腾冲火山研究综述

近３０年来，众多学对腾冲火山进行了大量的研究与考察工作，并在火山地质、地球化学、地热等方面取得了一批有价值的成果。本试图对部分有代表性的观点及研究成果进行综合性的介绍，供正在开展的《腾冲火山活动监测、预测与对策研究》重大项目的项专题研究参考。     

玄武质岩石的单颗粒锆石U-Pb年龄谱

报道了托云、东浮山、羊角、雪花山和山旺5处新生代玄武岩的SHRIMP锆石U-Pb测年结果。位于西南天山造山带的托云新生代玄武岩的14个测点年龄值十分发散,最大值与最小值分别为857.1和203.4Ma,它们与其余4件玄武岩样品49个SHRIMP锆石测点年龄一同构筑了涵盖各个地质时期几乎贯穿整个地质时间的复杂年龄谱。位于华北克拉通中部区域南太行山造山带的东浮山、羊角和雪花山新生代玄武岩3件样品累计36个锆石测点形成的锆石年龄谱相对简单,其中35个测点的年龄集中在1719.9～2641.6Ma,唯一的古生代年龄(311.3Ma)出现在雪花山玄武岩7.1测点。位于华北克拉通东部裂谷带内山旺玄武岩6件样品27个测点的单颗粒锆石年龄构筑的锆石年龄谱形成3个集中时间段,分别为新太古代—古元古代(2595.4～1852.2Ma)、古生代(385.8～271.1Ma)和中生代(109.4Ma)。3个年龄谱中大部分单颗粒锆石U-Pb年龄均能在各自所处区域内发现与之对应的岩浆-热事件,部分单颗粒锆石年龄可能暗示所在区域至今未发现的岩浆热事件,托云、东浮山-羊角-雪花山、山旺新生代玄武岩的复杂单颗粒锆石年龄谱再造了各自所处区域的地质演化史。3个锆石年龄谱的复杂程度与各自区域地表出露岩浆岩的规模和期次复杂程度相关,天山造山带内岩浆岩发育,托云玄武岩锆石年龄普最复杂,记录了天山造山带的演化,而华北克拉通中部区域南太行山造山带地表零星出露岩浆岩,东浮山-羊角-雪花山玄武岩的锆石年龄普最简单。处于后期遭受破坏改造的华北克拉通东部裂谷带内的山旺玄武岩的单颗粒锆石年龄谱,其复杂程度明显低于托云玄武岩的年龄谱,而又高于东浮山-羊角-雪花山玄武岩的年龄谱。鉴于玄武质岩浆同化混染围岩过程中能量消耗和地球化学印记以及玄武质岩浆上升的耗时限制,认为托云、东浮山、羊角、雪花山和山旺新生代玄武岩中具有复杂年龄信息的锆石捕掳晶不是玄武质岩浆在快速上升过程中从围岩中捕获的,而是在岩石圈拆沉过程中进入软流圈地幔中,随着具原生岩浆性质的玄武质岩浆喷发到达地表。     

数值模拟研究二叠纪峨眉山玄武岩浆在四川盆地的热效应

四川盆地是我国重要的含油气盆地,其西南部位于峨眉山大火成岩省的外带,二叠纪峨眉山玄武岩浆对四川盆地热历史及烃源岩热演化的影响一直备受关注.近年来,盆地古温标结果揭示出盆地在二叠纪存在高古热流（75~85 mW·m^-2）,甚至部分点位存在超高古热流（97~114 mW·m^-2）,被认为和峨眉山玄武岩浆的热效应有关.为了解这些高-超高古热流的成因机制,以及溢流到地表的玄武岩浆对二叠系及以下地层和烃源岩的热影响,本文采用二维有限元方法对二叠纪峨眉山玄武岩浆的热效应进行了模拟,得出如下结论：（1）置于岩石圈底部的地幔柱头高温异常体和挤入地壳底部的高温玄武岩浆在短期内（4 Ma内）对地表热流的扰动分别小于5 mW·m^-2和20 mW·m^-2,均无法解释四川盆地二叠纪的异常古热流.（2）古热流与侵入到地壳内部的岩浆有关,中心在7~17 km深度的不同形态的岩浆都有可能造成高或超高古热流的形成,引起超高古热流的水平状岩浆囊厚度在2~10 km,表层距地表在6~12 km之间.（3）地表岩浆越厚、下伏地层越浅,岩浆对该地层产生的热扰动越大,其中烃源岩所受影响也越大.如,上覆岩浆厚度为300 m时,在深度300 m（二叠系）、800 m（奥陶系）、1250 m（寒武系）、2000 m（震旦系）地层引起的最大升温分别是241℃、77℃、40℃和19℃,所需时间分别为2100年、6100年、1.17万年和2.56万年.（4）相变热的存在对二叠系和奥陶系地层不可忽略,如300 m厚岩浆产生的相变热可以使二叠系地层额外增温达55℃.

     

Miocene shallow-water limestones from São Nicolau (Cabo Verde): Caribbean-type benthic fauna and time constraints for volcanism

Shallow-water limestones of presumed Late Cretaceous and Eocene age, interbedded with basaltic lavas, were described by earlier authors from São Nicolau in the northwestern part of the Cabo Verde archipelago. If confirmed, these ages would imply late Mesozoic shallow-marine and subaerial volcanic activity in the Cabo Verde archipelago, and document a geological history very different from that known so far from other Cabo Verde Islands, from which no subaerial volcanic activity before the mid-Cenozoic is known. Our re-investigation of the foraminiferal fauna indicates a Late Miocene age for the presumed Late Cretaceous and Eocene limestones. The hypothesis of a long-lived hot spot, active by the Early Cretaceous, and of a major island-building stage in the Cabo Verde Islands during this period, is therefore not supported by the present bio- or chronostratigraphic data.     

A case of no-wind plinian fallout at Pululagua caldera (Ecuador): implications for models of clast dispersal

The caldera of Pululagua is an eruptive centre of the Northern Volcanic Zone of the South American volcanic arc, located about 15 km north of Quito, Ecuador. Activity leading to formation of the caldera occurred about 2450 b.p. as a series of volcanic episodes during which an estimated 5–6 km³ (DRE) of hornblende-bearing dacitic magma was erupted. A basal pumice-fall deposit covers more than 2.2x10⁴ km² with a volume of about 1.1 km³ and represents the principal and best-preserved plinian layer. Circular patterns of isopachs and pumice, lithic and Md isopleths of the Basal Fallout (BF) around the caldera indicate emplacement in wind-free conditions. Absence of wind is confirmed by an ubiquitous, normally graded, thin ash bed at the top of the lapilli layer which originated from slow settling of fines after cessation of the plinian column (co-plinian ash). The unusual atmospheric conditions during deposition make the BF deposit particularly suitable for the application and evaluation of pyroclast dispersal models. Application of the Carey and Sparks' (1986) model shows that whereas the 3.2-, 1.6-, and 0.8-cm lithic isopleths predict a model column height of about 36 km, the 6.4-cm isopleth yields and estimate of only 21 km. The 4.9- and 6.4-cm isopleths yield a column height of 28 km using the model of Wilson and Walker (1987). The two models give the same mass discharge rate of 2x10⁸ kg s^-1. A simple exponential decrease of thickness with distance, as proposed by Pyle (1989) for plinian falls, fits well with the BF. Exponential decrease of size with distance is followed by clasts less than about 3 cm, suggesting, in agreement with Wilson and Walker (1987), that only a small proportion of large clasts reach the top of the column. Variations with distance in clast distribution patterns imply that, in order to obtain column heights by clast dispersal models, the distribution should be known from both proximal and distal zones. Knowledge of only a few isopleths, irrespective of their distance from the vent, is not sufficient as seemed justified by the method of Pyle (1989).     

Permian volcanic rocks from the Apuseni Mountains (Romania): Geochemistry and tectonic constraints

An Early Permian volcanic assemblage is well exposed in the central-western part of the Apuseni Mountains (Romania). The rocks are represented by rhyolites, basalts and subordinate andesites suggesting a bimodal volcanic activity that is intimately associated with a post-orogenic (Variscan) syn-sedimentary intra-basinal continental molasse sequences. The mafic and mafic-intermediate rocks belong to sub-alkaline tholeiitic series were separated in three groups (I–III) showing a high Th and Pb abundances, depletion in Nb, Ta and Sr, and slightly enriched in LREE patterns (La_N/Yb_N = 1.4–4.4). Isotopically, the rocks of Group I have the initial ratios ⁸⁷Sr/⁸⁶Sr_(i) = 0.709351–0.707112, ¹⁴³Nd/¹⁴⁴Nd_(i) = 0.512490–0.512588 and high positive ?_Nd270 values from 3.9 to 5.80; the rocks of Group II present for the initial ratios values ⁸⁷Sr/⁸⁶Sr_(i) = 0.709434–0.710092, ¹⁴³Nd/¹⁴⁴Nd_(i) = 0.512231–0.512210 and for ?_Nd270 the negative values from −1.17 to −1.56; the rocks of Group III display for the initial ratios the values ⁸⁷Sr/⁸⁶Sr_(i) = 0.710751–0.709448, ¹⁴³Nd/¹⁴⁴Nd_(i) = 0.512347–0.512411 and for ?_Nd270 the positive values from 1.64 to 2.35. The rocks resembling continental tholeiites, suggest a mantle origin and were further affected by fractionation and crustal contamination. In addition, the REE geochemistry (1 > Sm_N/Yb_N < 2.5; 0.9 > La_N/Sm_N < 2.5) suggests that these rocks were generated by high percentage partial melting of a metasomatized mantle in the garnet peridotite facies. The felsic rocks are enriched in Cs, Rb Th and U and depleted in Nb, Ta, Sr, Eu, and Ti. The REE fractionation patterns show a strong negative Eu anomaly (Eu/Eu* = 0.23–0.40). The felsic rocks show the initial ratios the values: ⁸⁷Sr/⁸⁶Sr_(i) = 0.704096–0.707805, ¹⁴³Nd/¹⁴⁴Nd_(i) = 0.512012–0.512021 and for ?_Nd270 the negative values from −5.27 to −5.44. They suggest to be generated within the lower crust during the emplacement of mantle-derived magmas that provided necessary heat to crustal partial melting.     

Early Cretaceous trachybasalt-trachyte-trachyrhyolitic volcanism in the Nyalga basin (Central Mongolia): sources and evolution of continental rift magmas

As shown by geological, mineralogical, and isotope geochemical data, trachybasaltic-trachytic-trachyrhyolitic (TTT) rocks from the Nyalga basin in Central Mongolia result from several eruptions of fractionated magmas within a short time span at about 120 Ma. Their parental basaltic melts formed by partial melting of mantle peridotite which was metasomatized and hydrated during previous subduction events. Basaltic trachyandesites have high TiO₂ and K₂O, relatively high P₂O₅, and low MgO contents, medium ⁸⁷Sr/⁸⁶Sr(₀) ratios (0.70526-0.70567), and almost zero or slightly negative ε_Nd(T) values. The isotope geochemical signatures of TTT rocks are typical of Late Mesozoic basaltic rocks from rift zones of Mongolia and Transbaikalia. The sources of basaltic magma at volcanic centers of Northern and Central Asia apparently moved from a shallower and more hydrous region to deeper and less hydrated lithospheric mantle (from spinel to garnet-bearing peridotite) between the Late Paleozoic and the latest Mesozoic. The geochemistry and mineralogy of TTT rocks fit the best models implying fractional crystallization of basaltic trachyandesitic, trachytic, and trachyrhyodacitic magmas. Mass balance calculations indicate that trachytic and trachydacitic magmas formed after crystallization of labradorite-andesine, Ti-augite, Sr-apatite, Ti-magnetite, and ilmenite from basaltic trachyandesitic melts. The melts evolved from trachytic to trachyrhyodacitic and trachyrhyolitic compositions as a result of prevalent crystallization of K-Na feldspar, with zircon, chevkinite-Ce, and LREE-enriched apatite involved in fractionation. Trachytic, trachyrhyodacitic, and trachyrhyolitic residual melts were produced by the evolution of compositionally different parental melts (basaltic trachyandesitic, trachytic, and trachyrhyodacitic, respectively), which moved to shallower continental crust and accumulated in isolated chambers. Judging by their isotopic signatures, the melts assimilated some crustal material, according to the assimilation and fractional crystallization (AFC) model.     

Opaque Mineralogy as a Tracer of Magmatic History of Volcanic Rocks:an Example from the Neogene-Quaternary Harrat Rahat Intercontinental Volcanic Field, North Western Saudi Arabia

The Neogene-Quaternary Harrat Rahat volcanic field is part of the major intercontinental Harrat fields in western Saudi Arabia.It comprises lava flows of olivine basalt and hawaiite,in addition to mugearite,benmorite,and trachyte that occur mainly as domes,tuff cones and lava flows.Based on opaque mineralogy and mineral chemistry,the Harrat Rahat volcanic varieties are distinguished into Group I(olivine basalt and hawaiite) and Group II(mugearite,benmorite and trachyte).The maximum forsterite content(~85) is encountered in zoned forsteritic olivine of Group I,whereas olivine of Group II is characterized by intermediate(Fo=50),fayalitic(Fo=25) and pure fayalite in the mugearite,benmorite and trachyte,respectively.The more evolved varieties of Group II contain minerals that show enrichment of Fe2+,Mn2+and Na+that indicates normal fractional crystallization.The common occurrence of coarse apatite with titanomagnetite in the benmorite indicates that P5+becomes saturated in this rock variety and drops again in trachyte.Cr-spinel is recorded in Group I varieties only and the Cr#(0.5) suggests lherzolite as a possible restite of the Harrat Rahat volcanics.The plots of Cr# vs.the forsterite content(Fo) suggest two distinct trends,which are typical of mixing of two basaltic magmas of different sources and different degrees of partial melting.The bimodality of Harrat Rahat Cr-spinel suggests possible derivation from recycled MORB slab in the mantle as indicated by the presence of high-Al spinel.It is believed that the subcontinental lithospheric mantle was modified by pervious subduction process and played the leading role in the genesis of the Harrat Rahat intraplate volcanics.The trachytes of the Harrat Rahat volcanic field were formed most probably by melting of a lower crust at the mantle-crust boundary.The increase in fO2 causes a decrease in Cr2 O3,and Al2 O3,and a strong increase in the proportion of Fe3+and Mg# of spinel crystallizing from the basaltic melt at T ~1200°C.The olivine-pyroxene and olivine-spinel geothermometers yielded equilibrium temperature in the range of 935-1025°C,whereas the range of <500-850°C from single-pyroxene thermometry indicates either post crystallization reequilibrium of the clinopyroxene,or the mineral is xenocrystic and re-equilibrated in a cooling basaltic magma.     

Facies architecture of the Early Devonian Ural Volcanics,New South Wales

The Ural Volcanics are a early Devonian, submarine, felsic lava-sill complex, exposed in the western central Lachlan Orogen, New South Wales. The Ural Volcanics and underlying Upper Silurian, deepwater, basin-fill sedimentary rocks make up the Rast Group. The Ural Range study area, centrally located in the Cargelligo 1:100 000 map sheet area, was mapped at 1:10 000 scale. Seventeen principal volcanic facies were identified in the study area, dominated by felsic coherent facies (rhyolite and dacite) and associated monomictic breccia and siltstone-matrix monomictic breccia facies. Subordinate volcaniclastic facies include the pumice-rich breccia facies association, rhyolite – dacite – siltstone breccia facies and fiamme – siltstone breccia facies. The sedimentary facies association includes mixed-provenance and non-volcanic sandstone to conglomerate, black mudstone, micaceous quartz sandstone and foliated mudstone. The succession was derived from at least two intrabasinal volcanic centres. One, in the north, was largely effusive and intrusive, building a lava – sill complex. Another, in the south, was effusive, intrusive and explosive, generating lavas and moderate-volume (～3 km³) pyroclastic facies. The presence of turbidites, marine fossils, very thick massive to graded volcaniclastic units and black mudstone, and the lack of large-scale cross-beds and erosional scours, provide evidence for deposition in a submarine environment below storm wave-base. The Ural Volcanics have potential for seafloor or sub-seafloor replacement massive sulfide deposits, although no massive sulfide prospects or related altered zones have yet been defined. Sparse, disseminated sulfides occur in sericite-altered, steeply dipping shear zones.     

桂北—湘南中生代玄武质岩石及其深源包体的地球化学性质和岩石成因探讨

桂北-湘南中生代玄武质岩石中含有丰富的深源包体，它们分别为橄榄岩、变形的辉长岩和中酸性片麻岩三大类，本文在论述上述岩石地球化学性质的基础上，探讨了它们之间的成因关系；寄主的中生代玄武质岩石为地幔楣榄岩部分熔融的产物，与辉长岩和中酸性片麻岩并无成因联系，后者属偶然包体，值得注意的是，深源包体中的变形辉长岩与片麻岩之间为分离结晶的成因关系，它们均为元古宙壳、幔间底侵玄武质岩浆的演化产物，其中辉长岩为底侵岩浆的堆积相，而片麻岩则为底侵岩浆经历分离结晶的堆积作用之后所剩下的残余岩浆的变质产物。