceased as conditions crossed the solidus, breaking the positive feedback loop between deformation and the presence of melt. We propose that microstructures indicative of the former presence of melt, such as the five identified above, may be used as a tool for recognising rocks formed during melt‐present high‐strain deformation where low (<5%) volumes of leucosome are “frozen” within the high‐strain zone. 相似文献
16.
Takashi Yoshino Jonathan D. Price David A. Wark E. Bruce Watson 《Contributions to Mineralogy and Petrology》2006,152(2):169-186
The pore geometry of texturally equilibrated rocks is controlled by the interfacial energy ratio between grain boundaries and solid–liquid boundaries. Faceting at pore walls, which is a common feature of pore networks in rocks, strongly affects the liquid distribution. We investigated the effects of faceting on the equilibrium pore geometries based on image analysis of several systems with various degrees of faceting and dihedral angles. The degree of faceting was assessed by the F value, which is the ratio of the flat interface length at the pore wall to the length of total interfacial boundary between solid and liquid. The F values tend to increase with increasing liquid volume fraction. Little-faceted systems show relatively homogeneous liquid distribution. Moderately-faceted systems with a higher dihedral angle (∼55°) are characterized by development of large pores surrounded by faceted walls and complementary shrinkage of triple junction tubes, whereas strongly faceted systems with a low dihedral angle show no evidence of shrinking triple junction tubes, although most pores are surrounded by faceted pore walls. The faceted systems tend to produce more facet boundaries at the pore walls due to the difference of interfacial energies between the flat and curved surfaces. In the systems with the same degree of faceting, heterogeneity of liquid distribution tends to decrease with dihedral angle. For faceting systems, the permeability of texturally equilibrated rocks with low liquid fraction would be significantly decreased by the relative reduction of triple junction volumes or by closure of channels along grain edge due to the truncation of facet walls. 相似文献
17.
In the absence of an externally applied stress, the segregation of small amounts of granitic or tonalitic melts from their
residual mafic crystals is possible only if the melt forms an interconnected network phase. Accordingly, this research focuses
on melt connectivity at low melt fraction (<4 wt% or 5 vol.%). Connectivity of granitic and tonalitic melts in amphibole-rich
rock was assessed by performing two types of piston-cylinder experiments at 1 GPa and 800 °C. The first involved annealing
samples that consisted of either alternating layers or homogeneous mixtures of calcic amphibole and metaluminous obsidian
powder. The second type of experiment involved creating diffusion couples. Here, an upper cylinder of amphibole-saturated
granitic or tonalitic melt was placed against a lower cylinder consisting of an amphibole-rich rock containing zero or a small
melt (granitic or tonalitic) fraction. The upper part of the diffusion couple was doped with β emitter (151Sm or 14C) and functioned as an infinite melt reservoir. The lower part of the diffusion couple was considered to be the host rock.
The experiments approached textural equilibrium which allowed us to characterize the wetting behaviour of the calcic amphibole
by the hydrous silicic melt (granitic or tonalitic). These particular experiments also provided information concerning diffusive
transport, because the β emitter could diffuse through the connected melt (liquid) in the amphibole-rich rock. The dihedral
angle measurements show that melt connectivity was achieved. This conclusion is based on the fact that the dihedral angles,
θ, consistently yielded median apparent values of 53°<θ<58° for an amphibole-rich rock/granitic melt system, and 46°<θ<48°
for an amphibole-rich rock/tonalitic melt system. However, the frequency distribution of θ angles is found to be relatively
broad. The results of the diffusion-couple experiments, assessed using the β radiographic technique, complement the dihedral
(wetting) angle measurements by showing that melt connectivity is achieved at a melt fraction less than 4wt% (5 vol.%).
Received: 15 April 1997 / Accepted: 23 September 1998 相似文献
18.
Marian B. Holness 《Contributions to Mineralogy and Petrology》1995,118(4):356-364
An investigation was made of the effect of trace amounts of feldspar (Na and/or K) on dihedral angles in the quartz-H2O-CO2 system at 4 kbar and 450–1050°C. Quartz-quartz-H2O dihedral angles in feldspar-bearing quartz aggregates are observed to be the same as those in pure quartz aggregates at
temperatures below 500°C. Above this temperature, they decrease with increasing temperature until the solidus. The final angle
at the inception of melting is about 65° for microcline-quartz-H2O and microcline-albite-quartz-H2O, and much less than 60° (the critical value for formation of grain-edge fluid channels in an isotropic system) for the albite-quartz-H2O system. CO2 was observed to produce a constant quartz-quartz-fluid dihedral angle of 97° in feldspar-bearing quartz aggregates at all
temperatures studied. Also examined were the dihedral angles for the two co-existing supersolidus fluids in quartz aggregates.
In all systems the quartz-volatile fluid angle is greater than 60°, whereas the quartz-melt angle is lower than 60°. Both
super-solidus angles decrease with increasing temperature. The transition from nonconnected to connected poro- sity with increasing
temperature observed in the quartz-albite-H2O system some tens of degrees below the solidus (termed a permeability transition), if a common feature of rocks near their
melting points, will play an important role in controlling the permeability of high-grade rocks to aqueous fluids.
Received: 27 October 1993 / Accepted: 11 July 1994 相似文献
19.
《Journal of Structural Geology》2003,25(10):1597-1613
Intragranular microshear zones within a greenschist facies calcite marble were studied to try to constrain better the processes of dynamic recrystallization as well as the deformation processes that occur within newly recrystallized grains. Intragranular recrystallized grains within large, twinned calcite porphyroclasts can be related to the host from which they have recrystallized and are the focus of an electron backscatter diffraction study. Lattice distortions, low angle boundaries and some high angle boundaries (>15°) in the microshears within a porphyroclast have the same misorientation axes suggesting that deformation occurred by climb-accommodated dislocation creep involving subgrain rotation recrystallization. Changes in the ratio of host and twin domain, as the deformation zone is entered, show that twin boundary migration also occurred. Recrystallized grains have similar sizes (10–60 μm) to subgrains, suggesting that they formed by subgrain rotation. However, within the intragranular microshear zones the misorientations between recrystallized grains and porphyroclasts are considerably larger than 15° and misorientation axes are randomly oriented. Moreover recrystallized grain orientations average around the porphyroclast orientation. We suggest that the recrystallized grains, once formed, are able to deform partly by diffusion accommodated grain boundary sliding, which is consistent with predictions made from lab flow laws. 相似文献
20.
Melt must transfer through the lower crust, yet the field signatures and mechanisms involved in such transfer zones (excluding dykes) are still poorly understood. We report field and microstructural evidence of a deformation‐assisted melt transfer zone that developed in the lower crustal magmatic arc environment of Fiordland, New Zealand. A 30–40 m wide hornblende‐rich body comprising hornblende ± clinozoisite and/or garnet exhibits 'igneous‐like' features and is hosted within a metamorphic, two‐pyroxene–pargasite gabbroic gneiss (GG). Previous studies have interpreted the hornblende‐rich body as an igneous cumulate or a mass transfer zone. We present field and microstructural characteristics supporting the later and indicating the body has formed by deformation‐assisted, channelized, reactive porous melt flow. The host granulite facies GG contains distinctive rectilinear dykes and garnet reaction zones (GRZ) from earlier in the geological history; these form important reaction and strain markers. Field observations show that the mineral assemblages and microstructures of the GG and GRZ are progressively modified with proximity to the hornblende‐rich body. At the same time, GRZ bend systematically into the hornblende‐rich body on each side of the unit, showing apparent sinistral shearing. Within the hornblende‐rich body itself, microstructures and electron back‐scatter diffraction mapping show evidence of the former presence of melt including observations consistent with melt crystallization within pore spaces, elongate pseudomorphs of melt films along grain boundaries, minerals with low dihedral angles as small as <10° and up to <60°, and interconnected 3D melt pseudomorph networks. Reaction microstructures with highly irregular contact boundaries are observed at the field and thin‐section scale in remnant islands of original rock and replaced grains, respectively. We infer that the hornblende‐rich body was formed by modification of the host GG in situ due to reaction between an externally derived, reactive, hydrous gabbroic to intermediate melt percolating via porous melt flow through an actively deforming zone. Extensive melt–rock interaction and metasomatism occurred via coupled dissolution–precipitation, triggered by chemical disequilibrium between the host rock and the fluxing melt. As a result, the host plagioclase and pyroxene became unstable and were reacted and dissolved into the melt, while hornblende and to a lesser extent clinozoisite and garnet grew replacing the unstable phases. Our study shows that hornblendite rocks commonly observed within deep crustal sections, and attributed to cumulate fractionation processes, may instead delineate areas of deformation‐assisted, channelized reactive porous melt flow formed by melt‐mediated coupled dissolution–precipitation replacement reactions. 相似文献